Modified gravity in the interior of population II stars

DOI10.1088/1475-7516/2021/05/040zbMath1485.85004arXiv2008.12264OpenAlexW3080651605MaRDI QIDQ5028134

Shaswata Chowdhury, Tapobrata Sarkar

Publication date: 8 February 2022

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

Full work available at URL: https://arxiv.org/abs/2008.12264

zbMATH Keywords

gravitymodified gravity

Mathematics Subject Classification ID

Chemically reacting flows (80A32) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Galactic and stellar structure (85A15)

Related Items (2)

White dwarf stars in modified gravity ⋮ Non-homogeneous exoplanets in metric-affine gravity

Cites Work

• Stellar structure models in modified theories of gravity: lessons and challenges
• Cosmological tests of gravity
• Tests of chameleon gravity
• An introduction to the Vainshtein mechanism
• Stellar Structure and Evolution
• Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
• Relativistic stars in beyond Horndeski theories
• Testing the Vainshtein mechanism using stars and galaxies
• Models for Red Giant Stars. I.
• Dark energy in Horndeski theories after GW170817: A review
• Dark energy and modified gravity in degenerate higher-order scalar–tensor (DHOST) theories: A review

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