Since C++ is based on C, you must be familiar with the syntax of C in order to program in C++, just as you
must be reasonably fluent in algebra in order to tackle calculus.

If you’ve never seen C before, this chapter will give you a decent background in the style of C used in C++. If you are familiar with the style of C described in the first edition of Kernighan & Ritchie (often called K&R C), you will find some new and different features in C++ as well as in Standard C. If you are familiar with Standard C, you should skim through this chapter looking for features that are particular to C++. Note that there are some fundamental C++ features introduced here, which are basic ideas that are akin to the features in C or often modifications to the way that C does things. The more sophisticated C++ features will not be introduced until later chapters.

This chapter is a fairly fast coverage of C constructs and introduction to some basic C++ constructs, with the understanding that you’ve had some experience programming in another language. A more gentle introduction to C is found in the CD ROM packaged in the back of this book, titled Thinking in C: Foundations for Java & C++ by Chuck Allison (published by MindView, Inc., and also available at www.MindView.net). This is a seminar on a CD ROM with the goal of taking you carefully through the fundamentals of the C language. It focuses on the knowledge necessary for you to be able to move on to the C++ or Java languages rather than trying to make you an expert in all the dark corners of C (one of the reasons for using a higher-level language like C++ or Java is precisely so we can avoid many of these dark corners). It also contains exercises and guided solutions. Keep in mind that because this chapter goes beyond the Thinking in C CD, the CD is not a replacement for this chapter, but should be used instead as a preparation for this chapter and for the book.

In old (pre-Standard) C, you could call a function with any number or type of arguments and the compiler wouldn’t complain. Everything seemed fine until you ran the program. You got mysterious results (or worse, the program crashed) with no hints as to why. The lack of help with argument passing and the enigmatic bugs that resulted is probably one reason why C was dubbed a “high-level assembly language.” Pre-Standard C programmers just adapted to it.

Standard C and C++ use a feature called function prototyping. With function prototyping, you must use a description of the types of arguments when declaring and defining a function. This description is the “prototype.” When the function is called, the compiler uses the prototype to ensure that the proper arguments are passed in and that the return value is treated correctly. If the programmer makes a mistake when calling the function, the compiler catches the mistake.

Essentially, you learned about function prototyping (without naming it as such) in the previous chapter, since the form of function declaration in C++ requires proper prototyping. In a function prototype, the argument list contains the types of arguments that must be passed to the function and (optionally for the declaration) identifiers for the arguments. The order and type of the arguments must match in the declaration, definition, and function call. Here’s an example of a function prototype in a declaration:

You do not use the same form when declaring variables in function prototypes as you do in ordinary variable definitions. That is, you cannot say: float x, y, z. You must indicate the type of each argument. In a function declaration, the following form is also acceptable:

Since the compiler doesn’t do anything but check for types when the function is called, the identifiers are only included for clarity when someone is reading the code.

In the function definition, names are required because the arguments are referenced inside the function:

It turns out this rule applies only to C. In C++, an argument may be unnamed in the argument list of the function definition. Since it is unnamed, you cannot use it in the function body, of course. Unnamed arguments are allowed to give the programmer a way to “reserve space in the argument list.” Whoever uses the function must still call the function with the proper arguments. However, the person creating the function can then use the argument in the future without forcing modification of code that calls the function. This option of ignoring an argument in the list is also possible if you leave the name in, but you will get an annoying warning message about the value being unused every time you compile the function. The warning is eliminated if you remove the name.

C and C++ have two other ways to declare an argument list. If you have an empty argument list, you can declare it as func( ) in C++, which tells the compiler there are exactly zero arguments. You should be aware that this only means an empty argument list in C++. In C it means “an indeterminate number of arguments (which is a “hole” in C since it disables type checking in that case). In both C and C++, the declaration func(void); means an empty argument list. The void keyword means “nothing” in this case (it can also mean “no type” in the case of pointers, as you’ll see later in this chapter).

The other option for argument lists occurs when you don’t know how many arguments or what type of arguments you will have; this is called a variable argument list. This “uncertain argument list” is represented by ellipses (...). Defining a function with a variable argument list is significantly more complicated than defining a regular function. You can use a variable argument list for a function that has a fixed set of arguments if (for some reason) you want to disable the error checks of function prototyping. Because of this, you should restrict your use of variable argument lists to C and avoid them in C++ (in which, as you’ll learn, there are much better alternatives). Handling variable argument lists is described in the library section of your local C guide.

A C++ function prototype must specify the return value type of the function (in C, if you leave off the return value type it defaults to int). The return type specification precedes the function name. To specify that no value is returned, use the void keyword. This will generate an error if you try to return a value from the function. Here are some complete function prototypes:

To return a value from a function, you use the return statement. return exits the function back to the point right after the function call. If return has an argument, that argument becomes the return value of the function. If a function says that it will return a particular type, then each return statement must return that type. You can have more than one return statement in a function definition:

In cfunc( ), the first if that evaluates to true exits the function via the return statement. Notice that a function declaration is not necessary because the function definition appears before it is used in main( ), so the compiler knows about it from that function definition.

All the functions in your local C function library are available while you are programming in C++. You should look hard at the function library before defining your own function – there’s a good chance that someone has already solved your problem for you, and probably given it a lot more thought and debugging.

A word of caution, though: many compilers include a lot of extra functions that make life even easier and are tempting to use, but are not part of the Standard C library. If you are certain you will never want to move the application to another platform (and who is certain of that?), go ahead –use those functions and make your life easier. If you want your application to be portable, you should restrict yourself to Standard library functions. If you must perform platform-specific activities, try to isolate that code in one spot so it can be changed easily when porting to another platform. In C++, platform-specific activities are often encapsulated in a class, which is the ideal solution.

The formula for using a library function is as follows: first, find the function in your programming reference (many programming references will index the function by category as well as alphabetically). The description of the function should include a section that demonstrates the syntax of the code. The top of this section usually has at least one #include line, showing you the header file containing the function prototype. Duplicate this #include line in your file so the function is properly declared. Now you can call the function in the same way it appears in the syntax section. If you make a mistake, the compiler will discover it by comparing your function call to the function prototype in the header and tell you about your error. The linker searches the Standard library by default, so that’s all you need to do: include the header file and call the function.

You can collect your own functions together into a library. Most programming packages come with a librarian that manages groups of object modules. Each librarian has its own commands, but the general idea is this: if you want to create a library, make a header file containing the function prototypes for all the functions in your library. Put this header file somewhere in the preprocessor’s search path, either in the local directory (so it can be found by #include "header") or in the include directory (so it can be found by #include <header>). Now take all the object modules and hand them to the librarian along with a name for the finished library (most librarians require a common extension, such as .lib or .a). Place the finished library where the other libraries reside so the linker can find it. When you use your library, you will have to add something to the command line so the linker knows to search the library for the functions you call. You must find all the details in your local manual, since they vary from system to system.

This section covers the execution control statements in C++. You must be familiar with these statements before you can read and write C or C++ code.

C++ uses all of C’s execution control statements. These include if-else, while, do-while, for, and a selection statement called switch. C++ also allows the infamous goto, which will be avoided in this book.

All conditional statements use the truth or falsehood of a conditional expression to determine the execution path. An example of a conditional expression is A == B. This uses the conditional operator == to see if the variable A is equivalent to the variable B. The expression produces a Boolean true or false (these are keywords only in C++; in C an expression is “true” if it evaluates to a nonzero value). Other conditional operators are >, <, >=, etc. Conditional statements are covered more fully later in this chapter.

The if-else statement can exist in two forms: with or without the else. The two forms are:

or

The “expression” evaluates to true or false. The “statement” means either a simple statement terminated by a semicolon or a compound statement, which is a group of simple statements enclosed in braces. Any time the word “statement” is used, it always implies that the statement is simple or compound. Note that this statement can also be another if, so they can be strung together.

It is conventional to indent the body of a control flow statement so the reader may easily determine where it begins and ends[30].

while, do-while, and for control looping. A statement repeats until the controlling expression evaluates to false. The form of a while loop is

The expression is evaluated once at the beginning of the loop and again before each further iteration of the statement.

This example stays in the body of the while loop until you type the secret number or press control-C.

The while’s conditional expression is not restricted to a simple test as in the example above; it can be as complicated as you like as long as it produces a true or false result. You will even see code where the loop has no body, just a bare semicolon:

In these cases, the programmer has written the conditional expression not only to perform the test but also to do the work.

The form of do-while is

The do-while is different from the while because the statement always executes at least once, even if the expression evaluates to false the first time. In a regular while, if the conditional is false the first time the statement never executes.

If a do-while is used in Guess.cpp, the variable guess does not need an initial dummy value, since it is initialized by the cin statement before it is tested:

For some reason, most programmers tend to avoid do-while and just work with while.

A for loop performs initialization before the first iteration. Then it performs conditional testing and, at the end of each iteration, some form of “stepping.” The form of the for loop is:

Any of the expressions initialization, conditional, or step may be empty. The initialization code executes once at the very beginning. The conditional is tested before each iteration (if it evaluates to false at the beginning, the statement never executes). At the end of each loop, the step executes.

for loops are usually used for “counting” tasks:

You may notice that the variable i is defined at the point where it is used, instead of at the beginning of the block denoted by the open curly brace ‘{’. This is in contrast to traditional procedural languages (including C), which require that all variables be defined at the beginning of the block. This will be discussed later in this chapter.

Inside the body of any of the looping constructs while, do-while, or for, you can control the flow of the loop using break and continue. break quits the loop without executing the rest of the statements in the loop. continue stops the execution of the current iteration and goes back to the beginning of the loop to begin a new iteration.

As an example of break and continue, this program is a very simple menu system:

If the user selects ‘q’ in the main menu, the break keyword is used to quit, otherwise the program just continues to execute indefinitely. After each of the sub-menu selections, the continue keyword is used to pop back up to the beginning of the while loop.

The while(true) statement is the equivalent of saying “do this loop forever.” The break statement allows you to break out of this infinite while loop when the user types a ‘q.’

A switch statement selects from among pieces of code based on the value of an integral expression. Its form is:

Selector is an expression that produces an integral value. The switch compares the result of selector to each integral value. If it finds a match, the corresponding statement (simple or compound) executes. If no match occurs, the default statement executes.

You will notice in the definition above that each case ends with a break, which causes execution to jump to the end of the switch body (the closing brace that completes the switch). This is the conventional way to build a switch statement, but the break is optional. If it is missing, your case “drops through” to the one after it. That is, the code for the following case statements execute until a break is encountered. Although you don’t usually want this kind of behavior, it can be useful to an experienced programmer.

The switch statement is a clean way to implement multi-way selection (i.e., selecting from among a number of different execution paths), but it requires a selector that evaluates to an integral value at compile-time. If you want to use, for example, a string object as a selector, it won’t work in a switch statement. For a string selector, you must instead use a series of if statements and compare the string inside the conditional.

