
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^2Learning 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:
This estimates near using the function value and slope at . It is accurate when is close to 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 , 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 is in radians for the trig functions.
Small-angle approximations
For small angles measured in radians,
cos heta approx 1-rac{ heta^2}{2}
These approximations are extremely useful. The simple pendulum equation becomes much easier when , 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 works well for small , but not for large angles. A angle in radians is small, while a 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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