P-stars as "dark matter"

From: Spudboy100@aol.com
Date: Sun Feb 02 2003 - 23:13:01 MST

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    <A HREF="http://xxx.lanl.gov/PS_cache/astro-ph/pdf/0301/0301578.pdf">http://xxx.lanl.gov/PS_cache/astro-ph/pdf/0301/0301578.pdf>

    astro-ph/0301578 [abs, ps, pdf, other] :

    Title: P-Stars
    Authors: Paolo Cea

    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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