Compact star in general F(R) gravity: Inevitable degeneracy problem and non-integer power correction-Reference-Cited by-同舟云学术

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Compact star in general F(R) gravity: Inevitable degeneracy problem and non-integer power correction

Published:2022-03 Issue: Volume:826 Page:136929
ISSN:0370-2693
Container-title:Physics Letters B
language:en
Short-container-title:Physics Letters B

Author:

Numajiri Kota^ORCID,Katsuragawa Taishi,Nojiri Shin'ichi^ORCID

Funder

Central China Normal University

Japan Society for the Promotion of Science

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics

Reference43 articles.

1. Shapiro delay measurement of a two solar mass neutron star;Demorest;Nature,2010

2. A massive pulsar in a compact relativistic binary;Antoniadis;Science,2013

3. Evidence for quark-matter cores in massive neutron stars;Annala;Nat. Phys.,2020

4. Introduction to modified gravity and gravitational alternative for dark energy;Nojiri;Int. J. Geom. Methods Mod. Phys.,2007

5. Beyond Einstein Gravity;Faraoni,2011

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1. Moment of inertia and compactness of quark stars within the context of f(R, T, L _m) gravity;Physica Scripta;2024-07-02

2. Phenomenology of axionic static neutron stars with masses in the mass-gap region;Classical and Quantum Gravity;2024-03-27

3. Magnetic string matter collapse in rainbow gravity;Canadian Journal of Physics;2024-01-01

4. Anisotropic quark stars in energy-momentum squared gravity;Journal of High Energy Astrophysics;2023-11

5. Modeling Wormholes Generated by Dark Matter Galactic Halos in f(R)$f(R)$ Modified Gravity;Annalen der Physik;2023-06-27

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