R-mode constraints from neutron star equation of state
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: HNPS Proceedings
سال: 2019
ISSN: 2654-0088,2654-007X
DOI: 10.12681/hnps.1913