So a function is like a machine, that takes values of x and returns an output y. The set of all values that x can have is called the domain. The set that contains every value that y can have is called the codomain.
If this happens, we say that y is a function of x, and we write y =f(x). f is the name of the function and one writes (function from X to Y) to represent the three parts of the function: the domain (x), the codomain (y) and the pairing process (the arrow).
An example of a function is f(x)=x+1 One gives a natural number (0,1,2,3...) as the input and gets a natural number , which is +1 (1,2,3,4...) The idea of a function has been set up to cover all sorts of possibilities. The function doesn't have to be an equation. The main idea is that inputs and outputs are paired up somehow even if the process is very complicated.
Metaphors[change | change source]
Tables[change | change source]
The inputs and outputs can be put in a table like the picture; this is easy if there is not too much data.
Graphs[change | change source]
In the picture it can be seen that both 2 and 3 have been paired with c; this is not allowed in the other direction, 2 could not output c and d,each input can only have one output. All of the (c and d in the picture) are usually called the image set of and the image set can be all of the codomain or not. One can say that the subset A of the codomain with the image set is f(A). If the inputs and outputs have an order it is easy to plot them on a graph: In that way the image come on the image of the set A. This will make a both of 2 and 3 have paired with is not allowed in the other direction,even one can make between codomain or not. A conclusion can be made that subset A of the codomain is the image set is F(A).
History[change | change source]
In 1748 Leonhard Euler gave: "A function of a variable quantity is an analytic expression composed in any way whatsoever of the variable quantity and numbers or constant quantities." and then in 1755: "If some quantities so depend on other quantities that if the latter are changed the former undergoes change, then the former quantities are called functions of the latter. This definition applies rather widely and includes all ways in which one quantity could be determined by other. If, therefore, x denotes a variable quantity, then all quantities which depend upon x in any way, or are determined by it, are called functions of x." which is very modern.
Usually, Dirichlet is credited with the version used in schools until the second half of the 20th century: "y is a function of a variable x, defined on the interval a < x < b, if to every value of the variable x in this interval there corresponds a definite value of the variable y. Also, it is irrelevant in what way this correspondence is established."
In 1939, the Bourbaki generalized the Dirichlet definition and gave a set theoretic version of the definition as a correspondence between inputs and outputs; this was used in schools from about 1960.
Finally in 1970, the Bourbaki gave the modern definition as a triple , with (i.e. and ).
Types of functions[change | change source]
- Elementary functions - The functions that are usually studied in school: fractions, square roots, the sine, cosine and tangent functions and some other functions.
- Non-elementary functions - Most of them do not use operations that we don't learn in school (like + or -, or powers). Many integrals are non-elementary.
- Inverse functions - Functions that undo another function. For example: if F(x) is the inverse of f(x)=y, then F(y)=x. Not all functions have inverses.
- Special functions: Functions that have names. For example: sine, cosine and tangent. Functions like f(x)=3x (three times x) are not called special functions. They can be elementary, non-elementary or inverses.