A comprehensive study of massive compact star admitting conformal motion under Bardeen geometry
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Publication:6536662
DOI10.1016/J.NUCLPHYSB.2024.116523MaRDI QIDQ6536662
Pradyumn Sahoo, [[Person:6196419|Author name not available (Why is that?)]]
Publication date: 13 May 2024
Published in: Nuclear Physics B (Search for Journal in Brave)
Cites Work
- Modified Gauss-Bonnet theory as gravitational alternative for dark energy
- Massive compact Bardeen stars with conformal motion
- Sharp bounds on the critical stability radius for relativistic charged spheres
- On the stability of a class of modified gravitational models
- Magnetized quark and strange quark matter in the spherical symmetric space-time admitting conformal motion
- Relativistic model for anisotropic strange stars
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
- Spherically symmetric spacetimes admitting inheriting conformal Killing vector fields
- General Relativistic Fluid Spheres
- Isotropic and anisotropic charged spheres admitting a one-parameter group of conformal motions
- Relativistic charged spheres: II. Regularity and stability
- QUARK STARS ADMITTING A ONE-PARAMETER GROUP OF CONFORMAL MOTIONS
- Relativistic Krori‐Barua Compact Stars in f(R,T)$f(R,T)$ Gravity
- Bardeen compact stars in modified \(f(R)\) gravity
- Compact Bardeen Stars in f(R,T)$f(\mathcal {R}, T)$ Theory with Conformal Motion
- A study of charged stellar structure in modified \(f(R, \phi, \chi)\) gravity
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