Challenges of relativistic astrophysics (2012)
- Autor:
- Autor USP: OPHER, REUVEN - IAG
- Unidade: IAG
- Subjects: ASTROFÍSICA; BURACOS NEGROS; ESTRELAS DE NEUTRONS; MATÉRIA ESCURA; UNIVERSO PRIMORDIAL; JATOS (ASTRONOMIA); RAIOS CÓSMICOS; CAMPO MAGNÉTICO
- Language: Inglês
- Imprenta:
- Publisher: Instituto Nacional de Pesquisas Espaciais
- Publisher place: São José dos Campos
- Date published: 2012
- Source:
- Título do periódico: Proceedings
- Conference titles: Texas Symposium on Relativistic Astrophysics
-
ABNT
OPHER, Reuven. Challenges of relativistic astrophysics. 2012, Anais.. São José dos Campos: Instituto Nacional de Pesquisas Espaciais, 2012. Disponível em: http://www.das.inpe.br/texas2012sp/portugues/program.php#plenary10. Acesso em: 19 abr. 2024. -
APA
Opher, R. (2012). Challenges of relativistic astrophysics. In Proceedings. São José dos Campos: Instituto Nacional de Pesquisas Espaciais. Recuperado de http://www.das.inpe.br/texas2012sp/portugues/program.php#plenary10 -
NLM
Opher R. Challenges of relativistic astrophysics [Internet]. Proceedings. 2012 ;[citado 2024 abr. 19 ] Available from: http://www.das.inpe.br/texas2012sp/portugues/program.php#plenary10 -
Vancouver
Opher R. Challenges of relativistic astrophysics [Internet]. Proceedings. 2012 ;[citado 2024 abr. 19 ] Available from: http://www.das.inpe.br/texas2012sp/portugues/program.php#plenary10 - Where does the gravitational energy and angular momentum go in the formation of stars?
- Study of the Casimir energy in an expanding finiteuniverse
- Origem e amplificação de campos magnéticos primordiais
- Studying the decay of the vacuum energy with the observed density power spectrum
- Origin of the intense magnetic fields in magnetars, quasars and GRBS
- Matter density fluctuations in the running 'lâmbda'CDM and 'lâmbda'XCDM models
- Magnetic fields in gamma-ray burst afterglows
- Generalized noncommutative inflation
- Origin of '10 POT. 15 - 10 pot. 16' magnetic fields in the central engine of gamma ray bursts
- Polarized radiation from am herculis binaries
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