Diquark condensation effects on hot quark star configurations

Oztas A., Blaschke D., Fredriksson S., Grigorian H.

NATO Advanced Research Workshop on Superdense QCD Matter and Compact Stars, Yerevan, Armenia, 27 September - 04 October 2003, vol.197, pp.341-351 identifier

  • Publication Type: Conference Paper / Full Text
  • Volume: 197
  • City: Yerevan
  • Country: Armenia
  • Page Numbers: pp.341-351
  • Hacettepe University Affiliated: No


The equation of state for quark matter is derived for a nonlocal, chiral quark model within the mean field approximation. We investigate the effects of a variation of the form-factors of the interaction on the phase diagram of quark matter. Special emphasis is on the occurrence of a diquark condensate which signals a phase transition to color superconductivity and its effects on the equation of state under the condition of beta- equilibrium and charge neutrality. We calculate the quark star configurations by solving the Tolman-Oppenheimer-Volkoff equations and obtain for the transition from a hot, normal quark matter core of a protoneutron star to a cool diquark condensed one a release of binding energy of the order of Delta Mc(2) similar to 10(53) erg. We find that this energy could not serve as an engine for explosive phenomena since the phase transition is not first order. Contrary to naive expectations the mass defect increases when for a given temperature we neglect the possibility of diquark condensation.