Dilatonic equation of hydrostatic equilibrium and neutron star structure
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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The structure of neutron stars is considered from theoretical and observational perspectives. We demonstrate an important aspect of neutron star structure: the neutron star radius is primarily determined by the behavior of the pressure of matter in the vicinity of nuclear matter equilibrium density. In the event that extreme softening does not occur at these densities, the radius is virtually i...
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ژورنال
عنوان ژورنال: Astrophysics and Space Science
سال: 2015
ISSN: 0004-640X,1572-946X
DOI: 10.1007/s10509-015-2429-x