Cyclotron Emissivity in the Early Universe

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dc.creatorSegre, Gino
dc.date1998-03-23
dc.date.accessioned2026-07-07T04:03:38Z
dc.date.available2026-07-07T04:03:38Z
dc.descriptionPrimordial magnetic fields present between the eras of neutrino decoupling and of positron-electron annihilation can lead to the emission of neutrino-anti neutrino pairs or axions by electrons in excited Landau levels, thereby changing the electron energy spectrum. The rate is calculated and shown to not affect significantly the standard Big Bang picture.
dc.description7 pages
dc.identifierhttps://arxiv.org/abs/hep-ph/9803430
dc.identifierhttp://arxiv.org/abs/hep-ph/9803430
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/47745
dc.subjectHigh Energy Physics - Phenomenology
dc.titleCyclotron Emissivity in the Early Universe
dc.typetext

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