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[PDF] Top 20 Spherical Anisotropic Fluid Distribution in General Relativity

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Spherical Anisotropic Fluid Distribution  in General Relativity

Spherical Anisotropic Fluid Distribution in General Relativity

... new general solution of Einstein Field Equations and its detailed study, in order to construct a realistic model of compact ...density, anisotropic pressures( radial and transverse pressures), anisotropy ... See full document

18

A New Charged Anisotropic Compact Star Model in General Relativity

A New Charged Anisotropic Compact Star Model in General Relativity

... We have shown the variation of metric potentials with radial coordinate for the star PSR J0348 + 0432 in Figure 1. It is clear from figure that metric poten- tials are regular and free form any singularity inside the ... See full document

17

Class of Charged Fluid Balls in General Relativity

Class of Charged Fluid Balls in General Relativity

... In the present study, we have obtained a new analytical solution of combined Eins- tein-Maxwell field equations describing the interior field of a ball having static spherically symmetric isotropic charged fluid ... See full document

18

Topics in general relativity

Topics in general relativity

... We first assume our mirrors and arm cavities to be infinite, and construct modes of infinite-mirror arm cavities using two identical (but non-spherical) mirrors facing each other. Because the cavities are ... See full document

120

Bianchi type v magnetized cosmological model with wet dark fluid in general relativity

Bianchi type v magnetized cosmological model with wet dark fluid in general relativity

... gravitation which has been very successful in describing gravitational phenomenon and also served as a basis for model of the universe. The homogenous isotropic expanding -scale properties of the universe. Bianchi type ... See full document

5

Anisotropic Fluid Star Model in Isotropic Coordinates

Anisotropic Fluid Star Model in Isotropic Coordinates

... the general relativistic field equations in isotropic coordinates for anisotropic neutral fluid, compatible with a super dense star modeling by considering a specific choice of anisotropy factor ∆ ... See full document

5

To the Schwarzschild Solution in General Relativity

To the Schwarzschild Solution in General Relativity

... As follows from the foregoing analysis, the Schwarzschild solution after some minor correction and reconstruction coincides with the traditional [3] interpre- tation of this solution. Both solutions do not satisfy the ... See full document

13

Spatially homogeneous anisotropic Bianchi Type I inflationary universe for barotropic fluid distribution with variable bulk viscosity

Spatially homogeneous anisotropic Bianchi Type I inflationary universe for barotropic fluid distribution with variable bulk viscosity

... = 0 is taken into account. We find that bulk viscosity prevents the matter density to vanish. The model in general represents anisotropic universe but at late time, it isotropizes. The spatial volume ... See full document

13

Anisotropic Geodesic Fluid in Non Comoving Spherical Coordinates

Anisotropic Geodesic Fluid in Non Comoving Spherical Coordinates

... (39) which holds also in the general relativistic case (see [14]). Keeping in mind that in our model φ is sourced not only by stellar matter but also by the so called dark sector contributions, we may use a ... See full document

8

A Spherical Relativistic Anisotropic Compact Star Model

A Spherical Relativistic Anisotropic Compact Star Model

... of anisotropic solution of Einstein’s relativistic field equation attracts the researchers to do work in this ...of fluid distribution by assuming constant matter energy ... See full document

22

Spherical Gravitational Collapse of  Anisotropic Radiating Fluid Sphere

Spherical Gravitational Collapse of Anisotropic Radiating Fluid Sphere

... Herrera and Santos [8] and Mitra [9] established the fact that gravitational collapse is a high energy dissipating process which plays a dominant role in the formation and evolution of stars. Historically the dissi- ... See full document

11

Tests of general relativity with GW150914

Tests of general relativity with GW150914

... in general relativ- ...parameterized general-relativity violations during the inspiral and merger phases, we perform quantitative tests on the gravitational-wave phase in the dynamical regime and we ... See full document

17

Tests of General Relativity with GW170817

Tests of General Relativity with GW170817

... the general-relativistic dynamics of the ...numerical relativity [32 – ...numerical relativity waveforms to describe the intermediate regime between inspiral ... See full document

15

General Relativity by Kawaguchi geometry

General Relativity by Kawaguchi geometry

... To find the solution of Euler-Lagrange equations is equivalent to find the extremal of the action, which is a submanifold that corresponds to our spacetime embedded into a greater space together with other dynamical ... See full document

6

Tests of General Relativity with GW170817

Tests of General Relativity with GW170817

... The recent discovery by Advanced LIGO and Advanced Virgo of a gravitational wave signal from a binary neutron star inspiral has enabled tests of general relativity (GR) with this new type of source. This ... See full document

14

The Definition of Density in General Relativity

The Definition of Density in General Relativity

... According to general relativity the geometry of space depends on the distribu- tion of matter or energy fields. The relation between the local geometrical pa- rameters and the volume enclosed in given ... See full document

10

Astronomical tests of general relativity

Astronomical tests of general relativity

... of General Relativity by Albert Einstein in 1916, experimental confirmation rested on three astronomical ...with General Relativity to the ... See full document

120

Decelerating Non Static Plane Symmetric cosmological Model with Varying

Decelerating Non Static Plane Symmetric cosmological Model with Varying

... [20] J.D. Barrow: Month.Notices of the Royal Astrono.Soc.211(2),1984, 221-227. [21] G.F. Ellis, M.A. MacCallum: Commu. in Math.Phys. 12(2), 1969, 108-141. [22] K.A. Dunn, B.O.J. Tupper: The Astrophysical Journal, 204, ... See full document

5

ch16 Special & General Relativity

ch16 Special & General Relativity

... Since the early 1800s astronomers measured a precession of Mercury’s orbit—about 574 seconds of arc per century. Perturbations by the other planets were found to account for the precession—except for 43 seconds of arc ... See full document

55

Tests of General Relativity with GW150914

Tests of General Relativity with GW150914

... posterior distribution of one parameter to be off centered with respect to zero, we expect that the posteriors of all of the other parameters will also be off ... See full document

20

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