Brown dwarfs, quark stars, and quark-hadron phase transition

Details Brown dwarfs, quark stars, and quark-hadron phase transition Brown dwarfs, quark stars, and quark-hadron phase transition

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994phrvl..73.1328c&link_type=abstract

Physical Review Letters, Volume 73, Issue 10, September 5, 1994, pp.1328-1331

Physics

22

Low Luminosity Stars, Subdwarfs, And Brown Dwarfs, Quark-Gluon Plasma, Dark Matter

Scientific paper

It is shown that within an effective model of QCD, the Lee-Wick model, bodies with quark content of mass of the order of 10-2 to one solar mass can be formed at a temperature T~1 MeV much lower than the quark-hadron phase transition temperature. This ensures their stability until the present epoch, and we suggest that they can be identified with the dark objects observed recently by gravitational microlensing.

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