The menu example shown above provides a particularly nice example of a switch:

The quit flag is a bool, short for “Boolean,” which is a type you’ll find only in C++. It can have only the keyword values true or false. Selecting ‘q’ sets the quit flag to true. The next time the selector is evaluated, quit == false returns false so the body of the while does not execute.

The goto keyword is supported in C++, since it exists in C. Using goto is often dismissed as poor programming style, and most of the time it is. Anytime you use goto, look at your code and see if there’s another way to do it. On rare occasions, you may discover goto can solve a problem that can’t be solved otherwise, but still, consider it carefully. Here’s an example that might make a plausible candidate:

The alternative would be to set a Boolean that is tested in the outer for loop, and then do a break from the inner for loop. However, if you have several levels of for or while this could get awkward.

Recursion is an interesting and sometimes useful programming technique whereby you call the function that you’re in. Of course, if this is all you do, you’ll keep calling the function you’re in until you run out of memory, so there must be some way to “bottom out” the recursive call. In the following example, this “bottoming out” is accomplished by simply saying that the recursion will go only until the cat exceeds ‘Z’:[31]

In removeHat( ), you can see that as long as cat is less than ‘Z’, removeHat( ) will be called from within removeHat( ), thus effecting the recursion. Each time removeHat( ) is called, its argument is one greater than the current cat so the argument keeps increasing.

Recursion is often used when evaluating some sort of arbitrarily complex problem, since you aren’t restricted to a particular “size” for the solution – the function can just keep recursing until it’s reached the end of the problem.

You can think of operators as a special type of function (you’ll learn that C++ operator overloading treats operators precisely that way). An operator takes one or more arguments and produces a new value. The arguments are in a different form than ordinary function calls, but the effect is the same.

From your previous programming experience, you should be reasonably comfortable with the operators that have been used so far. The concepts of addition (+), subtraction and unary minus (-), multiplication (*), division (/), and assignment(=) all have essentially the same meaning in any programming language. The full set of operators is enumerated later in this chapter.

Operator precedence defines the order in which an expression evaluates when several different operators are present. C and C++ have specific rules to determine the order of evaluation. The easiest to remember is that multiplication and division happen before addition and subtraction. After that, if an expression isn’t transparent to you it probably won’t be for anyone reading the code, so you should use parentheses to make the order of evaluation explicit. For example:

has a very different meaning from the same statement with a particular grouping of parentheses:

(Try evaluating the result with X = 1, Y = 2, and Z = 3.)

C, and therefore C++, is full of shortcuts. Shortcuts can make code much easier to type, and sometimes much harder to read. Perhaps the C language designers thought it would be easier to understand a tricky piece of code if your eyes didn’t have to scan as large an area of print.

One of the nicer shortcuts is the auto-increment and auto-decrement operators. You often use these to change loop variables, which control the number of times a loop executes.

The auto-decrement operator is ‘--’ and means “decrease by one unit.” The auto-increment operator is ‘++’ and means “increase by one unit.” If A is an int, for example, the expression ++A is equivalent to (A = A + 1). Auto-increment and auto-decrement operators produce the value of the variable as a result. If the operator appears before the variable, (i.e., ++A), the operation is first performed and the resulting value is produced. If the operator appears after the variable (i.e. A++), the current value is produced, and then the operation is performed. For example:

If you’ve been wondering about the name “C++,” now you understand. It implies “one step beyond C.”

Data types define the way you use storage (memory) in the programs you write. By specifying a data type, you tell the compiler how to create a particular piece of storage, and also how to manipulate that storage.

Data types can be built-in or abstract. A built-in data type is one that the compiler intrinsically understands, one that is wired directly into the compiler. The types of built-in data are almost identical in C and C++. In contrast, a user-defined data type is one that you or another programmer create as a class. These are commonly referred to as abstract data types. The compiler knows how to handle built-in types when it starts up; it “learns” how to handle abstract data types by reading header files containing class declarations (you’ll learn about this in later chapters).

The Standard C specification for built-in types (which C++ inherits) doesn’t say how many bits each of the built-in types must contain. Instead, it stipulates the minimum and maximum values that the built-in type must be able to hold. When a machine is based on binary, this maximum value can be directly translated into a minimum number of bits necessary to hold that value. However, if a machine uses, for example, binary-coded decimal (BCD) to represent numbers, then the amount of space in the machine required to hold the maximum numbers for each data type will be different. The minimum and maximum values that can be stored in the various data types are defined in the system header files limits.h and float.h (in C++ you will generally #include <climits> and <cfloat> instead).

C and C++ have four basic built-in data types, described here for binary-based machines. A char is for character storage and uses a minimum of 8 bits (one byte) of storage, although it may be larger. An int stores an integral number and uses a minimum of two bytes of storage. The float and double types store floating-point numbers, usually in IEEE floating-point format. float is for single-precision floating point and double is for double-precision floating point.

As mentioned previously, you can define variables anywhere in a scope, and you can define and initialize them at the same time. Here’s how to define variables using the four basic data types:

The first part of the program defines variables of the four basic data types without initializing them. If you don’t initialize a variable, the Standard says that its contents are undefined (usually, this means they contain garbage). The second part of the program defines and initializes variables at the same time (it’s always best, if possible, to provide an initialization value at the point of definition). Notice the use of exponential notation in the constant 6e-4, meaning “6 times 10 to the minus fourth power.”

Before bool became part of Standard C++, everyone tended to use different techniques in order to produce Boolean-like behavior. These produced portability problems and could introduce subtle errors.

The Standard C++ bool type can have two states expressed by the built-in constants true (which converts to an integral one) and false (which converts to an integral zero). All three names are keywords. In addition, some language elements have been adapted:

Because there’s a lot of existing code that uses an int to represent a flag, the compiler will implicitly convert from an int to a bool (nonzero values will produce true while zero values produce false). Ideally, the compiler will give you a warning as a suggestion to correct the situation.

An idiom that falls under “poor programming style” is the use of ++ to set a flag to true. This is still allowed, but deprecated, which means that at some time in the future it will be made illegal. The problem is that you’re making an implicit type conversion from bool to int, incrementing the value (perhaps beyond the range of the normal bool values of zero and one), and then implicitly converting it back again.

Pointers (which will be introduced later in this chapter) will also be automatically converted to bool when necessary.

Specifiers modify the meanings of the basic built-in types and expand them to a much larger set. There are four specifiers: long, short, signed, and unsigned.

long and short modify the maximum and minimum values that a data type will hold. A plain int must be at least the size of a short. The size hierarchy for integral types is: short int, int, long int. All the sizes could conceivably be the same, as long as they satisfy the minimum/maximum value requirements. On a machine with a 64-bit word, for instance, all the data types might be 64 bits.

The size hierarchy for floating point numbers is: float, double, and long double. “long float” is not a legal type. There are no short floating-point numbers.

The signed and unsigned specifiers tell the compiler how to use the sign bit with integral types and characters (floating-point numbers always contain a sign). An unsigned number does not keep track of the sign and thus has an extra bit available, so it can store positive numbers twice as large as the positive numbers that can be stored in a signed number. signed is the default and is only necessary with char; char may or may not default to signed. By specifying signed char, you force the sign bit to be used.

The following example shows the size of the data types in bytes by using the sizeof operator, introduced later in this chapter:

Be aware that the results you get by running this program will probably be different from one machine/operating system/compiler to the next, since (as mentioned previously) the only thing that must be consistent is that each different type hold the minimum and maximum values specified in the Standard.

When you are modifying an int with short or long, the keyword int is optional, as shown above.

Whenever you run a program, it is first loaded (typically from disk) into the computer’s memory. Thus, all elements of your program are located somewhere in memory. Memory is typically laid out as a sequential series of memory locations; we usually refer to these locations as eight-bit bytes but actually the size of each space depends on the architecture of the particular machine and is usually called that machine’s word size. Each space can be uniquely distinguished from all other spaces by its address. For the purposes of this discussion, we’ll just say that all machines use bytes that have sequential addresses starting at zero and going up to however much memory you have in your computer.

Since your program lives in memory while it’s being run, every element of your program has an address. Suppose we start with a simple program:

Each of the elements in this program has a location in storage when the program is running. Even the function occupies storage. As you’ll see, it turns out that what an element is and the way you define it usually determines the area of memory where that element is placed.

There is an operator in C and C++ that will tell you the address of an element. This is the ‘&’ operator. All you do is precede the identifier name with ‘&’ and it will produce the address of that identifier. YourPets1.cpp can be modified to print out the addresses of all its elements, like this:

The (long) is a cast. It says “Don’t treat this as if it’s normal type, instead treat it as a long.” The cast isn’t essential, but if it wasn’t there, the addresses would have been printed out in hexadecimal instead, so casting to a long makes things a little more readable.

The results of this program will vary depending on your computer, OS, and all sorts of other factors, but it will always give you some interesting insights. For a single run on my computer, the results looked like this:

You can see how the variables that are defined inside main( ) are in a different area than the variables defined outside of main( ); you’ll understand why as you learn more about the language. Also, f( ) appears to be in its own area; code is typically separated from data in memory.

Another interesting thing to note is that variables defined one right after the other appear to be placed contiguously in memory. They are separated by the number of bytes that are required by their data type. Here, the only data type used is int, and cat is four bytes away from dog, bird is four bytes away from cat, etc. So it would appear that, on this machine, an int is four bytes long.

Other than this interesting experiment showing how memory is mapped out, what can you do with an address? The most important thing you can do is store it inside another variable for later use. C and C++ have a special type of variable that holds an address. This variable is called a pointer.

The operator that defines a pointer is the same as the one used for multiplication: ‘*’. The compiler knows that it isn’t multiplication because of the context in which it is used, as you will see.

When you define a pointer, you must specify the type of variable it points to. You start out by giving the type name, then instead of immediately giving an identifier for the variable, you say “Wait, it’s a pointer” by inserting a star between the type and the identifier. So a pointer to an int looks like this:

The association of the ‘*’ with the type looks sensible and reads easily, but it can actually be a bit deceiving. Your inclination might be to say “intpointer” as if it is a single discrete type. However, with an int or other basic data type, it’s possible to say:

whereas with a pointer, you’d like to say:

C syntax (and by inheritance, C++ syntax) does not allow such sensible expressions. In the definitions above, only ipa is a pointer, but ipb and ipc are ordinary ints (you can say that “* binds more tightly to the identifier”). Consequently, the best results can be achieved by using only one definition per line; you still get the sensible syntax without the confusion:

Since a general guideline for C++ programming is that you should always initialize a variable at the point of definition, this form actually works better. For example, the variables above are not initialized to any particular value; they hold garbage. It’s much better to say something like:

Now both a and ipa have been initialized, and ipa holds the address of a.

Once you have an initialized pointer, the most basic thing you can do with it is to use it to modify the value it points to. To access a variable through a pointer, you dereference the pointer using the same operator that you used to define it, like this:

Now a contains the value 100 instead of 47.

These are the basics of pointers: you can hold an address, and you can use that address to modify the original variable. But the question still remains: why do you want to modify one variable using another variable as a proxy?

