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Taylor series

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A Taylor series is a way to represent a mathematical function as an infinite sum of terms. These terms are built using the function's derivatives at a single specific point. In mathematical analysis, this process allows us to express complex functions using power series. For most common functions, the sum of the series is equal to the function near that starting point. This makes the Taylor series a powerful tool for understanding how functions behave.

sintay SVG
sintay SVG

To understand the mechanism, we must look at how the series is constructed. The series uses the derivatives of a function at a chosen point, often called $a$. The $n$-th derivative is denoted as $f^{(n)}(a)$. Each term in the series includes a factorial, written as $n!$, in the denominator. The formula combines these derivatives with powers of the variable $(x - a)$. When we use the specific point $a = 0$, the series is called a Maclaurin series. This special case was extensively used by Colin Maclaurin during the 18th century.

Exp series
Exp series

We often cannot use an infinite sum in practical calculations. Instead, we use a partial sum called a Taylor polynomial. A Taylor polynomial of degree $n$ uses only the first few terms of the series. These polynomials act as approximations of the original function. As the degree $n$ increases, the polynomial generally becomes more accurate. We can use Taylor's theorem to find quantitative estimates of the error. This error is known as the remainder, denoted as $R_n(x)$.

Second Order Taylor
Second Order Taylor

History shows that Brook Taylor introduced these series in 1715. The development of these tools changed how mathematicians approached complex problems. Before these series, working with non-polynomial functions was much more difficult. The ability to turn functions into sums of powers allowed for easier calculation. Later, Nicholas Mercator published work on the natural logarithm in 1668. His specific expansion is known as the Mercator series. These historical contributions built the foundation for modern mathematical analysis.

There are many distinct types of series for different mathematical functions. The exponential function has a Maclaurin series that converges for all values of $x$. The natural logarithm has a series that converges for specific intervals. The binomial series is another important type, using generalized binomial coefficients. Trigonometric functions like sine and cosine also have their own series. These expansions often involve special constants, such as Bernoulli numbers or Euler numbers.

Exp neg inverse square
Exp neg inverse square

Not every function behaves the same way when using a Taylor series. A function is called analytic at a point if it equals its Taylor series in an open interval. Some functions are "entire," meaning they are equal to their Taylor series across the whole complex plane. Examples of entire functions include polynomials and the exponential function. However, other functions have a limit called a radius of convergence. If you try to use the series too far from the starting point, the series will diverge. This means the sum will no longer accurately represent the function.

Taylor series connect to many broad fields in mathematics and science. They allow mathematicians to perform differentiation and integration term by term. This makes complex calculus operations much simpler to solve. In complex analysis, Taylor series help extend functions into the complex plane. They are also used in statistical thermodynamics through polylogarithmic functions. Even in computer science, systems use these series to compute function values numerically. By turning curves into polynomials, we can navigate the most complex mathematical landscapes.

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Exp series.gif
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