128 Relativistic Kinetic Energy Formula Derivation
A derivation of the relativistic kinetic energy formula that is used to obtain \(K_{\mathrm{rel}} = (\gamma - 1)mc^{2}\) from the work done by a force.
definition [d] (Relativistic Kinetic Energy Formula Derivation) From OpenStax: the relativistic kinetic energy follows from the work-energy theorem. With force
- \(\mathbf{F} = \dfrac{d\mathbf{p}}{dt} = m\dfrac{d(\gamma\mathbf{u})}{dt}\) ,
the work that accelerates a particle from rest to final speed \(u\) is, in one dimension,
- \(K = \displaystyle\int F\, dx = m\displaystyle\int u\,\dfrac{d}{dt}\!\left(\dfrac{u}{\sqrt{1-\left(\dfrac{u}{c}\right)^{2}}}\right) dt\) .
Integrating by parts from rest to speed \(u\) gives
- \(K = \dfrac{mu^{2}}{\sqrt{1-\left(\dfrac{u}{c}\right)^{2}}} - m\displaystyle\int\dfrac{u}{\sqrt{1-\left(\dfrac{u}{c}\right)^{2}}}\, du\) ,
- \(K = \dfrac{mu^{2}}{\sqrt{1-\left(\dfrac{u}{c}\right)^{2}}} + mc^{2}\sqrt{1-\left(\dfrac{u}{c}\right)^{2}}\Big|_{0}^{u}\) ,
- \(K = \dfrac{mc^{2}}{\sqrt{1-\left(\dfrac{u}{c}\right)^{2}}} - mc^{2}\) ,
hence
- \(K_{\mathrm{rel}} = (\gamma - 1)mc^{2}\) ,
with
- \(\gamma = \dfrac{1}{\sqrt{1-\dfrac{u^{2}}{c^{2}}}}\) .
At low speed, the binomial approximation \(\gamma \approx 1 + \dfrac{1}{2}\left(\dfrac{u^{2}}{c^{2}}\right)\) yields
- \(K_{\mathrm{rel}} \approx \dfrac{1}{2}mu^{2} = K_{\mathrm{class}}\) .
where
- \(\mathbf{F}\) is the force.
- \(F\) is the one-dimensional force component.
- \(\mathbf{p}\) is the relativistic momentum.
- \(t\) is time.
- \(dt\) is the time differential.
- \(m\) is the rest mass.
- \(\gamma\) is the Lorentz factor.
- \(\mathbf{u}\) is the velocity.
- \(u\) is the particle speed.
- \(c\) is the speed of light in vacuum.
- \(dx\) is the displacement differential.
- \(du\) is the speed differential.
- \(K\) is the work integral equal to the gained kinetic energy.
- \(K_{\mathrm{rel}}\) is the relativistic kinetic energy.
- \(K_{\mathrm{class}}\) is the Newtonian kinetic energy.
- \(\displaystyle\int F\, dx\) is the work done by the force.
128.1 Elementary Example
128.1.1 Simple
At \(u = 0\), one has \(\gamma = 1\), so
\[ K_{\mathrm{rel}} = (1 - 1)mc^{2} = 0 \]
where
- \(u\) is the particle speed.
- \(\gamma\) is the Lorentz factor.
- \(K_{\mathrm{rel}}\) is the relativistic kinetic energy.
- \(m\) is the rest mass.
- \(c\) is the speed of light in vacuum.
128.1.2 General
An electron with speed \(u = 0.990c\) has \(\gamma = 7.0888\), so
\[ K_{\mathrm{rel}} = (\gamma - 1)mc^{2} = 3.12\,\mathrm{MeV} \]
where
- \(u\) is the electron speed.
- \(c\) is the speed of light in vacuum.
- \(\gamma\) is the Lorentz factor.
- \(m\) is the electron rest mass.
- \(K_{\mathrm{rel}}\) is the relativistic kinetic energy.
128.2 References
- OpenStax. University Physics Volume 3, §5.9 Relativistic Energy. — \(K=\int F\,dx\) with \(F=\dfrac{dp}{dt}\) yields \(K_{\mathrm{rel}}=(\gamma-1)mc^{2}\); electron example at \(u=0.990c\). https://openstax.org/books/university-physics-volume-3/pages/5-9-relativistic-energy
- Annihilation
- Constancy of the Speed of Light
- Contracted Length
- Coordinate Transformations
- Elastic Potential Energy Formula Derivation
- Electromagnetic Field Transformations
- Field Tensor
- Frame
- Gravitational Potential Energy Formula Derivation
- Inertial Frame
- Inertial Reference Frames
- Kinetic Energy
- Kinetic Energy Formula Derivation
- Length Contraction
- Lorentz Factor
- Lorentz Transformations
- Magnetism as a Relativistic Effect
- Mass-Energy Equivalence
- Massless Particles
- Minkowski Metric
- Minkowski Space
- Moving Clocks
- Newtonian Kinetic Energy Formula Derivation
- Nuclear Energy
- Particle Creation
- Photon Energy
- Potential Energy
- Potential Energy Formula Derivation
- Principle of Relativity
- Proper Length
- Proper Time
- Reference Frames
- Relativistic Electrodynamics
- Relativistic Kinetic Energy Formula Derivation
- Relativistic Momentum
- Relativistic Momentum and Energy
- Relativity Principle
- Rest Energy
- Simultaneity
- Time Dilation
- Twin Paradox