For this introductory view of pointers, we can put the answer into two broad categories:

Ordinarily, when you pass an argument to a function, a copy of that argument is made inside the function. This is referred to as pass-by-value. You can see the effect of pass-by-value in the following program:

In f( ), a is a local variable, so it exists only for the duration of the function call to f( ). Because it’s a function argument, the value of a is initialized by the arguments that are passed when the function is called; in main( ) the argument is x, which has a value of 47, so this value is copied into a when f( ) is called.

When you run this program you’ll see:

Initially, of course, x is 47. When f( ) is called, temporary space is created to hold the variable a for the duration of the function call, and a is initialized by copying the value of x, which is verified by printing it out. Of course, you can change the value of a and show that it is changed. But when f( ) is completed, the temporary space that was created for a disappears, and we see that the only connection that ever existed between a and x happened when the value of x was copied into a.

When you’re inside f( ), x is the outside object (my terminology), and changing the local variable does not affect the outside object, naturally enough, since they are two separate locations in storage. But what if you do want to modify the outside object? This is where pointers come in handy. In a sense, a pointer is an alias for another variable. So if we pass a pointer into a function instead of an ordinary value, we are actually passing an alias to the outside object, enabling the function to modify that outside object, like this:

Now f( ) takes a pointer as an argument and dereferences the pointer during assignment, and this causes the outside object x to be modified. The output is:

Notice that the value contained in p is the same as the address of x – the pointer p does indeed point to x. If that isn’t convincing enough, when p is dereferenced to assign the value 5, we see that the value of x is now changed to 5 as well.

Thus, passing a pointer into a function will allow that function to modify the outside object. You’ll see plenty of other uses for pointers later, but this is arguably the most basic and possibly the most common use.

Pointers work roughly the same in C and in C++, but C++ adds an additional way to pass an address into a function. This is pass-by-reference and it exists in several other programming languages so it was not a C++ invention.

Your initial perception of references may be that they are unnecessary, that you could write all your programs without references. In general, this is true, with the exception of a few important places that you’ll learn about later in the book. You’ll also learn more about references later, but the basic idea is the same as the demonstration of pointer use above: you can pass the address of an argument using a reference. The difference between references and pointers is that calling a function that takes references is cleaner, syntactically, than calling a function that takes pointers (and it is exactly this syntactic difference that makes references essential in certain situations). If PassAddress.cpp is modified to use references, you can see the difference in the function call in main( ):

In f( )’s argument list, instead of saying int* to pass a pointer, you say int& to pass a reference. Inside f( ), if you just say ‘r’ (which would produce the address if r were a pointer) you get the value in the variable that r references. If you assign to r, you actually assign to the variable that r references. In fact, the only way to get the address that’s held inside r is with the ‘&’ operator.

In main( ), you can see the key effect of references in the syntax of the call to f( ), which is just f(x). Even though this looks like an ordinary pass-by-value, the effect of the reference is that it actually takes the address and passes it in, rather than making a copy of the value. The output is:

So you can see that pass-by-reference allows a function to modify the outside object, just like passing a pointer does (you can also observe that the reference obscures the fact that an address is being passed; this will be examined later in the book). Thus, for this simple introduction you can assume that references are just a syntactically different way (sometimes referred to as “syntactic sugar”) to accomplish the same thing that pointers do: allow functions to change outside objects.

So far, you’ve seen the basic data types char, int, float, and double, along with the specifiers signed, unsigned, short, and long, which can be used with the basic data types in almost any combination. Now we’ve added pointers and references that are orthogonal to the basic data types and specifiers, so the possible combinations have just tripled:

Pointers and references also work when passing objects into and out of functions; you’ll learn about this in a later chapter.

There’s one other type that works with pointers: void. If you state that a pointer is a void*, it means that any type of address at all can be assigned to that pointer (whereas if you have an int*, you can assign only the address of an int variable to that pointer). For example:

Once you assign to a void* you lose any information about what type it is. This means that before you can use the pointer, you must cast it to the correct type:

The cast (int*)vp takes the void* and tells the compiler to treat it as an int*, and thus it can be successfully dereferenced. You might observe that this syntax is ugly, and it is, but it’s worse than that – the void* introduces a hole in the language’s type system. That is, it allows, or even promotes, the treatment of one type as another type. In the example above, I treat an int as an int by casting vp to an int*, but there’s nothing that says I can’t cast it to a char* or double*, which would modify a different amount of storage that had been allocated for the int, possibly crashing the program. In general, void pointers should be avoided, and used only in rare special cases, the likes of which you won’t be ready to consider until significantly later in the book.

You cannot have a void reference, for reasons that will be explained in Chapter 11.

Scoping rules tell you where a variable is valid, where it is created, and where it gets destroyed (i.e., goes out of scope). The scope of a variable extends from the point where it is defined to the first closing brace that matches the closest opening brace before the variable was defined. That is, a scope is defined by its “nearest” set of braces. To illustrate:

The example above shows when variables are visible and when they are unavailable (that is, when they go out of scope). A variable can be used only when inside its scope. Scopes can be nested, indicated by matched pairs of braces inside other matched pairs of braces. Nesting means that you can access a variable in a scope that encloses the scope you are in. In the example above, the variable scp1 is available inside all of the other scopes, while scp3 is available only in the innermost scope.

As noted earlier in this chapter, there is a significant difference between C and C++ when defining variables. Both languages require that variables be defined before they are used, but C (and many other traditional procedural languages) forces you to define all the variables at the beginning of a scope, so that when the compiler creates a block it can allocate space for those variables.

While reading C code, a block of variable definitions is usually the first thing you see when entering a scope. Declaring all variables at the beginning of the block requires the programmer to write in a particular way because of the implementation details of the language. Most people don’t know all the variables they are going to use before they write the code, so they must keep jumping back to the beginning of the block to insert new variables, which is awkward and causes errors. These variable definitions don’t usually mean much to the reader, and they actually tend to be confusing because they appear apart from the context in which they are used.

C++ (not C) allows you to define variables anywhere in a scope, so you can define a variable right before you use it. In addition, you can initialize the variable at the point you define it, which prevents a certain class of errors. Defining variables this way makes the code much easier to write and reduces the errors you get from being forced to jump back and forth within a scope. It makes the code easier to understand because you see a variable defined in the context of its use. This is especially important when you are defining and initializing a variable at the same time – you can see the meaning of the initialization value by the way the variable is used.

You can also define variables inside the control expressions of for loops and while loops, inside the conditional of an if statement, and inside the selector statement of a switch. Here’s an example showing on-the-fly variable definitions:

In the innermost scope, p is defined right before the scope ends, so it is really a useless gesture (but it shows you can define a variable anywhere). The p in the outer scope is in the same situation.

The definition of i in the control expression of the for loop is an example of being able to define a variable exactly at the point you need it (you can do this only in C++). The scope of i is the scope of the expression controlled by the for loop, so you can turn around and re-use i in the next for loop. This is a convenient and commonly-used idiom in C++; i is the classic name for a loop counter and you don’t have to keep inventing new names.

Although the example also shows variables defined within while, if, and switch statements, this kind of definition is much less common than those in for expressions, possibly because the syntax is so constrained. For example, you cannot have any parentheses. That is, you cannot say:

The addition of the extra parentheses would seem like an innocent and useful thing to do, and because you cannot use them, the results are not what you might like. The problem occurs because ‘!=’ has a higher precedence than ‘=’, so the char c ends up containing a bool converted to char. When that’s printed, on many terminals you’ll see a smiley-face character.

In general, you can consider the ability to define variables within while, if, and switch statements as being there for completeness, but the only place you’re likely to use this kind of variable definition is in a for loop (where you’ll use it quite often).

When creating a variable, you have a number of options to specify the lifetime of the variable, how the storage is allocated for that variable, and how the variable is treated by the compiler.

Global variables are defined outside all function bodies and are available to all parts of the program (even code in other files). Global variables are unaffected by scopes and are always available (i.e., the lifetime of a global variable lasts until the program ends). If the existence of a global variable in one file is declared using the extern keyword in another file, the data is available for use by the second file. Here’s an example of the use of global variables:

Here’s a file that accesses globe as an extern:

Storage for the variable globe is created by the definition in Global.cpp, and that same variable is accessed by the code in Global2.cpp. Since the code in Global2.cpp is compiled separately from the code in Global.cpp, the compiler must be informed that the variable exists elsewhere by the declaration

When you run the program, you’ll see that the call to func( ) does indeed affect the single global instance of globe.

In Global.cpp, you can see the special comment tag (which is my own design):

This says that to create the final program, the object file with the name Global2 must be linked in (there is no extension because the extension names of object files differ from one system to the next). In Global2.cpp, the first line has another special comment tag {O}, which says “Don’t try to create an executable out of this file, it’s being compiled so that it can be linked into some other executable.” The ExtractCode.cpp program in Volume 2 of this book (downloadable at www.BruceEckel.com) reads these tags and creates the appropriate makefile so everything compiles properly (you’ll learn about makefiles at the end of this chapter).

Local variables occur within a scope; they are “local” to a function. They are often called automatic variables because they automatically come into being when the scope is entered and automatically go away when the scope closes. The keyword auto makes this explicit, but local variables default to auto so it is never necessary to declare something as an auto.

A register variable is a type of local variable. The register keyword tells the compiler “Make accesses to this variable as fast as possible.” Increasing the access speed is implementation dependent, but, as the name suggests, it is often done by placing the variable in a register. There is no guarantee that the variable will be placed in a register or even that the access speed will increase. It is a hint to the compiler.

There are restrictions to the use of register variables. You cannot take or compute the address of a register variable. A register variable can be declared only within a block (you cannot have global or static register variables). You can, however, use a register variable as a formal argument in a function (i.e., in the argument list).

In general, you shouldn’t try to second-guess the compiler’s optimizer, since it will probably do a better job than you can. Thus, the register keyword is best avoided.

The static keyword has several distinct meanings. Normally, variables defined local to a function disappear at the end of the function scope. When you call the function again, storage for the variables is created anew and the values are re-initialized. If you want a value to be extant throughout the life of a program, you can define a function’s local variable to be static and give it an initial value. The initialization is performed only the first time the function is called, and the data retains its value between function calls. This way, a function can “remember” some piece of information between function calls.

You may wonder why a global variable isn’t used instead. The beauty of a static variable is that it is unavailable outside the scope of the function, so it can’t be inadvertently changed. This localizes errors.

Here’s an example of the use of static variables:

Each time func( ) is called in the for loop, it prints a different value. If the keyword static is not used, the value printed will always be ‘1’.

The second meaning of static is related to the first in the “unavailable outside a certain scope” sense. When static is applied to a function name or to a variable that is outside of all functions, it means “This name is unavailable outside of this file.” The function name or variable is local to the file; we say it has file scope. As a demonstration, compiling and linking the following two files will cause a linker error:

Even though the variable fs is claimed to exist as an extern in the following file, the linker won’t find it because it has been declared static in FileStatic.cpp.

