We study different stages of the neutron star cooling by computing neutron star properties at various temperatures and entropies using an effective chiral model including hadronic and quark degrees of freedom. Macroscopic properties of the star such as mass and radius are calculated and compared with...
The dynamics of the interior of the neutron star is important to understand a rich variety of phenomena, such as observed spin glitches, thermal evolution, waves and oscillations, and diversified instabilities8. In this regard, the importance of hydrodynamic instabilities in such neutron stars has b...
A novel scenario is proposed for the origin of cosmological γ-ray bursts relating them with the induced collapse of an isolated neutron star under the action of a primordial black hole inside it. A mechanism is pointed out for black hole capturing into bounded orbits in a contracting protostel...
Neutron star mergers also create black holes, and AT2017gfo created the smallest one ever observed, though there’s some doubt. The gravitational wave GW170817 is associated with the kilonova and was detected by LIGO in August 2017. It was the first time a GW event was seen ...
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a ball of matter so dense that atomic electrons 一个球形物质,密度非常高,以致于原子的电子 collapse from their quantum orbits into the depths of atomic nuclei. 会从它们的量子轨道落到原子核的深处。 The death of that star is the birth of a neutron star: ...
A 3D illustration of a neutron star in the nebula. (Image credit: Shutterstock) Neutron stars are the remnants of giant stars that died in a fiery explosion known as a supernova. After such an outburst, the cores of these former stars compact into an ultradense object with the mass of...
We consider electrostatic plasma modes along the open field lines of a rotating neutron star. Goldreich-Julian charge density in general relativity is analyzed for the neutron star with zero inclination. It is found that the charge density is maximum at the polar cap and remains almost the same...
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