Hyperon stars at finite temperature in the Brueckner theory
arXiv:1101.0726 · doi:10.1103/PhysRevC.83.025804
Abstract
We perform Brueckner-Hartree-Fock calculations of hypernuclear matter at finite temperature and provide convenient analytical parametrizations of the results. We study then the properties of (proto)neutron stars containing hyperons. We find important effects of trapping and finite temperature on the structure of hyperonic stars.
6 pages, 5 figures, accepted for publication in Phys. Rev. C
References in corpus (9)
- Neutron Star Observations: Prognosis for Equation of State Constraints
- Dimension as a Key to the Neutrino Mechanism of Core-Collapse Supernova Explosions
- Hadron-quark mixed phase in hyperon stars
- Tables of Hyperonic Matter Equation of State for Core-Collapse Supernovae
- Hybrid protoneutron stars with the MIT bag model
- Evolutionary sequences of rotating protoneutron stars
- Quark matter in neutron stars within the Nambu - Jona-Lasinio model and confinement
- Protoneutron stars in the Brueckner-Hartree-Fock approach and finite-temperature kaon condensation
- Isothermal vs. isentropic description of protoneutron stars in the Brueckner-Bethe-Goldstone theory
Cited by in corpus (66)
- Equations of state for supernovae and compact stars
- Neutron Stars and the Nuclear Equation of State
- Do hyperons exist in the interior of neutron stars ?
- Maximum mass of neutron stars and strange neutron-star cores
- Hyperons in neutron-star cores and two-solar-mass pulsar
- Superfluidity in nuclear systems and neutron stars
- Antinuclei in Heavy-Ion Collisions
- Equation of state of hypernuclear matter: impact of hyperon--scalar-meson couplings
- Too massive neutron stars: The role of dark matter?
- A new temperature dependent hyperonic equation of state: application to rotating neutron star models and I-Q-relations
- Internal X-ray plateau in short GRBs: Signature of supramassive fast-rotating quark stars?
- Equation of state of dense nuclear matter and neutron star structure from nuclear chiral interactions
- Neutron star equation of state from the quark level in the light of GW170817
- Ab Initio Description of p-Shell Hypernuclei
- Phase transitions in dense matter and the maximum mass of neutron stars
- On the Maximum Mass of Neutron Stars
- Hyperons in neutron stars and supernova cores
- Cooling of hypernuclear compact stars
- (1232) effects in density-dependent relativistic Hartree-Fock theory and neutron stars
- Hyperons: the strange ingredients of the nuclear equation of state
- An extended equation of state for core-collapse simulations
- Hybrid equation of state approach in binary neutron-star merger simulations
- EoS for massive neutron stars
- Constraining hadron-quark phase transition parameters within the quark-mean-field model using multimessenger observations of neutron stars
- Microscopic equation of state of hot nuclear matter for numerical relativity simulations
- Equations of state for hot neutron stars -- II. The role of exotic particle degrees of freedom
- Massive hybrid stars with a first order phase transition
- Hybrid protoneutron stars with the Dyson-Schwinger quark model
- Astrophysical implications on hyperon couplings and hyperon star properties with relativistic equations of states
- Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence
- Oscillations of hot, young neutron stars: Gravitational wave frequencies and damping times
- Thermal states of neutron stars with a consistent model of interior
- Hot neutron stars with microscopic equations of state
- Nucleon effective mass in hot dense matter
- Structures of the Vela pulsar and the glitch crisis from the Brueckner theory
- New equation of states for postmerger supramassive quark stars
- Extended quark mean-field model for neutron stars
- Anisotropic pressure and hyperons in neutron stars
- Tidal deformability of strange stars and the GW170817 event
- Phenomenological QCD equations of state for neutron star dynamics: Nuclear-2SC continuity and evolving effective couplings
- Binary neutron star merger simulations with hot microscopic equations of state
- Hyperons in Neutron Stars
- Solution to the hyperon puzzle using dark matter
- Structure of the hadron-quark mixed phase in protoneutron stars
- Phase transition towards strange matter
- Nonrelativistic nucleon effective masses in nuclear matter: BHF versus RHF
- Quark mean-field model for single and double and hypernuclei
- Setting nonperturbative uncertainties on finite-temperature properties of neutron matter
- Hot neutron stars and their equation of state
- Microscopic nuclear equation of state at finite temperature and stellar stability
- Nuclear matter at finite temperature and static properties of proto-neutron star
- Liquid-gas phase transition in strange hadronic matter with relativistic models
- Parameters of rotating neutron stars with and without hyperons
- Amorphous state in the mixed phase of quark-hadron phase transition in protoneutron stars
- Revisiting the hot matter in the center of gamma-ray bursts and supernova
- Kaon-meson condensation and resonance in hyperonic stellar matter within a relativistic mean-field model
- Hadron-Quark Phase Transitions in Hyperon Stars
- Probing the impact of Delta-Baryons on Nuclear Matter and Non-Radial Oscillations in Neutron Stars
- Exploring -resonance in neutron stars: implications from astrophysical and nuclear observations
- Thermal behavior of the mass and residue of hyperons
- The phase transition in hot hypernuclei within relativistic Thomas-Fermi approximation
- Equation of State of Hot Neutron Star Matter using Finite Range Simple Effective Interaction
- Quark stars in - holographic model
- Effects of Phi and -meson on properties of hyperon stars including resonance
- Exploring Hyperon Skyrme Forces in Multi- Hypernuclei and Neutron Star Matter
- Effect of chiral nuclear forces on the neutrino mean free path in hot neutron matter