Neutron star instabilities in full general relativity using aΓ=2.75ideal fluid
نویسندگان
چکیده
منابع مشابه
Gravitational waves from axisymmetric rotating stellar core collapse to a neutron star in full general relativity
Axisymmetric numerical simulations of rotating stellar core collapse to a neutron star are performed in the framework of full general relativity. The so-called Cartoon method, in which the Einstein field equations are solved in the Cartesian coordinates and the axisymmetric condition is imposed around the y = 0 plane, is adopted. The hydrodynamic equations are solved in the cylindrical coordina...
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ژورنال
عنوان ژورنال: Physical Review D
سال: 2014
ISSN: 1550-7998,1550-2368
DOI: 10.1103/physrevd.90.024034