The static specifier may also be used inside a class. This explanation will be delayed until you learn to create classes, later in the book.

The extern keyword has already been briefly described and demonstrated. It tells the compiler that a variable or a function exists, even if the compiler hasn’t yet seen it in the file currently being compiled. This variable or function may be defined in another file or further down in the current file. As an example of the latter:

When the compiler encounters the declaration ‘extern int i’, it knows that the definition for i must exist somewhere as a global variable. When the compiler reaches the definition of i, no other declaration is visible, so it knows it has found the same i declared earlier in the file. If you were to define i as static, you would be telling the compiler that i is defined globally (via the extern), but it also has file scope (via the static), so the compiler will generate an error.

To understand the behavior of C and C++ programs, you need to know about linkage. In an executing program, an identifier is represented by storage in memory that holds a variable or a compiled function body. Linkage describes this storage as it is seen by the linker. There are two types of linkage: internal linkage and external linkage.

Internal linkage means that storage is created to represent the identifier only for the file being compiled. Other files may use the same identifier name with internal linkage, or for a global variable, and no conflicts will be found by the linker – separate storage is created for each identifier. Internal linkage is specified by the keyword static in C and C++.

External linkage means that a single piece of storage is created to represent the identifier for all files being compiled. The storage is created once, and the linker must resolve all other references to that storage. Global variables and function names have external linkage. These are accessed from other files by declaring them with the keyword extern. Variables defined outside all functions (with the exception of const in C++) and function definitions default to external linkage. You can specifically force them to have internal linkage using the static keyword. You can explicitly state that an identifier has external linkage by defining it with the extern keyword. Defining a variable or function with extern is not necessary in C, but it is sometimes necessary for const in C++.

Automatic (local) variables exist only temporarily, on the stack, while a function is being called. The linker doesn’t know about automatic variables, and so these have no linkage.

In old (pre-Standard) C, if you wanted to make a constant, you had to use the preprocessor:

Everywhere you used PI, the value 3.14159 was substituted by the preprocessor (you can still use this method in C and C++).

When you use the preprocessor to create constants, you place control of those constants outside the scope of the compiler. No type checking is performed on the name PI and you can’t take the address of PI (so you can’t pass a pointer or a reference to PI). PI cannot be a variable of a user-defined type. The meaning of PI lasts from the point it is defined to the end of the file; the preprocessor doesn’t recognize scoping.

C++ introduces the concept of a named constant that is just like a variable, except that its value cannot be changed. The modifier const tells the compiler that a name represents a constant. Any data type, built-in or user-defined, may be defined as const. If you define something as const and then attempt to modify it, the compiler will generate an error.

You must specify the type of a const, like this:

In Standard C and C++, you can use a named constant in an argument list, even if the argument it fills is a pointer or a reference (i.e., you can take the address of a const). A const has a scope, just like a regular variable, so you can “hide” a const inside a function and be sure that the name will not affect the rest of the program.

The const was taken from C++ and incorporated into Standard C, albeit quite differently. In C, the compiler treats a const just like a variable that has a special tag attached that says “Don’t change me.” When you define a const in C, the compiler creates storage for it, so if you define more than one const with the same name in two different files (or put the definition in a header file), the linker will generate error messages about conflicts. The intended use of const in C is quite different from its intended use in C++ (in short, it’s nicer in C++).

In C++, a const must always have an initialization value (in C, this is not true). Constant values for built-in types are expressed as decimal, octal, hexadecimal, or floating-point numbers (sadly, binary numbers were not considered important), or as characters.

In the absence of any other clues, the compiler assumes a constant value is a decimal number. The numbers 47, 0, and 1101 are all treated as decimal numbers.

A constant value with a leading 0 is treated as an octal number (base 8). Base 8 numbers can contain only digits 0-7; the compiler flags other digits as an error. A legitimate octal number is 017 (15 in base 10).

A constant value with a leading 0x is treated as a hexadecimal number (base 16). Base 16 numbers contain the digits 0-9 and a-f or A-F. A legitimate hexadecimal number is 0x1fe (510 in base 10).

Floating point numbers can contain decimal points and exponential powers (represented by e, which means “10 to the power of”). Both the decimal point and the e are optional. If you assign a constant to a floating-point variable, the compiler will take the constant value and convert it to a floating-point number (this process is one form of what’s called implicit type conversion). However, it is a good idea to use either a decimal point or an e to remind the reader that you are using a floating-point number; some older compilers also need the hint.

Legitimate floating-point constant values are: 1e4, 1.0001, 47.0, 0.0, and -1.159e-77. You can add suffixes to force the type of floating-point number: f or F forces a float, L or l forces a long double; otherwise the number will be a double.

Character constants are characters surrounded by single quotes, as: ‘A’, ‘0’, ‘ ‘. Notice there is a big difference between the character ‘0’ (ASCII 96) and the value 0. Special characters are represented with the “backslash escape”: ‘\n’ (newline), ‘\t’ (tab), ‘\\’ (backslash), ‘\r’ (carriage return), ‘\"’ (double quotes), ‘\'’ (single quote), etc. You can also express char constants in octal: ‘\17’ or hexadecimal: ‘\xff’.

Whereas the qualifier const tells the compiler “This never changes” (which allows the compiler to perform extra optimizations), the qualifier volatile tells the compiler “You never know when this will change,” and prevents the compiler from performing any optimizations based on the stability of that variable. Use this keyword when you read some value outside the control of your code, such as a register in a piece of communication hardware. A volatile variable is always read whenever its value is required, even if it was just read the line before.

A special case of some storage being “outside the control of your code” is in a multithreaded program. If you’re watching a particular flag that is modified by another thread or process, that flag should be volatile so the compiler doesn’t make the assumption that it can optimize away multiple reads of the flag.

Note that volatile may have no effect when a compiler is not optimizing, but may prevent critical bugs when you start optimizing the code (which is when the compiler will begin looking for redundant reads).

The const and volatile keywords will be further illuminated in a later chapter.

This section covers all the operators in C and C++.

All operators produce a value from their operands. This value is produced without modifying the operands, except with the assignment, increment, and decrement operators. Modifying an operand is called a side effect. The most common use for operators that modify their operands is to generate the side effect, but you should keep in mind that the value produced is available for your use just as in operators without side effects.

Assignment is performed with the operator =. It means “Take the right-hand side (often called the rvalue) and copy it into the left-hand side (often called the lvalue).” An rvalue is any constant, variable, or expression that can produce a value, but an lvalue must be a distinct, named variable (that is, there must be a physical space in which to store data). For instance, you can assign a constant value to a variable (A = 4;), but you cannot assign anything to constant value – it cannot be an lvalue (you can’t say 4 = A;).

The basic mathematical operators are the same as the ones available in most programming languages: addition (+), subtraction (-), division (/), multiplication (*), and modulus (%; this produces the remainder from integer division). Integer division truncates the result (it doesn’t round). The modulus operator cannot be used with floating-point numbers.

C and C++ also use a shorthand notation to perform an operation and an assignment at the same time. This is denoted by an operator followed by an equal sign, and is consistent with all the operators in the language (whenever it makes sense). For example, to add 4 to the variable x and assign x to the result, you say: x += 4;.

This example shows the use of the mathematical operators:

The rvalues of all the assignments can, of course, be much more complex.

Notice the use of the macro PRINT( ) to save typing (and typing errors!). Preprocessor macros are traditionally named with all uppercase letters so they stand out – you’ll learn later that macros can quickly become dangerous (and they can also be very useful).

The arguments in the parenthesized list following the macro name are substituted in all the code following the closing parenthesis. The preprocessor removes the name PRINT and substitutes the code wherever the macro is called, so the compiler cannot generate any error messages using the macro name, and it doesn’t do any type checking on the arguments (the latter can be beneficial, as shown in the debugging macros at the end of the chapter).

Relational operators establish a relationship between the values of the operands. They produce a Boolean (specified with the bool keyword in C++) true if the relationship is true, and false if the relationship is false. The relational operators are: less than (<), greater than (>), less than or equal to (<=), greater than or equal to (>=), equivalent (==), and not equivalent (!=). They may be used with all built-in data types in C and C++. They may be given special definitions for user-defined data types in C++ (you’ll learn about this in Chapter 12, which covers operator overloading).

The logical operators and (&&) and or (||) produce a true or false based on the logical relationship of its arguments. Remember that in C and C++, a statement is true if it has a non-zero value, and false if it has a value of zero. If you print a bool, you’ll typically see a ‘1’ for true and ‘0’ for false.

This example uses the relational and logical operators:

You can replace the definition for int with float or double in the program above. Be aware, however, that the comparison of a floating-point number with the value of zero is strict; a number that is the tiniest fraction different from another number is still “not equal.” A floating-point number that is the tiniest bit above zero is still true.

The bitwise operators allow you to manipulate individual bits in a number (since floating point values use a special internal format, the bitwise operators work only with integral types: char, int and long). Bitwise operators perform Boolean algebra on the corresponding bits in the arguments to produce the result.

The bitwise and operator (&) produces a one in the output bit if both input bits are one; otherwise it produces a zero. The bitwise or operator (|) produces a one in the output bit if either input bit is a one and produces a zero only if both input bits are zero. The bitwise exclusive or, or xor (^) produces a one in the output bit if one or the other input bit is a one, but not both. The bitwise not (~, also called the ones complement operator) is a unary operator – it only takes one argument (all other bitwise operators are binary operators). Bitwise not produces the opposite of the input bit – a one if the input bit is zero, a zero if the input bit is one.

Bitwise operators can be combined with the = sign to unite the operation and assignment: &=, |=, and ^= are all legitimate operations (since ~ is a unary operator it cannot be combined with the = sign).

The shift operators also manipulate bits. The left-shift operator (<<) produces the operand to the left of the operator shifted to the left by the number of bits specified after the operator. The right-shift operator (>>) produces the operand to the left of the operator shifted to the right by the number of bits specified after the operator. If the value after the shift operator is greater than the number of bits in the left-hand operand, the result is undefined. If the left-hand operand is unsigned, the right shift is a logical shift so the upper bits will be filled with zeros. If the left-hand operand is signed, the right shift may or may not be a logical shift (that is, the behavior is undefined).

Shifts can be combined with the equal sign (<<= and >>=). The lvalue is replaced by the lvalue shifted by the rvalue.

What follows is an example that demonstrates the use of all the operators involving bits. First, here’s a general-purpose function that prints a byte in binary format, created separately so that it may be easily reused. The header file declares the function:

Here’s the implementation of the function:

The printBinary( ) function takes a single byte and displays it bit-by-bit. The expression

produces a one in each successive bit position; in binary: 00000001, 00000010, etc. If this bit is bitwise anded with val and the result is nonzero, it means there was a one in that position in val.

Finally, the function is used in the example that shows the bit-manipulation operators:

Once again, a preprocessor macro is used to save typing. It prints the string of your choice, then the binary representation of an expression, then a newline.

