Change in the cosmic photon to neutrino temperature ratio and primordial nucleosynthesis due plasmons in the early universe (1993)
- Authors:
- Autor USP: OPHER, REUVEN - IAG
- Unidade: IAG
- Assunto: ASTRONOMIA
- Language: Inglês
- Imprenta:
- Publisher: Inpe/Fapesp/Finep/Banco do Brasil
- Publisher place: São Paulo
- Date published: 1993
- Source:
- Título: Proceedings
- Conference titles: Encontro Brasileiro de Fisica dos Plasmas
-
ABNT
OPHER, M e OPHER, Reuven. Change in the cosmic photon to neutrino temperature ratio and primordial nucleosynthesis due plasmons in the early universe. 1993, Anais.. São Paulo: Inpe/Fapesp/Finep/Banco do Brasil, 1993. . Acesso em: 24 jan. 2026. -
APA
Opher, M., & Opher, R. (1993). Change in the cosmic photon to neutrino temperature ratio and primordial nucleosynthesis due plasmons in the early universe. In Proceedings. São Paulo: Inpe/Fapesp/Finep/Banco do Brasil. -
NLM
Opher M, Opher R. Change in the cosmic photon to neutrino temperature ratio and primordial nucleosynthesis due plasmons in the early universe. Proceedings. 1993 ;[citado 2026 jan. 24 ] -
Vancouver
Opher M, Opher R. Change in the cosmic photon to neutrino temperature ratio and primordial nucleosynthesis due plasmons in the early universe. Proceedings. 1993 ;[citado 2026 jan. 24 ] - Summary talk X Latin American Workshop on Plasma Physics November 30,2003-December 5,2003 - Sâo Pedro,S.P.,Brazil
- Razao da temperatura de radiacao de fundo a temperatura dos neutrinos de fundo devido aos plasmons no universo primordial
- Mudancas nas abundancias primordiais devido as flutuacoes eletromagneticas no plasma primordial
- Origin of intergalactic magnetic fields due to extragalactic jets
- Decay of the vacuum energy into cosmic microwave background photons
- Origin of magnetic fields in galaxies
- Modelo simplificado de criacao de vazios em grande escala pela explosao de supernovas primordiais
- Influencia de defeitos topologicos sobre a nucleossintese primordial
- Influence of a primordial magnetic field on the baryon mass fraction of small haloes
- Generalized noncommutative inflation
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