A unified model for ultra high energy cosmic rays (1998)
- Authors:
- Autor USP: OPHER, REUVEN - IAG
- Unidade: IAG
- Subjects: ASTRONOMIA; RAIOS CÓSMICOS
- Language: Inglês
- Imprenta:
- Publisher: World Scientific
- Publisher place: Singapura
- Date published: 1998
- Source:
- Título: Proceedings
- Conference titles: Texas Symposium on Relativistic Astrophysics and Cosmology
-
ABNT
OPHER, Erella e OPHER, Reuven. A unified model for ultra high energy cosmic rays. 1998, Anais.. Singapura: World Scientific, 1998. . Acesso em: 18 jan. 2026. -
APA
Opher, E., & Opher, R. (1998). A unified model for ultra high energy cosmic rays. In Proceedings. Singapura: World Scientific. -
NLM
Opher E, Opher R. A unified model for ultra high energy cosmic rays. Proceedings. 1998 ;[citado 2026 jan. 18 ] -
Vancouver
Opher E, Opher R. A unified model for ultra high energy cosmic rays. Proceedings. 1998 ;[citado 2026 jan. 18 ] - Impact of primordial magnetic fields on the gas content of dark matter halos
- Origin of '10 POT. 15 - 10 POT. 16' G magnetic fields in the central engine of gamma ray bursts
- The origin of magnetic fields in galaxies
- Decrease in the number of small dark matter haloes due to oscillations in the inflaton potential
- Decrease in the number of small dark matter haloes due to oscillations in the inflation potential
- Inflation with inflatons
- What is the susy mass scale?
- Collapse of primordial clouds - I
- Distorcao da radiacao cosmica de fundo no cenario explosivo para a criacao de vazios em grande escala
- Origin of '10 POT. 15 - 10 pot. 16' magnetic fields in the central engine of gamma ray bursts
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