Theory of relativity
Relativistic momentum and energy, E = mc²
Energy and momentum form the four-momentum; rest mass is invariant and satisfies the energy–momentum relation.
An object of rest mass m moving at speed v has momentum p=γmv and total energy E=γmc². Its rest energy E₀=mc² remains when it is at rest.
Definition: Definition
The energy–momentum four-vector is . Its invariant gives . For a photon m=0 and ; a massive particle’s kinetic energy is .
Physical meaning
Avoid calling γmc² “relativistic mass” when m denotes invariant rest mass. Keeping mass and energy distinct makes conservation laws consistent across frames.
Example: Worked example
A proton has rest mass m and momentum p=mc. Find its total energy in units of mc² and its kinetic energy.
Solution
The relation gives , so . Thus .
Example: Relativistic kinetic energy
A particle with rest energy moves at . Find its momentum in units of and its kinetic energy in .
Solution
. Thus and . The kinetic energy is ; indeed .
The four-momentum has Minkowski norm in the time-negative signature. This yields , valid for massive particles and for photons when . The mass is invariant; it does not increase with speed, so the phrase “relativistic mass” can obscure the distinction between mass and energy. In a center-of-momentum frame, total momentum vanishes, yet the system’s energy can still contribute to its invariant mass.
In a collision, each particle’s kinetic energy need not be conserved, but the total four-momentum of an isolated system is. The final products’ rest energy can differ from the initial total rest energy because initial kinetic energy may become new rest mass. For a photon, because its invariant mass is zero, yet it carries energy and momentum. Two counter-propagating photons can form a system with nonzero invariant mass.
Quick check
A particle has invariant mass m and momentum p=mc. What is its total energy?
Which quantity is invariant under Lorentz transformations?
References
- Edwin F. Taylor, John Archibald Wheeler (1992). Spacetime Physics
- Robert Resnick (1968). Introduction to Special Relativity