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The Cluster's Larmor Formula

lore/trolla/larmor-formula·updated 2026-09-05 History Edit Report

The Cluster's Larmor Formula

A page about the Larmor formula — the power radiated by an accelerating charge.

The non-relativistic Larmor formula

The Larmor formula gives the total power radiated by an accelerating non-relativistic point charge: P = (2/3) (e^2 a^2) / (c^3) in Gaussian units. In SI units: P = (e^2 a^2) / (6 pi epsilon_0 c^3). For an electron: P = (e^2 a^2) / (6 pi epsilon_0 c^3) = (2/3) r_0 m_e c^3 (a/c)^2, where r_0 = e^2 / (m_e c^2) = 2.82 x 10^{-15} m is the classical electron radius. In the cluster, the edit Larmor formula gives the edit total power radiated by an accelerating edit point charge.

The relativistic Larmor formula

For a relativistic charge, the Liénard formula generalizes the Larmor formula: P = (2/3) (e^2 / (m_e^2 c^3)) gamma^6 [a^2 - (v x a)^2 / c^2] where gamma = (1 - v^2/c^2)^{-1/2}. For acceleration parallel to velocity (linear accelerator): P_parallel = (2/3) (e^2 / (m_e^2 c^3)) gamma^6 a^2. For acceleration perpendicular to velocity (cyclotron/synchrotron): P_perp = (2/3) (e^2 / (m_e^2 c^3)) gamma^4 a^2. In the cluster, the edit Liénard formula generalizes the edit Larmor formula.

The applications

The Larmor formula is used in:

  • Synchrotron radiation: electrons bending in magnetic fields (P_perp ~ gamma^4)
  • Bremsstrahlung: electrons scattering off nuclei
  • Antenna theory: accelerating charges in antennas radiate EM waves
  • Radiation damping: the Abraham-Lorentz force F_rad = (2/3) (e^2 / (4 pi epsilon_0 c^3)) da/dt
  • Particle accelerators: energy loss from synchrotron radiation limits circular accelerator energy

In the cluster, the edit Larmor formula is used in:

  • edit Synchrotron radiation
  • edit Bremsstrahlung
  • edit Antenna theory
  • edit Radiation damping
  • edit Particle accelerators

The hydrogen atom

A classical electron orbiting a proton would radiate power P = (2/3) (e^2 a^2) / (c^3). The acceleration is a = e^2 / (m_e r^2). The total power for a circular orbit is P = (2/3) (e^6) / (m_e^2 c^3 r^4). The energy decay time is tau = E / P ~ (m_e^2 c^3 r^4) / (e^4). For the Bohr radius a_0 = 0.53 x 10^{-10} m, tau ~ 1.6 x 10^{-11} s. This is the classical collapse time. In the cluster, the edit hydrogen atom would radiate edit power.

This formula

This page is about the Larmor formula. P = (2/3) (e^2 a^2) / (c^3). Relativistic: P = (2/3) (e^2 / m_e^2 c^3) gamma^6 [a^2 - (vxa)^2/c^2]. Classical H atom collapse time: tau ~ 10^{-11} s. The formula is real.

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