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Kinetic Energy

Overview

$$E_\mathrm{kin} = \frac{1}{2}mv^2$$

Introduction

Kinetic energy is defined as the ability of an object to carry out work due to its mechanical motion. Every moving object, such as a falling stone, a driving car, or a planet orbiting around a star, has a certain amount of kinetic energy. This form of energy is, therefore, called energy of motion. Kinetic energy is stored in a moving object and can be converted into other energy forms like heat through friction or transferred to other objects during collisions.

Constant Acceleration

In the first step, we want to derive a formula for the kinetic energy for a constant acceleration $a$. In this case, the energy can simply be calculated according to $$E = Fs$$ where $F$ is the driving force and $s$ is the distance. In the next step, we can replace the force with Newton's second law $F=ma$ which leads to $$E = mas$$ For constant acceleration, we can use the previously derived quadratic relation between the distance and time which is given as $s = \frac{1}{2}at^2$. The result is then given as $$E = \frac{1}{2}ma^2t^2$$ If the body is accelerated with $a$, it reaches the speed $v$ after the time $t = v/a$. After inserting this relation into the equation above, the acceleration cancels out and the following equation remains: $$\boxed{E = \frac{1}{2}mv^2}$$ This equation is the famous formula for calculating the kinetic energy of an object after a certain acceleration takes place.

General Derivation

Now we want to show that we can obtain the same formula when we drop the condition of a constant acceleration, but rather consider any arbitrary trajectory. If an object undergoes an acceleration $\vec{a}$, the definition of the energy can be rewritten as follows: $$E = \int_0^\vec{r} \vec{F}\cdot\mathrm{d}\vec{r} = \int_0^\vec{r} m\vec{a}\cdot\mathrm{d}\vec{r}$$ In the next step, the acceleration $\vec{a}$ can be replaced with its definition $\mathrm{d}\vec{v}/\mathrm{d}t$ which leads to the following equation: $$E = m\int_0^t \frac{\mathrm{d}\vec{v}}{\mathrm{d}t}\cdot\mathrm{d}\vec{r}$$ The mass $m$ is a constant and can therefore be drawn in front of the integral. If the derivation of the velocity with respect to time is treated as an ordinary fraction, the denominator $\mathrm{d}t$ can be shifted to the right. Together with the replacement $\vec{v} = \mathrm{d}\vec{r}/\mathrm{d}t$, the integrand becomes $$E = \int_0^\vec{v} m \vec{v}\cdot\mathrm{d}\vec{v}$$ Now, the product rule can be applied. Therefore, only the absolute value of the velocity remains that can easily be integrated to $$\boxed{E_\mathrm{kin} = \frac{1}{2}mv^2}$$ This formula describes the energy of motion of a body that has been accelerated speed until it reaches the velocity $v$ and is therefore called kinetic energy.
Kinetic Energy


The kinetic energy of an object with the mass $m$ moving with the speed $v$ is given as $$E_\mathrm{kin} = \frac{1}{2}mv^2$$

This formula can be applied for a speed $v$ which is much smaller than the speed of light. If $v$ gets too large (around 10% of c), then the approximation gets worse and formulas from the theory of relativity have to be used. This subject will be discussed at a later stage.
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