Neutron-star tidal deformability and equation-of-state constraints
نویسندگان
چکیده
منابع مشابه
Pulsar Constraints on Neutron Star Structure and Equation of State
The sudden spin jumps, or glitches, commonly seen in isolated neutron stars are thought to represent angular momentum transfer between the crust and the liquid interior [1]. In this picture, as a neutron star’s crust spins down under magnetic torque, differential rotation develops between the stellar crust and a portion of the liquid interior. The more rapidly rotating component then acts as an...
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ژورنال
عنوان ژورنال: General Relativity and Gravitation
سال: 2020
ISSN: 0001-7701,1572-9532
DOI: 10.1007/s10714-020-02754-3