Do hyperons exist in the interior of neutron stars?
By D. Chatterjee, Isaac Vidaña. 2015
222 citations recorded by the source corpus.
Abstract.In this work we review the role of hyperons on the properties of neutron and proto-neutron stars. In particular, we revise the so-called “hyperon puzzle”, go over some of the solutions proposed to tackle it, and discuss the implications that the recent measurements of unusually high neutron star masses have on our present knowledge of hypernuclear physics. We re-examine also the role of hyperons on the cooling properties of newly born neutron stars and on the so-called r-mode instability.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/7a7256cf99944a8eb05fa7691783db96bb64ab9b
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In Astronomy and Astrophysics
- Diego Rubiera-García
- Aneta Wojnar
- Armen Sedrakian
- John W. Clark Jr.
- G. Olmo
- Valerio Faraoni
- Tiberiu Harko
- Francisco S. N. Lobo
Citations in the corpus
- Stellar structure models in modified theories of gravity: Lessons and challenges (2019, background): “Among the many difficulties related to this extrapolation one finds that, at large enough densities, it is energetically favourable for some of the nucleons to combine to form hyperons which, yielding softer EOS, would reduce the maximum neutron mass thus producing a tension between nuclear physics ”
- Superfluidity in nuclear systems and neutron stars (2018, methodology): “See Chatterjee and Vidaña (2016); Oertel et al. (2017) and references therein.”