Chapter 3: Energy-Momentum Relation

The energy-momentum relation is the fundamental equation connecting energy, momentum, and mass. It's the relativistic version of the kinetic energy formula and reveals the deep connection between these quantities.

The Energy-Momentum Relation

\( E^2 = (pc)^2 + (mc^2)^2 \)

The "mass shell" condition—true for all free particles

At Rest (p = 0)

$E = mc^2$ (rest energy)

Massless (m = 0)

$E = pc$ (photons)

General

\( E = \gamma mc^2 \)

pcEE² = (pc)² + (mc²)²massive (hyperbola)E = pcmassless (asymptote)rest: E = mc²Mass shell is a hyperbola in (pc, E) space; photons travel along the asymptote E = pc.

Relativistic Kinetic Energy

\( K = E - mc^2 = (\gamma - 1)mc^2 \)

Total energy minus rest energy

At low speeds (v ≪ c), expanding γ - 1 ≈ v²/2c² gives:

\( K \approx \frac{1}{2}mv^2 \) (classical result)

The Dispersion Relation

In quantum mechanics, E = ℏω and p = ℏk. The energy-momentum relation becomes:

\( \omega^2 = c^2k^2 + \frac{m^2c^4}{\hbar^2} \)

This is the Klein-Gordon dispersion relation, fundamental to relativistic quantum field theory.

Interactive Simulations

Energy-Momentum Relation: E^2 = (pc)^2 + (mc^2)^2

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Fortran: Energy-Momentum Dispersion Relation

Fortran
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