scholarly journals ENERGY OF SPHERICALLY SYMMETRIC SPACE–TIMES ON REGULARIZING TELEPARALLELISM

2010 ◽  
Vol 25 (14) ◽  
pp. 2883-2895 ◽  
Author(s):  
GAMAL G. L. NASHED
Keyword(s):  
General Relativity ◽  
Symmetric Space ◽  
Total Energy ◽  
Gravitational Energy ◽  
Spherically Symmetric ◽  
Tetrad Formulation ◽  
Spherically Symmetric Solutions

We calculate the total energy of an exact spherically symmetric solutions, i.e. Schwarzschild and Reissner–Nordström, using the gravitational energy–momentum 3-form within the tetrad formulation of general relativity. We explain how the effect of the inertial makes the total energy unphysical. Therefore, we use the covariant teleparallel approach which makes the energy always physical one. We also show that the inertial has no effect on the calculation of momentum.

Spherically symmetric solutions with heat flow in general relativity

Pramana ◽  
1990 ◽  
Vol 34 (5) ◽  
pp. 397-401 ◽  
Author(s):  
A Banerjee ◽  
S B Dutta Choudhury ◽  
B K Bhui
Keyword(s):  
General Relativity ◽  
Heat Flow ◽  
Spherically Symmetric ◽  
Spherically Symmetric Solutions

Stable wormhole models in general relativity under conformal symmetry

2021 ◽  
Vol 18 (03) ◽  
pp. 2150041
Author(s):  
Asifa Ashraf ◽  
Zhiyue Zhang
Keyword(s):  
General Relativity ◽  
Symmetric Space ◽  
Conformal Symmetry ◽  
Energy Condition ◽  
Null Energy Condition ◽  
Anisotropic Fluid ◽  
Spherically Symmetric ◽  
Shape Functions ◽  
The Stability ◽  
Tov Equation

In this study, we shall explore conformal symmetry to examine the wormhole models by considering traceless fluid. In this regard, we shall take anisotropic fluid with spherically symmetric space-time. Further, we shall calculate the properties of shape-functions, which are necessary for the existence of wormhole geometry. The presence of exotic matter is confirmed in all the cases through the violation of the Null Energy Condition. Furthermore, we have discussed the stability of wormhole solutions through the Tolman–Oppenheimer–Volkoff (TOV) equation. It is observed that our acquired solutions are stable under the particular values of involved parameters in different cases in conformal symmetry.

scholarly journals Classic tests of General Relativity described by brane-based spherically symmetric solutions

2014 ◽  
Vol 74 (8) ◽  
Author(s):  
R. R. Cuzinatto ◽  
P. J. Pompeia ◽  
M. de Montigny ◽  
F. C. Khanna ◽  
J. M. Hoff da Silva
Keyword(s):  
General Relativity ◽  
Spherically Symmetric ◽  
Tests Of General Relativity ◽  
Spherically Symmetric Solutions

A REVIEW ON THE GEOMETRIC FORMULATION OF TOLMAN–BONDI EQUATIONS IN GENERAL RELATIVITY

2009 ◽  
Vol 06 (04) ◽  
pp. 595-617 ◽  
Author(s):  
IVANA BOCHICCHIO ◽  
MAURO FRANCAVIGLIA ◽  
ETTORE LASERRA
Keyword(s):  
General Relativity ◽  
Symmetric Space ◽  
Exact Solutions ◽  
Structural Properties ◽  
Spherically Symmetric ◽  
Principal Curvatures ◽  
Spherical Shells ◽  
Geometric Formulation ◽  
Dust Universe

This work is focused on spherically symmetric space-times. More precisely, geometric and structural properties of spatially spherical shells of a dust universe are analyzed in detail considering recent results of our research. Moreover, exact solutions, obtained for constant Ricci principal curvatures, are inferred and qualitatively analyzed through suitable classic analogies.

scholarly journals Nonstatic Spherically Symmetric Solutions for a Perfect Fluid in General Relativity

1976 ◽  
Vol 29 (2) ◽  
pp. 113 ◽  
Author(s):  
N Chakravarty ◽  
SB Dutta Choudhury ◽  
A Banerjee
Keyword(s):  
General Relativity ◽  
Exact Solutions ◽  
Perfect Fluid ◽  
Dynamical Behaviour ◽  
Symmetric Distribution ◽  
Spherically Symmetric ◽  
Field Equations ◽  
Spherically Symmetric Solutions ◽  
Spherically Symmetric Distribution ◽  
General Method

A general method is described by which exact solutions of Einstein's field equations are obtained for a nonstatic spherically symmetric distribution of a perfect fluid. In addition to the previously known solutions which are systematically derived, a new set of exact solutions is found, and the dynamical behaviour of the corresponding models is briefly discussed.

scholarly journals New Black Holes Solutions in a Modified Gravity

2011 ◽  
Vol 2011 ◽  
pp. 1-7 ◽  
Author(s):  
M. Hamani Daouda ◽  
Manuel E. Rodrigues ◽  
M. J. S. Houndjo
Keyword(s):  
Black Holes ◽  
General Relativity ◽  
Modified Gravity ◽  
Gauge Theories ◽  
Matter Content ◽  
Spherically Symmetric ◽  
Commutator Algebra ◽  
Spherically Symmetric Solutions ◽  
Basic Concepts ◽  
Rindler Acceleration

We present some basic concepts of a theory of modified gravity, inspired by the gauge theories, where the commutator algebra of covariant derivative gives us an added term with respect to the General Relativity, which represents the interaction of gravity with a substratum. New spherically symmetric solutions of this theory are obtained and can be viewed as solutions that reproduce the mass, the charge, the cosmological constant, and the Rindler acceleration, without coupling with the matter content, that is, in the vacuum.

scholarly journals Static spherically symmetric solutions in a subclass of Horndeski theories of gravity

2018 ◽  
Vol 15 (09) ◽  
pp. 1850152 ◽  
Author(s):  
Lorenzo Sebastiani
Keyword(s):  
General Relativity ◽  
Black Hole ◽  
Integration Constant ◽  
Spherically Symmetric ◽  
Rotation Curves ◽  
Spherically Symmetric Solutions ◽  
Euclidean Action ◽  
Theories Of Gravity ◽  
Static Spherically Symmetric Solutions

In this paper, we will consider a subclass of models of Horndeski theories of gravity and we will check for several Static Spherically Symmetric solutions. We will find a model which admits an exact black hole (BH) solution and we will study its thermodynamics by using the Euclidean Action. We will see that, in analogy with the case of General Relativity (GR), the integration constant of the solution can be identified with the mass of the BH itself. Other solutions will be discussed, by posing special attention on the possibility of reproducing the observed profiles of the rotation curves of galaxies. a

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