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Self-bound models of compact stars and recent mass-radius measurements
Self-bound models compact stars recent mass-radius measurements
2011/10/20
The exact composition of a specific class of compact stars, historically referred to as "neutron stars", is still quite unknown. Possibilities ranging from hadronic to quark degrees of freedom, includ...
The formation and evolution of compact stars in binaries。
In an earlier analysis it was demonstrated that general relativity
gives higher values of surface tension in strange stars with quark
matter than neutron stars.We generate the modified Tolman–Oppenh...
In an earlier analysis it was demonstrated that general relativity gives higher values of surface tension in strange stars with quark matter than neutron stars.We generate the modified Tolman–Oppenhei...