In main( ), the variables are unsigned. This is because, in general, you don't want signs when you are working with bytes. An int must be used instead of a char for getval because the “cin >>” statement will otherwise treat the first digit as a character. By assigning getval to a and b, the value is converted to a single byte (by truncating it).

The << and >> provide bit-shifting behavior, but when they shift bits off the end of the number, those bits are lost (it’s commonly said that they fall into the mythical bit bucket, a place where discarded bits end up, presumably so they can be reused...). When manipulating bits you can also perform rotation, which means that the bits that fall off one end are inserted back at the other end, as if they’re being rotated around a loop. Even though most computer processors provide a machine-level rotate command (so you’ll see it in the assembly language for that processor), there is no direct support for “rotate” in C or C++. Presumably the designers of C felt justified in leaving “rotate” off (aiming, as they said, for a minimal language) because you can build your own rotate command. For example, here are functions to perform left and right rotations:

Try using these functions in Bitwise.cpp. Notice the definitions (or at least declarations) of rol( ) and ror( ) must be seen by the compiler in Bitwise.cpp before the functions are used.

The bitwise functions are generally extremely efficient to use because they translate directly into assembly language statements. Sometimes a single C or C++ statement will generate a single line of assembly code.

Bitwise not isn’t the only operator that takes a single argument. Its companion, the logical not (!), will take a true value and produce a false value. The unary minus (-) and unary plus (+) are the same operators as binary minus and plus; the compiler figures out which usage is intended by the way you write the expression. For instance, the statement

has an obvious meaning. The compiler can figure out:

but the reader might get confused, so it is safer to say:

The unary minus produces the negative of the value. Unary plus provides symmetry with unary minus, although it doesn’t actually do anything.

The increment and decrement operators (++ and --) were introduced earlier in this chapter. These are the only operators other than those involving assignment that have side effects. These operators increase or decrease the variable by one unit, although “unit” can have different meanings according to the data type – this is especially true with pointers.

The last unary operators are the address-of (&), dereference (* and ->), and cast operators in C and C++, and new and delete in C++. Address-of and dereference are used with pointers, described in this chapter. Casting is described later in this chapter, and new and delete are introduced in Chapter 4.

The ternary if-else is unusual because it has three operands. It is truly an operator because it produces a value, unlike the ordinary if-else statement. It consists of three expressions: if the first expression (followed by a ?) evaluates to true, the expression following the ? is evaluated and its result becomes the value produced by the operator. If the first expression is false, the third expression (following a :) is executed and its result becomes the value produced by the operator.

The conditional operator can be used for its side effects or for the value it produces. Here’s a code fragment that demonstrates both:

Here, the conditional produces the rvalue. a is assigned to the value of b if the result of decrementing b is nonzero. If b became zero, a and b are both assigned to -99. b is always decremented, but it is assigned to -99 only if the decrement causes b to become 0. A similar statement can be used without the “a =” just for its side effects:

Here the second B is superfluous, since the value produced by the operator is unused. An expression is required between the ? and :. In this case, the expression could simply be a constant that might make the code run a bit faster.

The comma is not restricted to separating variable names in multiple definitions, such as

Of course, it’s also used in function argument lists. However, it can also be used as an operator to separate expressions – in this case it produces only the value of the last expression. All the rest of the expressions in the comma-separated list are evaluated only for their side effects. This example increments a list of variables and uses the last one as the rvalue:

In general, it’s best to avoid using the comma as anything other than a separator, since people are not used to seeing it as an operator.

As illustrated above, one of the pitfalls when using operators is trying to get away without parentheses when you are even the least bit uncertain about how an expression will evaluate (consult your local C manual for the order of expression evaluation).

Another extremely common error looks like this:

The statement a = b will always evaluate to true when b is non-zero. The variable a is assigned to the value of b, and the value of b is also produced by the operator =. In general, you want to use the equivalence operator == inside a conditional statement, not assignment. This one bites a lot of programmers (however, some compilers will point out the problem to you, which is helpful).

A similar problem is using bitwise and and or instead of their logical counterparts. Bitwise and and or use one of the characters (& or |), while logical and and or use two (&& and ||). Just as with = and ==, it’s easy to just type one character instead of two. A useful mnemonic device is to observe that “Bits are smaller, so they don’t need as many characters in their operators.”

The word cast is used in the sense of “casting into a mold.” The compiler will automatically change one type of data into another if it makes sense. For instance, if you assign an integral value to a floating-point variable, the compiler will secretly call a function (or more probably, insert code) to convert the int to a float. Casting allows you to make this type conversion explicit, or to force it when it wouldn’t normally happen.

To perform a cast, put the desired data type (including all modifiers) inside parentheses to the left of the value. This value can be a variable, a constant, the value produced by an expression, or the return value of a function. Here’s an example:

Casting is powerful, but it can cause headaches because in some situations it forces the compiler to treat data as if it were (for instance) larger than it really is, so it will occupy more space in memory; this can trample over other data. This usually occurs when casting pointers, not when making simple casts like the one shown above.

C++ has an additional casting syntax, which follows the function call syntax. This syntax puts the parentheses around the argument, like a function call, rather than around the data type:

Of course in the case above you wouldn’t really need a cast; you could just say 200f (in effect, that’s typically what the compiler will do for the above expression). Casts are generally used instead with variables, rather than constants.

Casts should be used carefully, because what you are actually doing is saying to the compiler “Forget type checking – treat it as this other type instead.” That is, you’re introducing a hole in the C++ type system and preventing the compiler from telling you that you’re doing something wrong with a type. What’s worse, the compiler believes you implicitly and doesn’t perform any other checking to catch errors. Once you start casting, you open yourself up for all kinds of problems. In fact, any program that uses a lot of casts should be viewed with suspicion, no matter how much you are told it simply “must” be done that way. In general, casts should be few and isolated to the solution of very specific problems.

Once you understand this and are presented with a buggy program, your first inclination may be to look for casts as culprits. But how do you locate C-style casts? They are simply type names inside of parentheses, and if you start hunting for such things you’ll discover that it’s often hard to distinguish them from the rest of your code.

Standard C++ includes an explicit cast syntax that can be used to completely replace the old C-style casts (of course, C-style casts cannot be outlawed without breaking code, but compiler writers could easily flag old-style casts for you). The explicit cast syntax is such that you can easily find them, as you can see by their names:

The first three explicit casts will be described more completely in the following sections, while the last one can be demonstrated only after you’ve learned more, in Chapter 15.

A static_cast is used for all conversions that are well-defined. These include “safe” conversions that the compiler would allow you to do without a cast and less-safe conversions that are nonetheless well-defined. The types of conversions covered by static_cast include typical castless conversions, narrowing (information-losing) conversions, forcing a conversion from a void*, implicit type conversions, and static navigation of class hierarchies (since you haven’t seen classes and inheritance yet, this last topic will be delayed until Chapter 15):

In Section (1), you see the kinds of conversions you’re used to doing in C, with or without a cast. Promoting from an int to a long or float is not a problem because the latter can always hold every value that an int can contain. Although it’s unnecessary, you can use static_cast to highlight these promotions.

Converting back the other way is shown in (2). Here, you can lose data because an int is not as “wide” as a long or a float; it won’t hold numbers of the same size. Thus these are called narrowing conversions. The compiler will still perform these, but will often give you a warning. You can eliminate this warning and indicate that you really did mean it using a cast.

Assigning from a void* is not allowed without a cast in C++ (unlike C), as seen in (3). This is dangerous and requires that programmers know what they’re doing. The static_cast, at least, is easier to locate than the old standard cast when you’re hunting for bugs.

Section (4) of the program shows the kinds of implicit type conversions that are normally performed automatically by the compiler. These are automatic and require no casting, but again static_cast highlights the action in case you want to make it clear what’s happening or hunt for it later.

If you want to convert from a const to a nonconst or from a volatile to a nonvolatile, you use const_cast. This is the only conversion allowed with const_cast; if any other conversion is involved it must be done using a separate expression or you’ll get a compile-time error.

If you take the address of a const object, you produce a pointer to a const, and this cannot be assigned to a nonconst pointer without a cast. The old-style cast will accomplish this, but the const_cast is the appropriate one to use. The same holds true for volatile.

This is the least safe of the casting mechanisms, and the one most likely to produce bugs. A reinterpret_cast pretends that an object is just a bit pattern that can be treated (for some dark purpose) as if it were an entirely different type of object. This is the low-level bit twiddling that C is notorious for. You’ll virtually always need to reinterpret_cast back to the original type (or otherwise treat the variable as its original type) before doing anything else with it.

In this simple example, struct X just contains an array of int, but when you create one on the stack as in X x, the values of each of the ints are garbage (this is shown using the print( ) function to display the contents of the struct). To initialize them, the address of the X is taken and cast to an int pointer, which is then walked through the array to set each int to zero. Notice how the upper bound for i is calculated by “adding” sz to xp; the compiler knows that you actually want sz pointer locations greater than xp and it does the correct pointer arithmetic for you.

The idea of reinterpret_cast is that when you use it, what you get is so foreign that it cannot be used for the type’s original purpose unless you cast it back. Here, we see the cast back to an X* in the call to print, but of course since you still have the original identifier you can also use that. But the xp is only useful as an int*, which is truly a “reinterpretation” of the original X.

A reinterpret_cast often indicates inadvisable and/or nonportable programming, but it’s available when you decide you have to use it.

The sizeof operator stands alone because it satisfies an unusual need. sizeof gives you information about the amount of memory allocated for data items. As described earlier in this chapter, sizeof tells you the number of bytes used by any particular variable. It can also give the size of a data type (with no variable name):

By definition, the sizeof any type of char (signed, unsigned or plain) is always one, regardless of whether the underlying storage for a char is actually one byte. For all other types, the result is the size in bytes.

Note that sizeof is an operator, not a function. If you apply it to a type, it must be used with the parenthesized form shown above, but if you apply it to a variable you can use it without parentheses:

sizeof can also give you the sizes of user-defined data types. This is used later in the book.

This is an escape mechanism that allows you to write assembly code for your hardware within a C++ program. Often you’re able to reference C++ variables within the assembly code, which means you can easily communicate with your C++ code and limit the assembly code to that necessary for efficiency tuning or to use special processor instructions. The exact syntax that you must use when writing the assembly language is compiler-dependent and can be discovered in your compiler’s documentation.

These are keywords for bitwise and logical operators. Non-U.S. programmers without keyboard characters like &, |, ^, and so on, were forced to use C’s horrible trigraphs, which were not only annoying to type, but obscure when reading. This is repaired in C++ with additional keywords:

If your compiler complies with Standard C++, it will support these keywords.

The fundamental data types and their variations are essential, but rather primitive. C and C++ provide tools that allow you to compose more sophisticated data types from the fundamental data types. As you’ll see, the most important of these is struct, which is the foundation for class in C++. However, the simplest way to create more sophisticated types is simply to alias a name to another name via typedef.

