Results 161 to 170 of about 2,365,879 (310)
Two-flavor Color Superconducting Quark Stars May Not Exist
Large uncertainties in the determinations of the equation of state of dense stellar matter allow for the intriguing possibility that the bulk quark matter in beta equilibrium might be the true ground state of the matter at zero pressure.
Wen-Li Yuan, Ang Li
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Strange matter in compact stars
We discuss possible scenarios for the existence of strange matter in compact stars. The appearance of hyperons leads to a hyperon puzzle in ab-initio approaches based on effective baryon-baryon potentials but is not a severe problem in relativistic mean ...
Klähn Thomas, Blaschke David B.
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Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars
We construct a set of equations of state (EoS) of dense and hot matter with a 1st order phase transition from a hadronic system to a deconfined quark matter state. In this two-phase approach, hadrons are described using the relativistic mean field theory
Mateusz Cierniak +4 more
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Quark matter symmetry energy effect on equation of state for neutron stars [PDF]
Xuhao Wu, Akira Ohnishi, Hong Shen
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Light Dark Matter Through the Quark Axial-Vector Current Portal [PDF]
Dillon Berger
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The Strange Prospects for Astrophysics
The implications of the formation of strange quark matter in neutron stars and in core-collapse supernovae is discussed with special emphasis on the possibility of having a strong first order QCD phase transition at high baryon densities.
A Mezzacappa +17 more
core +1 more source
Collapsing strange quark matter in Vaidya geometry [PDF]
T. Harko, K.S. Cheng
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J. P. Carlomagno +3 more
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In asymptotically dense quark matter, colored glue forces cause an unusual variant of superconductivity. Instead of pairing, the quarks clump in groups of six. We investigate the gap equation in the weak coupling limit, and find the leading behavior of the energy gap and the critical temperature as functions of the renormalized coupling constant.
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Quark matter — Facts and hopes [PDF]
Abstract The aim is to study nuclear matter under extreme conditions. The hope is that conditions reached in present relativistic heavy ion collisions are adequate for the formation of a quark-gluon plasma where colour would no longer be confined to hadronic dimensions. The situation prior to the “Quark Matter '88” conference is reviewed.
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