Quark deconfinement and neutrino trapping in compact stars
arXiv:nucl-th/0411051 · doi:10.1088/0954-3899/31/6/079
Abstract
We study the role played by neutrino trapping on the hadron star (HS) to quark star (QS) conversion mechanism proposed recently by Berezhiani and collaborators. We find that the nucleation of quark matter drops inside hadron matter, and therefore the conversion of a HS into a QS, is strongly inhibit by the presence of neutrinos.
arXiv comment3 pages, 3 figures. Talk given at the VIII International Conference on Strangeness in Quark Matter. Cape Town, South Africa, Septembre 2004
References in corpus (6)
- Quark deconfinement and implications for the radius and the limiting mass of compact stars
- Gamma Ray Bursts from delayed collapse of neutron stars to quark matter stars
- Effects of hyperons on the dynamical deconfinement transition in cold neutron star matter
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Cited by in corpus (8)
- Burning of an hadronic star into a quark or a hybrid star
- Quark matter nucleation in neutron stars and astrophysical implications
- Effects of color superconductivity on the nucleation of quark matter in neutron stars
- Metastability of hadronic compact stars
- Effects of quark matter nucleation on the evolution of proto-neutron stars
- Dense stellar matter with trapped neutrinos under strong magnetic fields
- Could the compact remnant of SN 1987A be a quark star?
- Numerical Simulation of the Hydrodynamical Combustion to Strange Quark Matter in the Trapped Neutrino Regime