This keyword promises more than it delivers: typedef suggests “type definition” when “alias” would probably have been a more accurate description, since that’s what it really does. The syntax is:

typedef existing-type-description alias-name

People often use typedef when data types get slightly complicated, just to prevent extra keystrokes. Here is a commonly-used typedef:

Now if you say ulong the compiler knows that you mean unsigned long. You might think that this could as easily be accomplished using preprocessor substitution, but there are key situations in which the compiler must be aware that you’re treating a name as if it were a type, so typedef is essential.

One place where typedef comes in handy is for pointer types. As previously mentioned, if you say:

This actually produces an int* which is x and an int (not an int*) which is y. That is, the ‘*’ binds to the right, not the left. However, if you use a typedef:

Then both x and y are of type int*.

You can argue that it’s more explicit and therefore more readable to avoid typedefs for primitive types, and indeed programs rapidly become difficult to read when many typedefs are used. However, typedefs become especially important in C when used with struct.

A struct is a way to collect a group of variables into a structure. Once you create a struct, then you can make many instances of this “new” type of variable you’ve invented. For example:

The struct declaration must end with a semicolon. In main( ), two instances of Structure1 are created: s1 and s2. Each of these has their own separate versions of c, i, f, and d. So s1 and s2 represent clumps of completely independent variables. To select one of the elements within s1 or s2, you use a ‘.’, syntax you’ve seen in the previous chapter when using C++ class objects – since classes evolved from structs, this is where that syntax arose from.

One thing you’ll notice is the awkwardness of the use of Structure1 (as it turns out, this is only required by C, not C++). In C, you can’t just say Structure1 when you’re defining variables, you must say struct Structure1. This is where typedef becomes especially handy in C:

By using typedef in this way, you can pretend (in C; try removing the typedef for C++) that Structure2 is a built-in type, like int or float, when you define s1 and s2 (but notice it only has data – characteristics – and does not include behavior, which is what we get with real objects in C++). You’ll notice that the struct identifier has been left off at the beginning, because the goal is to create the typedef. However, there are times when you might need to refer to the struct during its definition. In those cases, you can actually repeat the name of the struct as the struct name and as the typedef:

If you look at this for awhile, you’ll see that sr1 and sr2 point to each other, as well as each holding a piece of data.

Actually, the struct name does not have to be the same as the typedef name, but it is usually done this way as it tends to keep things simpler.

In the examples above, all the structs are manipulated as objects. However, like any piece of storage, you can take the address of a struct object (as seen in SelfReferential.cpp above). To select the elements of a particular struct object, you use a ‘.’, as seen above. However, if you have a pointer to a struct object, you must select an element of that object using a different operator: the ‘->’. Here’s an example:

In main( ), the struct pointer sp is initially pointing to s1, and the members of s1 are initialized by selecting them with the ‘->’ (and you use this same operator in order to read those members). But then sp is pointed to s2, and those variables are initialized the same way. So you can see that another benefit of pointers is that they can be dynamically redirected to point to different objects; this provides more flexibility in your programming, as you will learn.

For now, that’s all you need to know about structs, but you’ll become much more comfortable with them (and especially their more potent successors, classes) as the book progresses.

An enumerated data type is a way of attaching names to numbers, thereby giving more meaning to anyone reading the code. The enum keyword (from C) automatically enumerates any list of identifiers you give it by assigning them values of 0, 1, 2, etc. You can declare enum variables (which are always represented as integral values). The declaration of an enum looks similar to a struct declaration.

An enumerated data type is useful when you want to keep track of some sort of feature:

shape is a variable of the ShapeType enumerated data type, and its value is compared with the value in the enumeration. Since shape is really just an int, however, it can be any value an int can hold (including a negative number). You can also compare an int variable with a value in the enumeration.

You should be aware that the example above of switching on type turns out to be a problematic way to program. C++ has a much better way to code this sort of thing, the explanation of which must be delayed until much later in the book.

If you don’t like the way the compiler assigns values, you can do it yourself, like this:

If you give values to some names and not to others, the compiler will use the next integral value. For example,

The compiler gives pop the value 26.

You can see how much more readable the code is when you use enumerated data types. However, to some degree this is still an attempt (in C) to accomplish the things that we can do with a class in C++, so you’ll see enum used less in C++.

C’s enumerations are fairly primitive, simply associating integral values with names, but they provide no type checking. In C++, as you may have come to expect by now, the concept of type is fundamental, and this is true with enumerations. When you create a named enumeration, you effectively create a new type just as you do with a class: The name of your enumeration becomes a reserved word for the duration of that translation unit.

In addition, there’s stricter type checking for enumerations in C++ than in C. You’ll notice this in particular if you have an instance of an enumeration color called a. In C you can say a++, but in C++ you can’t. This is because incrementing an enumeration is performing two type conversions, one of them legal in C++ and one of them illegal. First, the value of the enumeration is implicitly cast from a color to an int, then the value is incremented, then the int is cast back into a color. In C++ this isn’t allowed, because color is a distinct type and not equivalent to an int. This makes sense, because how do you know the increment of blue will even be in the list of colors? If you want to increment a color, then it should be a class (with an increment operation) and not an enum, because the class can be made to be much safer. Any time you write code that assumes an implicit conversion to an enum type, the compiler will flag this inherently dangerous activity.

Unions (described next) have similar additional type checking in C++.

Sometimes a program will handle different types of data using the same variable. In this situation, you have two choices: you can create a struct containing all the possible different types you might need to store, or you can use a union. A union piles all the data into a single space; it figures out the amount of space necessary for the largest item you’ve put in the union, and makes that the size of the union. Use a union to save memory.

Anytime you place a value in a union, the value always starts in the same place at the beginning of the union, but only uses as much space as is necessary. Thus, you create a “super-variable” capable of holding any of the union variables. All the addresses of the union variables are the same (in a class or struct, the addresses are different).

Here’s a simple use of a union. Try removing various elements and see what effect it has on the size of the union. Notice that it makes no sense to declare more than one instance of a single data type in a union (unless you’re just doing it to use a different name).

The compiler performs the proper assignment according to the union member you select.

Once you perform an assignment, the compiler doesn’t care what you do with the union. In the example above, you could assign a floating-point value to x:

and then send it to the output as if it were an int:

This would produce garbage.

Arrays are a kind of composite type because they allow you to clump a lot of variables together, one right after the other, under a single identifier name. If you say:

You create storage for 10 int variables stacked on top of each other, but without unique identifier names for each variable. Instead, they are all lumped under the name a.

To access one of these array elements, you use the same square-bracket syntax that you use to define an array:

However, you must remember that even though the size of a is 10, you select array elements starting at zero (this is sometimes called zero indexing), so you can select only the array elements 0-9, like this:

Array access is extremely fast. However, if you index past the end of the array, there is no safety net – you’ll step on other variables. The other drawback is that you must define the size of the array at compile time; if you want to change the size at runtime you can’t do it with the syntax above (C does have a way to create an array dynamically, but it’s significantly messier). The C++ vector, introduced in the previous chapter, provides an array-like object that automatically resizes itself, so it is usually a much better solution if your array size cannot be known at compile time.

You can make an array of any type, even of structs:

Notice how the struct identifier i is independent of the for loop’s i.

To see that each element of an array is contiguous with the next, you can print out the addresses like this:

When you run this program, you’ll see that each element is one int size away from the previous one. That is, they are stacked one on top of the other.

The identifier of an array is unlike the identifiers for ordinary variables. For one thing, an array identifier is not an lvalue; you cannot assign to it. It’s really just a hook into the square-bracket syntax, and when you give the name of an array, without square brackets, what you get is the starting address of the array:

When you run this program you’ll see that the two addresses (which will be printed in hexadecimal, since there is no cast to long) are the same.

So one way to look at the array identifier is as a read-only pointer to the beginning of an array. And although we can’t change the array identifier to point somewhere else, we can create another pointer and use that to move around in the array. In fact, the square-bracket syntax works with regular pointers as well:

The fact that naming an array produces its starting address turns out to be quite important when you want to pass an array to a function. If you declare an array as a function argument, what you’re really declaring is a pointer. So in the following example, func1( ) and func2( ) effectively have the same argument lists:

Even though func1( ) and func2( ) declare their arguments differently, the usage is the same inside the function. There are some other issues that this example reveals: arrays cannot be passed by value[32], that is, you never automatically get a local copy of the array that you pass into a function. Thus, when you modify an array, you’re always modifying the outside object. This can be a bit confusing at first, if you’re expecting the pass-by-value provided with ordinary arguments.

You’ll notice that print( ) uses the square-bracket syntax for array arguments. Even though the pointer syntax and the square-bracket syntax are effectively the same when passing arrays as arguments, the square-bracket syntax makes it clearer to the reader that you mean for this argument to be an array.

Also note that the size argument is passed in each case. Just passing the address of an array isn’t enough information; you must always be able to know how big the array is inside your function, so you don’t run off the end of that array.

Arrays can be of any type, including arrays of pointers. In fact, when you want to pass command-line arguments into your program, C and C++ have a special argument list for main( ), which looks like this:

The first argument is the number of elements in the array, which is the second argument. The second argument is always an array of char*, because the arguments are passed from the command line as character arrays (and remember, an array can be passed only as a pointer). Each whitespace-delimited cluster of characters on the command line is turned into a separate array argument. The following program prints out all its command-line arguments by stepping through the array:

You’ll notice that argv[0] is the path and name of the program itself. This allows the program to discover information about itself. It also adds one more to the array of program arguments, so a common error when fetching command-line arguments is to grab argv[0] when you want argv[1].

You are not forced to use argc and argv as identifiers in main( ); those identifiers are only conventions (but it will confuse people if you don’t use them). Also, there is an alternate way to declare argv:

Both forms are equivalent, but I find the version used in this book to be the most intuitive when reading the code, since it says, directly, “This is an array of character pointers.”

All you get from the command-line is character arrays; if you want to treat an argument as some other type, you are responsible for converting it inside your program. To facilitate the conversion to numbers, there are some helper functions in the Standard C library, declared in <cstdlib>. The simplest ones to use are atoi( ), atol( ), and atof( ) to convert an ASCII character array to an int, long, and double floating-point value, respectively. Here’s an example using atoi( ) (the other two functions are called the same way):

In this program, you can put any number of arguments on the command line. You’ll notice that the for loop starts at the value 1 to skip over the program name at argv[0]. Also, if you put a floating-point number containing a decimal point on the command line, atoi( ) takes only the digits up to the decimal point. If you put non-numbers on the command line, these come back from atoi( ) as zero.

The printBinary( ) function introduced earlier in this chapter is handy for delving into the internal structure of various data types. The most interesting of these is the floating-point format that allows C and C++ to store numbers representing very large and very small values in a limited amount of space. Although the details can’t be completely exposed here, the bits inside of floats and doubles are divided into three regions: the exponent, the mantissa, and the sign bit; thus it stores the values using scientific notation. The following program allows you to play around by printing out the binary patterns of various floating point numbers so you can deduce for yourself the scheme used in your compiler’s floating-point format (usually this is the IEEE standard for floating point numbers, but your compiler may not follow that):

First, the program guarantees that you’ve given it an argument by checking the value of argc, which is two if there’s a single argument (it’s one if there are no arguments, since the program name is always the first element of argv). If this fails, a message is printed and the Standard C Library function exit( ) is called to terminate the program.

