Abstract mathematical symbols and equations representing physics mathematics

Taylor series and approximations

PHYS 110 · Differential Equations and Series

Taylor series approximate functions near a point using polynomials. This lesson explains linearization, small-angle approximations, and why approximation is central in physics.

Key equations

f(x) \approx f(a) + f'(a)(x-a)f(x)=f(a)+f'(a)(x-a)+\frac{f''(a)}{2!}(x-a)^2+\frac{f'''(a)}{3!}(x-a)^3+\cdotse^x = 1+x+\frac{x^2}{2!}+\frac{x^3}{3!}+\cdots\sin x = x-\frac{x^3}{3!}+\frac{x^5}{5!}-\cdots\cos x = 1-\frac{x^2}{2!}+\frac{x^4}{4!}-\cdots\sin\theta \approx \theta\tan\theta \approx \thetaU(x) \approx U_0 + \frac{1}{2}kx^2

Learning objectives

  • Explain Taylor series as polynomial approximations.
  • Use linear approximation near a point.
  • Apply small-angle approximations in radians.
  • Describe why approximations are essential in physics.

Why approximations matter

Physics often deals with systems that are too complicated to solve exactly. Approximation is not a failure; it is one of the most powerful scientific strategies. A good approximation captures the important behavior while ignoring details that are too small to matter in the situation.

Taylor series provide a systematic way to approximate functions using polynomials. Polynomials are easier to calculate, differentiate, and integrate than many other functions.

Linear approximation

The simplest approximation is the tangent-line approximation:

f(x)approxf(a)+f(a)(xa)f(x) approx f(a) + f'(a)(x-a)

This estimates f(x)f(x) near x=ax=a using the function value and slope at aa. It is accurate when xx is close to aa and the function does not curve too sharply.

In physics, linear approximations appear whenever changes are small. A spring force is approximately linear near equilibrium. A complicated potential energy function may look like a parabola near a stable minimum.

Taylor series

A Taylor series includes higher-order derivative information:

f(x)=f(a)+f'(a)(x-a)+ rac{f''(a)}{2!}(x-a)^2+ rac{f'''(a)}{3!}(x-a)^3+cdots

If a=0a=0, the series is often called a Maclaurin series:

f(x)=f(0)+f'(0)x+ rac{f''(0)}{2!}x^2+ rac{f'''(0)}{3!}x^3+cdots

Each additional term can improve accuracy near the expansion point.

Important series

Some common Maclaurin series are:

e^x = 1+x+ rac{x^2}{2!}+ rac{x^3}{3!}+cdots

sin x = x- rac{x^3}{3!}+ rac{x^5}{5!}-cdots

cos x = 1- rac{x^2}{2!}+ rac{x^4}{4!}-cdots

These assume xx is in radians for the trig functions.

Small-angle approximations

For small angles measured in radians,

sinhetaapproxhetasin heta approx heta

cos heta approx 1- rac{ heta^2}{2}

anhetaapproxheta an heta approx heta

These approximations are extremely useful. The simple pendulum equation becomes much easier when sinhetaapproxhetasin heta approx heta, allowing pendulum motion to be modeled as simple harmonic motion for small swings.

Estimating error

Approximations have limits. The farther you move from the expansion point, the less accurate a short Taylor approximation may become. Higher-order terms indicate the possible size of neglected effects.

For example, using sinhetaapproxhetasin heta approx heta works well for small heta heta, but not for large angles. A 5circ5^circ angle in radians is small, while a 60circ60^circ angle is not.

Physics near equilibrium

Taylor series explain why so many systems behave like harmonic oscillators near stable equilibrium. Near a minimum of potential energy, the first derivative is zero and the leading nonconstant term is often quadratic:

U(x) approx U_0 + rac{1}{2}kx^2

This leads to a restoring force proportional to displacement.

The big idea

Taylor series approximate complicated functions with polynomials built from derivatives. They justify linearization, small-angle approximations, and many simplified physics models. Approximation is not guessing carelessly; it is controlled reasoning about which terms matter most in a given situation.

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