Equation of states in the curved spacetime of slowly rotating degenerate stars

被引：3
作者：
Hossain, Golam Mortuza [1 ]
Mandal, Susobhan [1 ]
机构：
[1] Indian Inst Sci Educ & Res Kolkata, Dept Phys Sci, Mohanpur 741246, WB, India
来源：
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2022年 / 10期
关键词：
Quantum fields in curved spacetimes; neutron stars; quantum field theory on curved space; QUANTUM-FIELD-THEORY; RELATIVISTIC STARS; FINITE-TEMPERATURE; NEUTRON-STARS; MAXIMUM MASS; DENSE MATTER;
D O I：
10.1088/1475-7516/2022/10/008
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We compute the equation of state for an ensemble of degenerate fermions by using the curved spacetime of a slowly rotating axially symmetric star. We show that the equation of state computed in such curved spacetime depends on the gravitational time dilation as well as on the dragging of inertial frames, unlike an equation of state computed in a globally flat spacetime. The effect of gravitational time dilation leads to a significant enhancement of the maximum mass limit of a degenerate neutron star. However, such an enhancement due to the frame-dragging effect is extremely small. Nevertheless, in general relativity the frame-dragging effect is crucial for computing angular momentum of the star which is also shown to be enhanced significantly due to the usage of curved spacetime in computing the of state.
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页数：20
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