The program grabs the argument from the command line and converts the characters to a double using atof( ). Then the double is treated as an array of bytes by taking the address and casting it to an unsigned char*. Each of these bytes is passed to printBinary( ) for display.

This example has been set up to print the bytes in an order such that the sign bit appears first – on my machine. Yours may be different, so you might want to re-arrange the way things are printed. You should also be aware that floating-point formats are not trivial to understand; for example, the exponent and mantissa are not generally arranged on byte boundaries, but instead a number of bits is reserved for each one and they are packed into the memory as tightly as possible. To truly see what’s going on, you’d need to find out the size of each part of the number (sign bits are always one bit, but exponents and mantissas are of differing sizes) and print out the bits in each part separately.

If all you could do with a pointer that points at an array is treat it as if it were an alias for that array, pointers into arrays wouldn’t be very interesting. However, pointers are more flexible than this, since they can be modified to point somewhere else (but remember, the array identifier cannot be modified to point somewhere else).

Pointer arithmetic refers to the application of some of the arithmetic operators to pointers. The reason pointer arithmetic is a separate subject from ordinary arithmetic is that pointers must conform to special constraints in order to make them behave properly. For example, a common operator to use with pointers is ++, which “adds one to the pointer.” What this actually means is that the pointer is changed to move to “the next value,” whatever that means. Here’s an example:

For one run on my machine, the output is:

What’s interesting here is that even though the operation ++ appears to be the same operation for both the int* and the double*, you can see that the pointer has been changed only 4 bytes for the int* but 8 bytes for the double*. Not coincidentally, these are the sizes of int and double on my machine. And that’s the trick of pointer arithmetic: the compiler figures out the right amount to change the pointer so that it’s pointing to the next element in the array (pointer arithmetic is only meaningful within arrays). This even works with arrays of structs:

The output for one run on my machine was:

So you can see the compiler also does the right thing for pointers to structs (and classes and unions).

Pointer arithmetic also works with the operators --, +, and -, but the latter two operators are limited: you cannot add two pointers, and if you subtract pointers the result is the number of elements between the two pointers. However, you can add or subtract an integral value and a pointer. Here’s an example demonstrating the use of pointer arithmetic:

It begins with another macro, but this one uses a preprocessor feature called stringizing (implemented with the ‘#’ sign before an expression) that takes any expression and turns it into a character array. This is quite convenient, since it allows the expression to be printed, followed by a colon, followed by the value of the expression. In main( ) you can see the useful shorthand that is produced.

Although pre- and postfix versions of ++ and -- are valid with pointers, only the prefix versions are used in this example because they are applied before the pointers are dereferenced in the expressions above, so they allow us to see the effects of the operations. Note that only integral values are being added and subtracted; if two pointers were combined this way the compiler would not allow it.

Here is the output of the program above:

In all cases, the pointer arithmetic results in the pointer being adjusted to point to the “right place,” based on the size of the elements being pointed to.

If pointer arithmetic seems a bit overwhelming at first, don’t worry. Most of the time you’ll only need to create arrays and index into them with [ ], and the most sophisticated pointer arithmetic you’ll usually need is ++ and --. Pointer arithmetic is generally reserved for more clever and complex programs, and many of the containers in the Standard C++ library hide most of these clever details so you don’t have to worry about them.

In an ideal environment, you have an excellent debugger available that easily makes the behavior of your program transparent so you can quickly discover errors. However, most debuggers have blind spots, and these will require you to embed code snippets in your program to help you understand what’s going on. In addition, you may be developing in an environment (such as an embedded system, which is where I spent my formative years) that has no debugger available, and perhaps very limited feedback (i.e. a one-line LED display). In these cases you become creative in the ways you discover and display information about the execution of your program. This section suggests some techniques for doing this.

If you hard-wire debugging code into a program, you can run into problems. You start to get too much information, which makes the bugs difficult to isolate. When you think you’ve found the bug you start tearing out debugging code, only to find you need to put it back in again. You can solve these problems with two types of flags: preprocessor debugging flags and runtime debugging flags.

By using the preprocessor to #define one or more debugging flags (preferably in a header file), you can test a flag using an #ifdef statement and conditionally include debugging code. When you think your debugging is finished, you can simply #undef the flag(s) and the code will automatically be removed (and you’ll reduce the size and runtime overhead of your executable file).

It is best to decide on names for debugging flags before you begin building your project so the names will be consistent. Preprocessor flags are traditionally distinguished from variables by writing them in all upper case. A common flag name is simply DEBUG (but be careful you don’t use NDEBUG, which is reserved in C). The sequence of statements might be:

Most C and C++ implementations will also let you #define and #undef flags from the compiler command line, so you can re-compile code and insert debugging information with a single command (preferably via the makefile, a tool that will be described shortly). Check your local documentation for details.

In some situations it is more convenient to turn debugging flags on and off during program execution, especially by setting them when the program starts up using the command line. Large programs are tedious to recompile just to insert debugging code.

To turn debugging code on and off dynamically, create bool flags:

This program continues to allow you to turn the debugging flag on and off until you type “quit” to tell it you want to exit. Notice it requires that full words are typed in, not just letters (you can shorten it to letter if you wish). Also, a command-line argument can optionally be used to turn debugging on at startup – this argument can appear anyplace in the command line, since the startup code in main( ) looks at all the arguments. The testing is quite simple because of the expression:

This takes the argv[i] character array and creates a string, which then can be easily compared to the right-hand side of the ==. The program above searches for the entire string --debug=on. You can also look for --debug= and then see what’s after that, to provide more options. Volume 2 (available from www.BruceEckel.com) devotes a chapter to the Standard C++ string class.

Although a debugging flag is one of the relatively few areas where it makes a lot of sense to use a global variable, there’s nothing that says it must be that way. Notice that the variable is in lower case letters to remind the reader it isn’t a preprocessor flag.

When writing debugging code, it is tedious to write print expressions consisting of a character array containing the variable name, followed by the variable. Fortunately, Standard C includes the stringize operator ‘#’, which was used earlier in this chapter. When you put a # before an argument in a preprocessor macro, the preprocessor turns that argument into a character array. This, combined with the fact that character arrays with no intervening punctuation are concatenated into a single character array, allows you to make a very convenient macro for printing the values of variables during debugging:

If you print the variable a by calling the macro PR(a), it will have the same effect as the code:

This same process works with entire expressions. The following program uses a macro to create a shorthand that prints the stringized expression and then evaluates the expression and prints the result:

You can see how a technique like this can quickly become indispensable, especially if you have no debugger (or must use multiple development environments). You can also insert an #ifdef to cause P(A) to be defined as “nothing” when you want to strip out debugging.

In the standard header file <cassert> you’ll find assert( ), which is a convenient debugging macro. When you use assert( ), you give it an argument that is an expression you are “asserting to be true.” The preprocessor generates code that will test the assertion. If the assertion isn’t true, the program will stop after issuing an error message telling you what the assertion was and that it failed. Here’s a trivial example:

The macro originated in Standard C, so it’s also available in the header file assert.h.

When you are finished debugging, you can remove the code generated by the macro by placing the line:

in the program before the inclusion of <cassert>, or by defining NDEBUG on the compiler command line. NDEBUG is a flag used in <cassert> to change the way code is generated by the macros.

Later in this book, you’ll see some more sophisticated alternatives to assert( ).

Once a function is compiled and loaded into the computer to be executed, it occupies a chunk of memory. That memory, and thus the function, has an address.

C has never been a language to bar entry where others fear to tread. You can use function addresses with pointers just as you can use variable addresses. The declaration and use of function pointers looks a bit opaque at first, but it follows the format of the rest of the language.

To define a pointer to a function that has no arguments and no return value, you say:

When you are looking at a complex definition like this, the best way to attack it is to start in the middle and work your way out. “Starting in the middle” means starting at the variable name, which is funcPtr. “Working your way out” means looking to the right for the nearest item (nothing in this case; the right parenthesis stops you short), then looking to the left (a pointer denoted by the asterisk), then looking to the right (an empty argument list indicating a function that takes no arguments), then looking to the left (void, which indicates the function has no return value). This right-left-right motion works with most declarations.

To review, “start in the middle” (“funcPtr is a ...”), go to the right (nothing there – you're stopped by the right parenthesis), go to the left and find the ‘*’ (“... pointer to a ...”), go to the right and find the empty argument list (“... function that takes no arguments ... ”), go to the left and find the void (“funcPtr is a pointer to a function that takes no arguments and returns void”).

You may wonder why *funcPtr requires parentheses. If you didn't use them, the compiler would see:

You would be declaring a function (that returns a void*) rather than defining a variable. You can think of the compiler as going through the same process you do when it figures out what a declaration or definition is supposed to be. It needs those parentheses to “bump up against” so it goes back to the left and finds the ‘*’, instead of continuing to the right and finding the empty argument list.

As an aside, once you figure out how the C and C++ declaration syntax works you can create much more complicated items. For instance:

Walk through each one and use the right-left guideline to figure it out. Number 1 says “fp1 is a pointer to a function that takes an integer argument and returns a pointer to an array of 10 void pointers.”

Number 2 says “fp2 is a pointer to a function that takes three arguments (int, int, and float) and returns a pointer to a function that takes an integer argument and returns a float.”

If you are creating a lot of complicated definitions, you might want to use a typedef. Number 3 shows how a typedef saves typing the complicated description every time. It says “An fp3 is a pointer to a function that takes no arguments and returns a pointer to an array of 10 pointers to functions that take no arguments and return doubles.” Then it says “a is one of these fp3 types.” typedef is generally useful for building complicated descriptions from simple ones.

Number 4 is a function declaration instead of a variable definition. It says “f4 is a function that returns a pointer to an array of 10 pointers to functions that return integers.”

You will rarely if ever need such complicated declarations and definitions as these. However, if you go through the exercise of figuring them out you will not even be mildly disturbed with the slightly complicated ones you may encounter in real life.

Once you define a pointer to a function, you must assign it to a function address before you can use it. Just as the address of an array arr[10] is produced by the array name without the brackets (arr), the address of a function func() is produced by the function name without the argument list (func). You can also use the more explicit syntax &func(). To call the function, you dereference the pointer in the same way that you declared it (remember that C and C++ always try to make definitions look the same as the way they are used). The following example shows how a pointer to a function is defined and used:

After the pointer to function fp is defined, it is assigned to the address of a function func() using fp = func (notice the argument list is missing on the function name). The second case shows simultaneous definition and initialization.

One of the more interesting constructs you can create is an array of pointers to functions. To select a function, you just index into the array and dereference the pointer. This supports the concept of table-driven code; instead of using conditionals or case statements, you select functions to execute based on a state variable (or a combination of state variables). This kind of design can be useful if you often add or delete functions from the table (or if you want to create or change such a table dynamically).

