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.
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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 $(\gamma - 1)mc^2$.