Total energy in special relativity includes both the rest energy and the kinetic energy of an object. It is given by the equation $E = \gamma mc^2$, where $\gamma$ is the Lorentz factor, $m$ is the rest mass, and $c$ is the speed of light.
5 Must Know Facts For Your Next Test
The total energy combines both rest energy and kinetic energy.
In relativistic physics, total energy is given by $E = \gamma mc^2$.
The Lorentz factor $\gamma$ accounts for time dilation and length contraction at high velocities.
As velocity approaches the speed of light, total energy increases without bound.
Rest mass ($m_0$) remains constant, but relativistic mass increases with velocity.
A factor that describes how much time dilates and lengths contract at velocities close to the speed of light, defined as $\gamma = \frac{1}{\sqrt{1 - (v^2/c^2)}}$.
Relativistic Kinetic Energy: The additional energy possessed by an object due to its motion, calculated as $(\gamma - 1)mc^2$.