The following example creates some dummy functions using a preprocessor macro, then creates an array of pointers to those functions using automatic aggregate initialization. As you can see, it is easy to add or remove functions from the table (and thus, functionality from the program) by changing a small amount of code:

At this point, you might be able to imagine how this technique could be useful when creating some sort of interpreter or list processing program.

When using separate compilation (breaking code into a number of translation units), you need some way to automatically compile each file and to tell the linker to build all the pieces – along with the appropriate libraries and startup code – into an executable file. Most compilers allow you to do this with a single command-line statement. For the GNU C++ compiler, for example, you might say

The problem with this approach is that the compiler will first compile each individual file, regardless of whether that file needs to be rebuilt or not. With many files in a project, it can become prohibitive to recompile everything if you’ve changed only a single file.

The solution to this problem, developed on Unix but available everywhere in some form, is a program called make. The make utility manages all the individual files in a project by following the instructions in a text file called a makefile. When you edit some of the files in a project and type make, the make program follows the guidelines in the makefile to compare the dates on the source code files to the dates on the corresponding target files, and if a source code file date is more recent than its target file, make invokes the compiler on the source code file. make only recompiles the source code files that were changed, and any other source-code files that are affected by the modified files. By using make, you don’t have to re-compile all the files in your project every time you make a change, nor do you have to check to see that everything was built properly. The makefile contains all the commands to put your project together. Learning to use make will save you a lot of time and frustration. You’ll also discover that make is the typical way that you install new software on a Linux/Unix machine (although those makefiles tend to be far more complicated than the ones presented in this book, and you’ll often automatically generate a makefile for your particular machine as part of the installation process).

Because make is available in some form for virtually all C++ compilers (and even if it isn’t, you can use freely-available makes with any compiler), it will be the tool used throughout this book. However, compiler vendors have also created their own project building tools. These tools ask you which files are in your project and determine all the relationships themselves. These tools use something similar to a makefile, generally called a project file, but the programming environment maintains this file so you don’t have to worry about it. The configuration and use of project files varies from one development environment to another, so you must find the appropriate documentation on how to use them (although project file tools provided by compiler vendors are usually so simple to use that you can learn them by playing around – my favorite form of education).

The makefiles used within this book should work even if you are also using a specific vendor’s project-building tool.

When you type make (or whatever the name of your “make” program happens to be), the make program looks in the current directory for a file named makefile, which you’ve created if it’s your project. This file lists dependencies between source code files. make looks at the dates on files. If a dependent file has an older date than a file it depends on, make executes the rule given after the dependency.

All comments in makefiles start with a # and continue to the end of the line.

As a simple example, the makefile for a program called “hello” might contain:

This says that hello.exe (the target) depends on hello.cpp. When hello.cpp has a newer date than hello.exe, make executes the “rule” mycompiler hello.cpp. There may be multiple dependencies and multiple rules. Many make programs require that all the rules begin with a tab. Other than that, whitespace is generally ignored so you can format for readability.

The rules are not restricted to being calls to the compiler; you can call any program you want from within make. By creating groups of interdependent dependency-rule sets, you can modify your source code files, type make and be certain that all the affected files will be rebuilt correctly.

A makefile may contain macros (note that these are completely different from C/C++ preprocessor macros). Macros allow convenient string replacement. The makefiles in this book use a macro to invoke the C++ compiler. For example,

The = is used to identify CPP as a macro, and the $ and parentheses expand the macro. In this case, the expansion means that the macro call $(CPP) will be replaced with the string mycompiler. With the macro above, if you want to change to a different compiler called cpp, you just change the macro to:

You can also add compiler flags, etc., to the macro, or use separate macros to add compiler flags.

It becomes tedious to tell make how to invoke the compiler for every single cpp file in your project, when you know it’s the same basic process each time. Since make is designed to be a time-saver, it also has a way to abbreviate actions, as long as they depend on file name suffixes. These abbreviations are called suffix rules. A suffix rule is the way to teach make how to convert a file with one type of extension (.cpp, for example) into a file with another type of extension (.obj or .exe). Once you teach make the rules for producing one kind of file from another, all you have to do is tell make which files depend on which other files. When make finds a file with a date earlier than the file it depends on, it uses the rule to create a new file.

The suffix rule tells make that it doesn’t need explicit rules to build everything, but instead it can figure out how to build things based on their file extension. In this case it says “To build a file that ends in exe from one that ends in cpp, invoke the following command.” Here’s what it looks like for the example above:

The .SUFFIXES directive tells make that it should watch out for any of the following file-name extensions because they have special meaning for this particular makefile. Next you see the suffix rule .cpp.exe, which says “Here’s how to convert any file with an extension of cpp to one with an extension of exe” (when the cpp file is more recent than the exe file). As before, the $(CPP) macro is used, but then you see something new: $<. Because this begins with a ‘$’ it’s a macro, but this is one of make’s special built-in macros. The $< can be used only in suffix rules, and it means “whatever prerequisite triggered the rule” (sometimes called the dependent), which in this case translates to “the cpp file that needs to be compiled.”

Once the suffix rules have been set up, you can simply say, for example, “make Union.exe,” and the suffix rule will kick in, even though there’s no mention of “Union” anywhere in the makefile.

After the macros and suffix rules, make looks for the first “target” in a file, and builds that, unless you specify differently. So for the following makefile:

If you just type ‘make’, then target1.exe will be built (using the default suffix rule) because that’s the first target that make encounters. To build target2.exe you’d have to explicitly say ‘make target2.exe’. This becomes tedious, so you normally create a default “dummy” target that depends on all the rest of the targets, like this:

Here, ‘all’ does not exist and there’s no file called ‘all’, so every time you type make, the program sees ‘all’ as the first target in the list (and thus the default target), then it sees that ‘all’ does not exist so it had better make it by checking all the dependencies. So it looks at target1.exe and (using the suffix rule) sees whether (1) target1.exe exists and (2) whether target1.cpp is more recent than target1.exe, and if so runs the suffix rule (if you provide an explicit rule for a particular target, that rule is used instead). Then it moves on to the next file in the default target list. Thus, by creating a default target list (typically called ‘all’ by convention, but you can call it anything) you can cause every executable in your project to be made simply by typing ‘make’. In addition, you can have other non-default target lists that do other things – for example, you could set it up so that typing ‘make debug’ rebuilds all your files with debugging wired in.

Using the program ExtractCode.cpp from Volume 2 of this book, all the code listings in this book are automatically extracted from the ASCII text version of this book and placed in subdirectories according to their chapters. In addition, ExtractCode.cpp creates several makefiles in each subdirectory (with different names) so you can simply move into that subdirectory and type make -f mycompiler.makefile (substituting the name of your compiler for ‘mycompiler’, the ‘-f’ flag says “use what follows as the makefile”). Finally, ExtractCode.cpp creates a “master” makefile in the root directory where the book’s files have been expanded, and this makefile descends into each subdirectory and calls make with the appropriate makefile. This way you can compile all the code in the book by invoking a single make command, and the process will stop whenever your compiler is unable to handle a particular file (note that a Standard C++ conforming compiler should be able to compile all the files in this book). Because implementations of make vary from system to system, only the most basic, common features are used in the generated makefiles.

As mentioned, the code-extraction tool ExtractCode.cpp automatically generates makefiles for each chapter. Because of this, the makefiles for each chapter will not be placed in the book (all the makefiles are packaged with the source code, which you can download from www.BruceEckel.com). However, it’s useful to see an example of a makefile. What follows is a shortened version of the one that was automatically generated for this chapter by the book’s extraction tool. You’ll find more than one makefile in each subdirectory (they have different names; you invoke a specific one with ‘make -f’). This one is for GNU C++:

The macro CPP is set to the name of the compiler. To use a different compiler, you can either edit the makefile or change the value of the macro on the command line, like this:

Note, however, that ExtractCode.cpp has an automatic scheme to automatically build makefiles for additional compilers.

The second macro OFLAG is the flag that’s used to indicate the name of the output file. Although many compilers automatically assume the output file has the same base name as the input file, others don’t (such as Linux/Unix compilers, which default to creating a file called a.out).

You can see that there are two suffix rules here, one for cpp files and one for .c files (in case any C source code needs to be compiled). The default target is all, and each line for this target is “continued” by using the backslash, up until Guess2, which is the last one in the list and thus has no backslash. There are many more files in this chapter, but only these are shown here for the sake of brevity.

The suffix rules take care of creating object files (with a .o extension) from cpp files, but in general you need to explicitly state rules for creating the executable, because normally an executable is created by linking many different object files and make cannot guess what those are. Also, in this case (Linux/Unix) there is no standard extension for executables so a suffix rule won’t work for these simple situations. Thus, you see all the rules for building the final executables explicitly stated.

This makefile takes the absolute safest route of using as few make features as possible; it only uses the basic make concepts of targets and dependencies, as well as macros. This way it is virtually assured of working with as many make programs as possible. It tends to produce a larger makefile, but that’s not so bad since it’s automatically generated by ExtractCode.cpp.

There are lots of other make features that this book will not use, as well as newer and cleverer versions and variations of make with advanced shortcuts that can save a lot of time. Your local documentation may describe the further features of your particular make, and you can learn more about make from Managing Projects with Make by Oram and Talbott (O’Reilly, 1993). Also, if your compiler vendor does not supply a make or it uses a non-standard make, you can find GNU make for virtually any platform in existence by searching the Internet for GNU archives (of which there are many).

This chapter was a fairly intense tour through all the fundamental features of C++ syntax, most of which are inherited from and in common with C (and result in C++’s vaunted backwards compatibility with C). Although some C++ features were introduced here, this tour is primarily intended for people who are conversant in programming, and simply need to be given an introduction to the syntax basics of C and C++. If you’re already a C programmer, you may have even seen one or two things about C here that were unfamiliar, aside from the C++ features that were most likely new to you. However, if this chapter has still seemed a bit overwhelming, you should go through the CD ROM course Thinking in C: Foundations for C++ and Java (which contains lectures, exercises, and guided solutions), which is bound into this book, and also available at www.BruceEckel.com.

Solutions to selected exercises can be found in the electronic document The Thinking in C++ Annotated Solution Guide, available for a small fee from www.BruceEckel.com.

[30] Note that all conventions seem to end after the agreement that some sort of indentation take place. The feud between styles of code formatting is unending. See Appendix A for the description of this book’s coding style.

[31] Thanks to Kris C. Matson for suggesting this exercise topic.

[32] Unless you take the very strict approach that “all argument passing in C/C++ is by value, and the ‘value’ of an array is what is produced by the array identifier: it’s address.” This can be seen as true from the assembly-language standpoint, but I don’t think it helps when trying to work with higher-level concepts. The addition of references in C++ makes the “all passing is by value” argument more confusing, to the point where I feel it’s more helpful to think in terms of “passing by value” vs. “passing addresses.”