Abstract mathematical symbols and equations representing physics mathematics

Inverse functions

PHYS 110 · Algebra and Functions

Inverse functions reverse the action of functions. This lesson explains how inverses work algebraically, graphically, and physically.

Key equations

f(x) = yf^{-1}(y) = xf(x) = 3x + 2f^{-1}(x) = \frac{x - 2}{3}x(t) = vtt(x) = \frac{x}{v}f^{-1}(x) = \sqrt{x}

Learning objectives

  • Define an inverse function conceptually.
  • Find inverses of simple algebraic functions.
  • Explain why one-to-one functions are needed for inverses.
  • Interpret inverse functions in physical contexts.

What an inverse function does

An inverse function reverses another function. If a function takes an input xx and produces an output yy, the inverse takes that output yy and returns the original input xx.

If

f(x)=yf(x) = y

then the inverse function satisfies

f1(y)=xf^{-1}(y) = x

The notation f1f^{-1} means inverse function, not reciprocal. This is an important distinction. In general, f1(x)f^{-1}(x) does not mean 1/f(x)1/f(x).

A simple example

Consider

f(x)=3x+2f(x) = 3x + 2

This function multiplies by 3 and then adds 2. To find the inverse, reverse those steps. Start with

y=3x+2y = 3x + 2

Subtract 2:

y2=3xy - 2 = 3x

Divide by 3:

x = rac{y - 2}{3}

Now switch variable names if desired:

f^{-1}(x) = rac{x - 2}{3}

The inverse subtracts 2 and then divides by 3.

Inverses in physics

In physics, inverse functions appear whenever you want to solve a relationship in the opposite direction. If position is given as a function of time, x(t)x(t), you might want to know the time when the object reaches a certain position. That requires an inverse relationship, at least over a suitable interval.

For example, if

x(t)=vtx(t) = vt

with constant positive velocity, then

t(x) = rac{x}{v}

The original function answers: where is the object at time tt? The inverse answers: when does the object reach position xx?

One-to-one requirement

Not every function has an inverse over its entire domain. A function must be one-to-one, meaning each output comes from only one input. If two different inputs produce the same output, the inverse would not know which input to return.

For example,

f(x)=x2f(x) = x^2

is not one-to-one over all real numbers because f(2)=4f(2)=4 and f(2)=4f(-2)=4. The output 4 corresponds to two inputs. To define an inverse, we often restrict the domain. If we use only xgeq0x geq 0, then the inverse is

f1(x)=sqrtxf^{-1}(x) = sqrt{x}

This idea matters in physics because physical context often selects the correct branch. Speed may be nonnegative, time may be positive, and distance may be restricted.

Graphing inverses

The graph of an inverse function is the reflection of the original graph across the line

y=xy = x

This happens because inputs and outputs switch roles. A point (a,b)(a,b) on the original function corresponds to (b,a)(b,a) on the inverse.

This graphical view helps you understand why a function that fails the horizontal line test does not have a full inverse. If a horizontal line crosses the original graph more than once, then one output corresponds to multiple inputs.

Inverse trig and inverse exponentials

Many important inverse functions appear in physics. Logarithms are inverses of exponentials. Inverse trigonometric functions, such as sin1(x)sin^{-1}(x), help find angles from ratios. Square roots are inverses of squaring when the domain is restricted.

For example, if

sin( heta) = rac{opposite}{hypotenuse}

then

ight)$$ ## The big idea Inverse functions reverse relationships. In physics, they let you switch from predicting an output to finding the input that caused it. Understanding inverses helps with solving equations, interpreting graphs, finding times from positions, finding angles from trig ratios, and solving exponential models with logarithms.

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