Confinement, Quark Matter Equation of State and Hybrid Stars

Details Confinement, Quark Matter Equation of State and Hybrid Stars Confinement, Quark Matter Equation of State and Hybrid Stars

1995-10-24

arxiv.org/abs/hep-ph/9510391v1

Mod.Phys.Lett. A10 (1995) 2651-2663

Physics

High Energy Physics

High Energy Physics - Phenomenology

15 pages, revtex, 7 figures (available on request) (To appear in Mod. Phys. Lett. A)

Scientific paper

10.1142/S0217732395002787

We consider here quark matter equation of state in a relativistic harmonic confinement model at zero temperature. The same is considered to study phase transition of neutron matter to quark matter at high densities. This, along with a phenomenological equation of state in the neutron matter sector is used to study hybrid stars. Using Tolman Oppenheimer Volkoff equations, stable solutions for hybrid stars are obtained with a maximum mass of 1.98 $M_\odot$ and radii around 10 kms with a quark core of about 1 to 2 kilometers.

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