Spherical symmetric perfect fluid collapse in \(f(R,T)\) gravity
From MaRDI portal
Publication:292962
DOI10.1007/s10773-015-2839-0zbMath1338.83137OpenAlexW2223342661MaRDI QIDQ292962
Publication date: 9 June 2016
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-015-2839-0
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (3)
Higher-dimensional gravitational collapse of perfect fluid spherically symmetric spacetime in f(R, T) gravity ⋮ Effects of electromagnetic field on gravitational collapse in \(f(R, T)\) gravity ⋮ Charged perfect fluid gravitational collapse in f(R, T) gravity
Cites Work
- Non-vacuum solutions of Bianchi type \(VI _{0}\) universe in \(f(R)\) gravity
- \(f(R)\) theories
- Gravitational collapse in generalized Vaidya space-time for Lovelock gravity theory
- Expanding and collapsing scalar field thin shell
- Gravitational dust collapse in \(f(R)\) gravity
- Gravitational collapse in higher dimensional Husain space-time
- Gravitational charged perfect fluid collapse in friedmann universe models
- \(1/R\) gravity and scalar-tensor gravity
- Where new gravitational physics comes from: M-theory?
- Quasi-spherical gravitational collapse in any dimension
- The force of gravity from a Lagrangian containing inverse powers of the Ricci scalar
- Quasi-spherical solution with heat flux and non-adiabatic collapse of radiating star
- Nature of singularity formed by the gravitational collapse in Husain space-time with electromagnetic field and scalar field
- Spatially homogeneous rotating solution in \(f(R)\) gravity and its energy contents
- Gravitational perfect fluid collapse in \(f(R)\) gravity
- LRS Bianchi type-I cosmological model in \(f(R,T)\) theory of gravity
- Locally rotationally symmetric vacuum solutions in \(f(R)\) gravity
- Presence of dark energy and dark matter: does cosmic acceleration signifies a weak gravitational collapse?
- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
- EFFECTS OF ELECTROMAGNETIC FIELD ON GRAVITATIONAL COLLAPSE
- Spherically symmetric solutions in f ( R ) gravity via the Noether symmetry approach
- PLANE SYMMETRIC SOLUTIONS IN f(R) GRAVITY
- PLANE SYMMETRIC GRAVITATIONAL COLLAPSE
- Consistent modified gravity: dark energy, acceleration and the absence of cosmic doomsday
- RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES
- AdS and stabilized extra dimensions in multi-dimensional gravitational models with nonlinear scalar curvature terms R −1 and R 4
- NAKED SINGULARITIES IN HIGHER DIMENSIONAL GRAVITATIONAL COLLAPSE
- On Continued Gravitational Contraction
This page was built for publication: Spherical symmetric perfect fluid collapse in \(f(R,T)\) gravity
