Anisotropic star by gravitational decoupling: A vanishing complexity approach

被引:11
作者
Smitha, T. T. [1 ]
Maurya, S. K. [1 ]
Dayanandan, B. [1 ]
Mustafa, G. [2 ]
机构
[1] Univ Nizwa, Coll Arts & Sci, Dept Math & Phys Sci, Nizwa, Oman
[2] Zhejiang Normal Univ, Dept Phys, Jinhua 321004, Peoples R China
关键词
Exact solutions; Compact objects; Gravitational decoupling; Complexity; MINIMAL GEOMETRIC DEFORMATION; TOLMAN VII SOLUTION; DYNAMICAL INSTABILITY; SCHWARZSCHILD LIMIT; INTERIOR SOLUTION; CRACKING;
D O I
10.1016/j.rinp.2023.106502
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
A new static spherically symmetric interior solution has been derived using Gravitational Decoupling via Complete Geometric Deformation, satisfying the vanishing complexity which explores the fundamental physical acceptability of the stellar model. In the current analysis, we present a systematic approach proposed by L. Herrera [Phys Rev D 97: 044010, 2018] and Contreras-Stuchlik [Eur Phys J C 82: 706, 2022] to derive a complexity-free solution. We plotted the graphical behavior of the energy density, radial pressure, tangential pressure, equation of state parameters, anisotropy, and stability analysis, respectively to check the physical viability of the complexity-free solution. In addition, we also discuss the energy exchange between the relativistic fluids which shows that the decoupling constant controls the direction of the energy exchange.
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页数:11
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