Stability window and mass–radius relation for magnetized strange quark stars
نویسندگان
چکیده
منابع مشابه
Dynamical stability of strange quark stars
The necessary and sufficient condition for dynamical stability is worked out for the sequences of relativistic star models corresponding to the well defined and causal values of adiabatic sound speed, √ (dP/dE)0 = v0, at the centre. On the basis of these conditions, we show that the mass-radius (M −R) relation corresponding to the MIT bag models of strange quark matter (SQM) and the models obta...
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ژورنال
عنوان ژورنال: Journal of Physics G: Nuclear and Particle Physics
سال: 2009
ISSN: 0954-3899,1361-6471
DOI: 10.1088/0954-3899/36/7/075202