Impact of equation of state on fluid spheres in Finselarian gravity

IF 5 2区物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS

Physics of the Dark Universe Pub Date : 2025-02-26 DOI:10.1016/j.dark.2025.101873

Allah Ditta , Rubab Manzoor , Faisal Javed , Muhammad Aslam , Muhammad Yousaf Malik , Guzalxon Belalova

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引用次数: 0

Abstract

The motivation behind this article is studying the configurations of compact bodies under the effects of Finselarian gravity in spherical symmetric spacetime coordinates. To examine the effects of gravity on compact stellar configurations, we use the Tolman–Kuchowicz components for spherical symmetric spacetime. We use the linear equation of state to find the function

u_{0}^{^{'}} (r)

involved in Finselsian gravity. We analyze the configurations using the data for the mass and radius for compact candidates

H e r X - 1, S M C X - 1, L M C X - 4, C e n X - 3

. All the star structures that are considered here are stable and ideally free of a central singularity. A detailed graphical investigation reveals that several physical properties, such as density, pressures, sound speeds, TOV forces, mass function, and compactification implemented in celestial formations are critical to their formation. Moreover, we conclude that our stellar models behave well and are acceptable.

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状态方程对芬塞尔引力中流体球体的影响

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来源期刊

Physics of the Dark Universe ASTRONOMY & ASTROPHYSICS-

CiteScore

9.60

自引率

7.30%

发文量

118

审稿时长

61 days

期刊介绍： Physics of the Dark Universe is an innovative online-only journal that offers rapid publication of peer-reviewed, original research articles considered of high scientific impact. The journal is focused on the understanding of Dark Matter, Dark Energy, Early Universe, gravitational waves and neutrinos, covering all theoretical, experimental and phenomenological aspects.