Revisiting the hot matter in the center of gamma-ray bursts and supernova
arXiv:1305.2530 · doi:10.1051/0004-6361/201321705
Abstract
Hot matter with nucleons can be produced in the inner region of the neutrino-dominated accretion flow in gamma-ray bursts or during the proto-neutron star birth in successful supernova. The composition and equation of state of the matter depend on the dynamic equilibrium under various neutrino opacities. The strong interaction between nucleons may also play an important role. We plan to extend the previous studies by incorporating these two aspects in our model. The modification of the -equilibrium condition from neutrino optically thin to thick has been modeled by an equilibrium factor ranging between the neutrino-freely-escaping case and the neutrino-trapped case. We employ the microscopic Brueckner-Hartree-Fock approach extended to the finite temperature regime to study the interacting nucleons. We show that the composition and chemical potentials of the hot nuclear matter for different densities and temperatures at each stage of equilibrium. We also compare our realistic equation of states with those of the free gas model. We find the neutrino opacity and the strong interaction between nucleons are important for the description and should be taken into account in model calculations.
accepted Astronomy & Astrophysics (2013)
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- Jet Luminosity of Gamma-ray Bursts: Blandford-Znajek Mechanism v.s. Neutrino Annihilation Process
- Relativistic global solutions of neutrino-dominated accretion flows
- Nucleon effective mass in hot dense matter
- Testing black hole neutrino-dominated accretion discs for long-duration gamma-ray bursts
- Self-gravity in neutrino-dominated accretion disks
- Evolutions of stellar-mass black hole hyperaccretion systems in the center of gamma-ray bursts
- Variability of the giant X-ray bump in GRB 121027A and possible origin
- Vertical convection in neutrino-dominated accretion flows
- Anisotropic neutrinos and gravitational waves from black hole neutrino-dominated accretion flows in fallback core-collapse supernovae
- Relativistic global solutions of neutrino-dominated accretion flows with magnetic coupling