Charged Gravastars with Conformal Motion in f(R,T) Gravity
arXiv:1911.08316 · doi:10.1007/s10509-019-3680-3
Abstract
This paper studies the effects of charge on a peculiar stellar object, recognized as gravastar, under the influence of gravity by considering the conjecture of Mazur and Mottola in general relativity. The gravastar is also known as an alternative to a black hole and is expressed by three distinct domains named as (i) the interior domain, (ii) the intermediate shell and (iii) the exterior domain. We analyze these domains for a specific gravity model conceding the conformal Killing vectors. In the interior domain, we assume that pressure is equal to negative energy density which leads to the existence of repulsive force on the spherical shell. The intermediate shell consists of ultra-relativistic plasma and pressure which shows a direct relation with energy density and counterbalances the repulsive force applied by the interior domain. The exterior vacuum spherical domain is taken to be the de Sitter spacetime illustrated by the Reissner-Nordström metric. We conclude that non-singular solutions of charged gravastar with various physical properties such as length, energy, entropy and equation of state parameter are physically consistent.
arXiv comment21 pages, 5 figures
References in corpus (29)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- f(R,T) gravity
- A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation
- Gravitational Vacuum Condensate Stars
- Stable gravastars - an alternative to black holes?
- Gravastars must have anisotropic pressures
- Stable dark energy stars
- f(R, T, R_μνT^μν) gravity phenomenology and ΛCDM universe
- How to tell a gravastar from a black hole
- Cosmological and Solar System Consequences of f(R,T) Gravity Models
- f(R,T) Cosmological Models in Phase Space
- Energy Conditions in Gravity
- Gravitational wave signatures of the absence of an event horizon. I. Nonradial oscillations of a thin-shell gravastar
- Cosmological solutions from Induced Matter Model applied to 5D f(R,T) gravity and the shrinking of the extra coordinate
- Stable gravastars with generalised exteriors
- Charged gravastars admitting conformal motion
- Quantum Phase Transitions and the Breakdown of Classical General Relativity
- RX J1856-3754: Evidence for a Stiff EOS
- Gravastars supported by nonlinear electrodynamics
- Can accretion disk properties distinguish gravastars from black holes?
- Electrically charged gravastar configurations
- Where are all the gravastars? Limits upon the gravastar model from accreting black holes
- Gravastars in Gravity
- Gravastar energy conditions revisited
- Electromagnetic Fields of Slowly Rotating Magnetized Gravastars
- Star Models with Dark Energy
- On Anisotropic Dark Energy
- Interior Solutions of Fluid Sphere in f(R,T) Gravity Admitting Conformal Killing Vectors
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- Novel Gravastar Solutions: Investigating Stability, Energy, and Entropy in the Presence of Cloud of Strings and Quintessence
- Gravastars in Gravity
- Stability of Gravastars with Exterior Regular Black Holes
- Massive Compact Bardeen Stars with Conformal Motion
- Relativistic isotropic stellar model in gravity with Durgapal- IV Metric
- Constraining study of charged gravastars solutions in symmetric teleparallel gravity
- Stable Bounded Excursion Gravastars with Regular Black Holes
- Isotropic Buchdahl's relativistic fluid sphere within gravity
- Inhomogeneous Perturbations and Stability Analysis of the Einstein Static Universe in f(R,T) Gravity
- Emergent scenario in mimetic gravity
- Impact of Charge on Gravastars in Gravity
- Charged Gravastar Solutions in the Finch-Skea Framework with f(\mathbb{Q}) Gravity
- On a Class of Exact Arbitrarily Differentiable de Sitter Cores with Kerr Exteriors: Possible gravastar or regular black hole mimickers