https://doi.org/10.1140/epjp/s13360-025-06202-6
Regular Article
Role of de Rham–Gabadadze–Tolley like massive gravity on stellar structure fluids
1
Department of Mathematics, School of Science, University of Management and Technology, 54000, Lahore, Pakistan
2
Research Center of Astrophysics and Cosmology, Khazar University, 41 Mehseti Street, AZ1096, Baku, Azerbaijan
3
Department of Mathematics, Government General Degree College Singur, 712 409, Hooghly, West Bengal, India
4
School of Science and Engineering, Khazar University, 41 Mehseti Street, AZ1096, Baku, Azerbaijan
5
Department of Mathematics, College of Sciences, King Khalid University, Abha, 61413, Saudi Arabia
6
Department of Physics, Zhejiang Normal University, 321004, Jinhua, People’s Republic of China
Received:
16
January
2025
Accepted:
6
March
2025
Published online:
10
May
2025
The main goal of this work is to investigate the dynamic properties of a spherically symmetric anisotropic compact star model. This study is carried out within the context of Tolman-Kuchowiz spacetime with substantial de Rham-Gabadadze-Tolley like massive gravity. We used the observed mass and radius estimates for the compact star model 
to evaluate the behavior of the anisotropic fluid and the stability of the compact star. The fundamental results are graphically analyzed and the other findings are comprehensively tabulated. We also discuss the mass-to-radius relationship graphically for compact star candidates 
. Through our analysis, we found that our stellar models are stable and well-behaved.
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© The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2025
Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
