Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8132876 | Astroparticle Physics | 2015 | 5 Pages |
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.
Related Topics
Physical Sciences and Engineering
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Authors
P.D. Morley, D.J. Buettner,