Dark quark `stars': do they matter for Ω_matter?

Details Dark quark `stars': do they matter for Ω_matter? Dark quark `stars': do they matter for Ω_matter?

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ssrv..100..175k&link_type=abstract

Space Science Reviews, v. 100, Issue 1/4, p. 175-192 (2002).

Physics

Scientific paper

The structure of a spherically symmetric stable dark `star' is discussed, at zero temperature, containing 1) a core of quarks in the deconfined phase and antileptons 2) a shell of hadrons in particular n, p, Λ and Σ^- and leptons or antileptons and 3) a shell of hydrogen in the superfluid phase. If the superfluid hydrogen phase goes over into the electromagnetic plasma phase at densities well below one atom (10 fm)^3, as is usually assumed, the hydrogen shell is insignificant for the mass and the radius of the `star'. These quantities are then determined approximatively: mass = 1.8 solar masses, radius = 9.2 km.

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