Instantaneous Power Radiated from Magnetic Dipole Moments
arXiv:1407.1274 · doi:10.1016/j.astropartphys.2014.07.005
Abstract
We compute the power radiated per unit solid angle of a moving magnetic dipole moment, and its instantaneous radiated power, both non-relativistically and relativistically. This is then applied to various interesting situations: solar neutrons, electron synchrotrons and cosmological Dirac neutrinos. Concerning the latter, we show that hypothesized early-universe Big Bang conditions allow for neutrino radiation cooling and provide an energy loss-mechanism for subsequent neutrino condensation.
arXiv comment12 pages, 1 figure, Accepted for publication in Astroparticle Physics
References in corpus (4)
Cited by in corpus (6)
- Charged particle motion and radiation in strong electromagnetic fields
- Instantaneous Radiation from Time-Varying Electric and Magnetic Dipoles
- Strong fields and neutral particle magnetic moment dynamics
- Dark Matter in the Local Group of Galaxies
- The vector potential of a point magnetic dipole
- Classical neutral point particle in linearly polarized EM plane wave field