P-Stars

Details P-Stars P-Stars

2003-01-29

arxiv.org/abs/astro-ph/0301578v2

Int.J.Mod.Phys. D13 (2004) 1917-1926

Astronomy and Astrophysics

Astrophysics

12 pages, 3 figures, revised version, to appear in IJMPD

Scientific paper

10.1142/S0218271804005833

P-Stars are a new class of compact stars made of up and down quarks in beta-equilibrium with electrons in an Abelian chromomagnetic condensate. We show that P-Stars are able to account for compact stars with R < 6 Km, as well as stars with radius comparable with canonical Neutron Stars. We find that cooling curves of P-Stars compare rather well with observational data. We suggest that P-Matter produced at the primordial deconfinement transition is a viable candidate for baryonic Cold Dark Matter. Finally, we show that P-Stars are able to overcome the gravitational collapse even for mass much greater than 10^6 Solar Mass.

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