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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 spin parameter of uniformly rotating compact stars
spin parameter of uniformly compact stars
2010/12/21
We study the dimensionless spin parameter j (= cJ/(GM2)) of uniformly rotating neutron stars
and quark stars in general relativity. We show numerically that the maximum value of the spin
parameter o...
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...
Gravitomagnetic Effects on Collective Plasma Oscillations in Compact Stars
gravitomagnetism compact stars plasma osillations
2007/8/15
2006Vol.45No.3pp.568-572DOI:
Gravitomagnetic Effects on Collective Plasma Oscillations in Compact Stars
Babur M. Mirza1 and Hamid Saleem2,3
1 Department of Mathematics, ...
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...