The simplest functions are lineal functions. Their formulas are polynomials with degree one or cero (this is the case when the function is the constant function). Their graphs are straight lines. A formula for these lineal functions is: We usually call it the slopeintercept form, where b is the yintercept and m is the slope. The slope, also called the gradient of the line, measures the degree of inclination of the line with the horizontal, the xaxis. The slope of a line characterizes the general direction in which a line points. The yintercept of a function is the point at which the graph of the function crosses the yaxis. (the x value equals 0 ). The yintercept of a linear function is: When b is positive, the line crosses the yaxis somewhere above the xaxis (y=0) and if b is negative, the line crosses the yaxis below the xaxis. A line is completely determined by any two distinct points along it. If (x_{0}, y_{0}) and (x_{1}, y_{1}) are two points (x_{0} not equal x_{1}) on a given line we can calculate the slope of the line: Notice that when the slope, m, is positive, the line slants upward to the right. The more positive m is, the steeper the line will slant upward to the right. When the slope is negative, the line slants downward to the right, and, as the slope becomes more and more negative, the line will slant downward steeper and steeper to the right. This is an example of a linear function with a negative slope: Horizontal lines have slope=0. All horizontal lines are of the form y = k (where k is some number). As a function, we call it a constant function. Vertical lines have no slope. They are not function at all. Note that if we try to calculate the slope we end up trying to divide by 0. In applications, if we know that the functional relation between the variables is characterized by a constant rate of change, then the underlying function is linear and its slope measures this rate of change. This information can be exploited to write down a formula for the function. The line thorugh P(x_{0}, y_{0}) with slope m is given by the pointslope form: We can rearrange to write it as a function: We can write the equation of the line though two points: That has the advantage that we do not need to divide. We can arrive at the general form (this algebraic form has an important advantage because it include vertical lines x = k, where k is some real number): The xintercept of a linear function is the point where the graph of the line crosses the xaxis. A nonhorizontal line always have one xintercept. To find the xintercept we need to solve the equation This solution of the equation is called a root of the polynomial. In general, a function can have several xintercepts. Then the xintercept of a linear function (with m not equal to 0) is:
The simplest example of a Lagrange Polynomial is, of course, the linear function through two points. We can write this linear function as a simple example of a Lagrange Polynomial: REFERENCES
Michael Spivak, Calculus, Third Edition, PublishorPerish, Inc.
Tom M. Apostol, Calculus, Second Edition, John Willey and Sons, Inc.
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Power with natural exponents are simple and important functions. Their inverse functions are power with rational exponents (a radical or a nth root)
Polynomials of degree 3 are cubic functions. A real cubic function always crosses the xaxis at least once.
We can consider the polynomial function that passes through a series of points of the plane. This is an interpolation problem that is solved here using the Lagrange interpolating polynomial.
Lagrange polynomials are polynomials that pases through n given points. We use Lagrange polynomials to explore a general polynomial function and its derivative.
If the derivative of F(x) is f(x), then we say that an indefinite integral of f(x) with respect to x is F(x). We also say that F is an antiderivative or a primitive function of f.
The integral concept is associate to the concept of area. We began considering the area limited by the graph of a function and the xaxis between two vertical lines.
Monotonic functions in a closed interval are integrable. In these cases we can bound the error we make when approximating the integral using rectangles.
If we consider the lower limit of integration a as fixed and if we can calculate the integral for different values of the upper limit of integration b then we can define a new function: an indefinite integral of f.
It is easy to calculate the area under a straight line. This is the first example of integration that allows us to understand the idea and to introduce several basic concepts: integral as area, limits of integration, positive and negative areas.
To calculate the area under a parabola is more difficult than to calculate the area under a linear function. We show how to approximate this area using rectangles and that the integral function of a polynomial of degree 2 is a polynomial of degree 3.
We can see some basic concepts about integration applied to a general polynomial function. Integral functions of polynomial functions are polynomial functions with one degree more than the original function.
The Fundamental Theorem of Calculus tell us that every continuous function has an antiderivative and shows how to construct one using the integral.
The Second Fundamental Theorem of Calculus is a powerful tool for evaluating definite integral (if we know an antiderivative of the function).
As an introduction to Piecewise Linear Functions we study linear functions restricted to an open interval: their graphs are like segments.
A piecewise function is a function that is defined by several subfunctions. If each piece is a constant function then the piecewise function is called Piecewise constant function or Step function.
A continuous piecewise linear function is defined by several segments or rays connected, without jumps between them.
Complex power functions with natural exponent have a zero (or root) of multiplicity n in the origin.
A polynomial of degree 2 has two zeros or roots. In this representation you can see Cassini ovals and a lemniscate.
The function is not defined for values less than 1. Taylor polynomials about the origin approximates the function between 1 and 1.
The function has a singularity at 1. Taylor polynomials about the origin approximates the function between 1 and 1.
The function has a singularity at 1. Taylor polynomials about the origin approximates the function between 1 and 1.
This function has two real singularities at 1 and 1. Taylor polynomials approximate the function in an interval centered at the center of the series. Its radius is the distance to the nearest singularity.
