Strong neutrino cooling by cycles of electron capture and `beta-´ decay in neutron star crusts (2013)
- Autores:
- Autor USP: GASQUES, LEANDRO ROMERO - IF
- Unidade: IF
- Assuntos: REAÇÕES NUCLEARES; ASTROFÍSICA; ÍONS PESADOS
- Idioma: Inglês
- Resumo: The temperature in the crust of an accreting neutron star, which comprises its outermost kilometer, is set by heating from nuclear reactions at large densities,1–4 neutrino cooling,5, 6 and heat transport from the interior.7–11 The heated crust has been thought to a ect observable phenomena at shallower depths, such as thermonuclear bursts in the accreted envelope.10, 11.
- Imprenta:
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ABNT
SCHATZ, H et al. Strong neutrino cooling by cycles of electron capture and `beta-´ decay in neutron star crusts. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: http://lanl.arxiv.org/pdf/1312.2513v1.pdf. Acesso em: 24 set. 2024. , 2013 -
APA
Schatz, H., Gupta, S., Moller, P., Beard, M., Brown, E. F., Deibel, A. T., et al. (2013). Strong neutrino cooling by cycles of electron capture and `beta-´ decay in neutron star crusts. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de http://lanl.arxiv.org/pdf/1312.2513v1.pdf -
NLM
Schatz H, Gupta S, Moller P, Beard M, Brown EF, Deibel AT, Gasques LR, Hix WR, Keek L, Lau R, Steiner AW, Wiescher M. Strong neutrino cooling by cycles of electron capture and `beta-´ decay in neutron star crusts [Internet]. 2013 ;[citado 2024 set. 24 ] Available from: http://lanl.arxiv.org/pdf/1312.2513v1.pdf -
Vancouver
Schatz H, Gupta S, Moller P, Beard M, Brown EF, Deibel AT, Gasques LR, Hix WR, Keek L, Lau R, Steiner AW, Wiescher M. Strong neutrino cooling by cycles of electron capture and `beta-´ decay in neutron star crusts [Internet]. 2013 ;[citado 2024 set. 24 ] Available from: http://lanl.arxiv.org/pdf/1312.2513v1.pdf - Investigation of the role of shell structure in quasi-fission mass distributions
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