Decrease in the number of small dark matter haloes due to oscillations in the inflaton potential (2009)
- Authors:
- Autor USP: OPHER, REUVEN - IAG
- Unidade: IAG
- Subjects: MATÉRIA ESCURA; ASTROFÍSICA
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Program & Abstracts
- Conference titles: Workshop on Challenges of New Physics in Space
-
ABNT
RODRIGUES, Luiz Felippe S e OPHER, Reuven. Decrease in the number of small dark matter haloes due to oscillations in the inflaton potential. 2009, Anais.. São Paulo: IAG-USP, 2009. . Acesso em: 19 abr. 2024. -
APA
Rodrigues, L. F. S., & Opher, R. (2009). Decrease in the number of small dark matter haloes due to oscillations in the inflaton potential. In Program & Abstracts. São Paulo: IAG-USP. -
NLM
Rodrigues LFS, Opher R. Decrease in the number of small dark matter haloes due to oscillations in the inflaton potential. Program & Abstracts. 2009 ;[citado 2024 abr. 19 ] -
Vancouver
Rodrigues LFS, Opher R. Decrease in the number of small dark matter haloes due to oscillations in the inflaton potential. Program & Abstracts. 2009 ;[citado 2024 abr. 19 ] - 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
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas