Neutron stars in \(f(R, T)\) theory: slow rotation approximation

DOI10.1088/1475-7516/2024/09/030zbMATH Open1548.83117MaRDI QIDQ6618115

Mehedi Kalam, Masum Murshid

Publication date: 14 October 2024

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

zbMATH Keywords

neutron star\(f(R, T)\) theoryI-Love-Q relationslow-rotation approximationtrace of energy-momentum tensor

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Cites Work

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• <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
• Stability of a Schwarzschild Singularity
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