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

DOI10.1088/1475-7516/2022/10/008OpenAlexW4300864155MaRDI QIDQ5042579

Golam Mortuza Hossain, Susobhan Mandal

Publication date: 20 October 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2204.12352

zbMATH Keywords

neutron starsquantum field theory on curved spacequantum fields in curved spacetimes

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Nuclear physics (81V35) Quantum field theory on curved space or space-time backgrounds (81T20) Galactic and stellar structure (85A15) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Motion of the gyroscope (70E05) Local deformation theory, Artin approximation, etc. (14B12) Fermionic systems in quantum theory (81V74)

Related Items (1)

Origin of primeval seed magnetism in rotating astrophysical bodies

Cites Work

• Unnamed Item
• Basics of thermal field theory. A tutorial on perturbative computations
• Rotating quantum states
• A New Approach to Quantum-Statistical Mechanics
• Equation of states in the curved spacetime of spherical degenerate stars
• Static Solutions of Einstein's Field Equations for Spheres of Fluid
• On Massive Neutron Cores

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