Definition:Kinetic Energy of Classical Particle
Should be a result page not a definition page.
Until this has been finished, please leave {{refactor}} in the code.
New contributors: Refactoring is a task which is expected to be undertaken by experienced editors only. Because of the underlying complexity of the work needed, it is recommended that you do not embark on a refactoring task until you have become familiar with the structural nature of pages of $\mathsf{Pr} \infty \mathsf{fWiki}$.
Definition
Let $\MM$ be an $n$-dimensional Euclidean manifold.
Let $P$ be a particle with an inertial mass $m_i$.
Let $t$ be the time variable of $P$.
Suppose the position of $P$ is a real differentiable $n$-dimensional vector-valued mapping $\mathbf x = \map {\mathbf x} t$.
Then the kinetic energy of a classical particle $P$ is:
- $T = \dfrac {m_i} 2 \paren {\dfrac {\d \mathbf x} {\d t} }^2$
where $\paren {\dfrac {\d \mathbf x} {\d t} }^2$ is the dot product of the vector $\dfrac {\d \mathbf x} {\d t}$ with itself.
Sources
- 1963: I.M. Gelfand and S.V. Fomin: Calculus of Variations ... (previous) ... (next): $\S 4.21$: The Principle of Least Action
