Constraints for the binding energy of strange matter implied by existence of massive neutron stars

Details Constraints for the binding energy of strange matter implied by existence of massive neutron stars Constraints for the binding energy of strange matter implied by existence of massive neutron stars

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991nuphs..24..134k&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 24, Issue 2, p. 134-138.

Physics

Nuclear Physics

Scientific paper

Some of the observed pulsars can be identified with ordinary neutron stars. If strange matter is stable, the central density of the neutron stars should be lower than the critical density of the quark-hadron phase transition occurring due to the strong interactions only. The quark matter being formed turns to more stable strange matter on a weak interaction time scale, converting neutron stars into strange stars. The requirement of stability of old and newly born hot neutron stars with respect to the phase transition is used to constrain the binding energy of strange matter.

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