Probing the metastability of protoneutron star with hyperon in core-collapse supernova
arXiv:1401.0369 · doi:10.1103/PhysRevC.89.035807
Abstract
We investigate the role of hyperons in the dynamical collapse of a non-rotating massive star to a black hole(BH) using one dimensional general relativistic code. We follow the dynamical formation and evolution of a protoneutron star (PNS) to a black hole using various progenitor models, adopting a hyperonic equation of state (EoS) generated by Shen et. al. We compare the results with those of nuclear EoS by Shen et. al. and understand the role of strange hyperons in the core collapse supernova. We discuss the neutrino signals that may be used as a probe to core collapse. Further, an exotic EoS can support a much lower maximum mass cold neutron star compared to PNS. In this regard, we also study the metastability of PNS in the presence of hyperon in the long-time evolution of the progenitors, relevant to supernova SN1987A.
References in corpus (6)
- Shapiro delay measurement of a two solar mass neutron star
- A Massive Pulsar in a Compact Relativistic Binary
- Nucleosynthesis and Remnants in Massive Stars of Solar Metallicity
- Proto-Neutron and Neutron Stars in a Chiral SU(3) Model
- Tables of Hyperonic Matter Equation of State for Core-Collapse Supernovae
- Double- hypernuclei in the relativistic mean-field theory
Cited by in corpus (9)
- Nuclear Equation of state for Compact Stars and Supernovae
- Equation of State and Progenitor Dependence of Stellar-Mass Black-Hole Formation
- Massive Neutron Stars with Antikaon Condensates in a Density Dependent Hadron Field Theory
- The in neutron stars - a new degree of freedom?
- Equation of State table with hyperon and antikaon for supernova and neutron star merger
- A Comparative study of hyperon equations of state in supernova simulations
- Thermal behavior as indicator for hyperons in binary neutron star merger remnants
- Hyperons and quarks in proto-neutron stars
- Neutron Stars: Laboratories for fundamental physics under extreme astrophysical conditions