Effects of new long-range interaction: Recombination of relic Heavy neutrinos and antineutrinos

dc.creatorBelotsky, K. M.
dc.creatorKhlopov, M. Yu.
dc.creatorLegonkov, S. V.
dc.creatorShibaev, K. I.
dc.date2005-04-27
dc.date.accessioned2026-07-07T06:23:57Z
dc.date.available2026-07-07T06:23:57Z
dc.descriptionIf stable Heavy neutrinos of 4th generation possess their own Coulomb-like interaction, recombination of pairs of Heavy neutrinos and antineutrinos can play important role in their cosmological evolution and lead to observable consequences. In particular, effect of this new interaction in the annihilation of neutrino-antineutrino pairs can account for $γ$-flux observed by EGRET.
dc.description10 pages, 4 figures; Invited talk at 6 International Conference on Cosmoparticle physics "Cosmion 2004"
dc.identifierhttps://arxiv.org/abs/astro-ph/0504621
dc.identifierhttp://arxiv.org/abs/astro-ph/0504621
dc.identifierGrav.Cosmol. 11 (2005) 27-33
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/96383
dc.subjectAstrophysics
dc.titleEffects of new long-range interaction: Recombination of relic Heavy neutrinos and antineutrinos
dc.typetext

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