Weak-field limit of \(f(R)\) gravity to unify peculiar white dwarfs

DOI10.1016/J.PHYSLETB.2022.136942zbMath1487.85022arXiv2201.12210OpenAlexW4210419144MaRDI QIDQ2119611

Surajit Kalita, Lupamudra Sarmah

Publication date: 29 March 2022

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2201.12210

zbMATH Keywords

modified gravitywhite dwarfsChandrasekhar limit

Mathematics Subject Classification ID

Poisson manifolds; Poisson groupoids and algebroids (53D17) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (1)

Tideless traversable wormholes surrounded by cloud of strings in f(R) gravity

Cites Work

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• \(f(R)\) theories
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• Rapidly rotating general relativistic stars - I. Numerical method and its application to uniformly rotating polytropes
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• Significantly super-Chandrasekhar mass-limit of white dwarfs in noncommutative geometry
• Constraints on modified gravity models from white dwarfs
• Modified Einstein's gravity to probe the sub- and super-Chandrasekhar limiting mass white dwarfs: a new perspective to unify under- and over-luminous type Ia supernovae
• Super-Chandrasekhar limiting mass white dwarfs as emergent phenomena of noncommutative squashed fuzzy spheres
• Introduction to General Relativity
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• SOLAR SYSTEM TESTS OF f(R) GRAVITY
• The cosmological constant problem

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