Constraints on the critical temperature of the phase transition to the quark-gluon plasma.

Details Constraints on the critical temperature of the phase transition to the quark-gluon plasma. Constraints on the critical temperature of the phase transition to the quark-gluon plasma.

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992svjnp..55..914k&link_type=abstract

Sov. J. Nucl. Phys., Vol. 55, No. 6, p. 914 - 916

Physics

Scientific paper

Low temperatures of the phase transition to the quark-gluon plasma correspond to low values of the bag model constant and to absolutely stable strange quark matter. Some of the observed pulsars are identified quite reliably as neutron stars. If strange matter is stable, the central density of these pulsars has to be smaller than the critical density of the phase transition to nonstrange quark matter. The nonstrange quark matter being formed turns to more stable strange matter on a weak interaction timescale, converting neutron stars into strange stars. The requirement of stability of old and newly born neutron stars is used to constrain the bag model constant and the critical temperature of the phase transition to the quark-gluon plasma at zero chemical potential.

Affiliated with

Also associated with

No associations

Rating

Constraints on the critical temperature of the phase transition to the quark-gluon plasma. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Constraints on the critical temperature of the phase transition to the quark-gluon plasma., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Constraints on the critical temperature of the phase transition to the quark-gluon plasma. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1524797