Is there a crisis in neutron star physics? (2013)
- Authors:
- Autor USP: HORVATH, JORGE ERNESTO - IAG
- Unidade: IAG
- Subjects: ESTRELAS DE NEUTRONS; ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Publisher: SLAC National Accelerator Laboratory
- Publisher place: Mento Park
- Date published: 2013
- Source:
- Título: CSQCD III : Proceedings
- Conference titles: Conference on Compact Stars in the QCD Phase Diagram
-
ABNT
HORVATH, Jorge Ernesto e BENVENUTO, O. G. Is there a crisis in neutron star physics? 2013, Anais.. Mento Park: SLAC National Accelerator Laboratory, 2013. Disponível em: http://slac.stanford.edu/econf/C121212/pdf/1307.1832v1.pdf. Acesso em: 16 mar. 2026. -
APA
Horvath, J. E., & Benvenuto, O. G. (2013). Is there a crisis in neutron star physics? In CSQCD III : Proceedings. Mento Park: SLAC National Accelerator Laboratory. Recuperado de http://slac.stanford.edu/econf/C121212/pdf/1307.1832v1.pdf -
NLM
Horvath JE, Benvenuto OG. Is there a crisis in neutron star physics? [Internet]. CSQCD III : Proceedings. 2013 ;[citado 2026 mar. 16 ] Available from: http://slac.stanford.edu/econf/C121212/pdf/1307.1832v1.pdf -
Vancouver
Horvath JE, Benvenuto OG. Is there a crisis in neutron star physics? [Internet]. CSQCD III : Proceedings. 2013 ;[citado 2026 mar. 16 ] Available from: http://slac.stanford.edu/econf/C121212/pdf/1307.1832v1.pdf - Evolution of primordial black holes in a radiation and phantom energy environment
- The stifness of the supranuclear equation of state (once again)
- Bayesian evidence for two populations of white dwarfs: Preliminary Results
- On the mass distribution of neutron stars
- Some possible dynamical constraints for life´s origin
- Progenitors and SNR associated to SGR/AXPs
- Maximum mass of magnetic white dwarfs
- Entropy, disequilibrium and complexity in compact stars: an information theory approach to understand their composition
- Color-flavor locked strange matter
- Primordial nuggets survival and QCD pairing
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