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相关论文: The Chaplygin dark star

200 篇论文

This manuscript investigate the dark energy Bianchi type-I cosmological models in presence of generalized Chaplygin gas, variable gravitational and cosmological constants. In this manuscript, exact solutions of Einstein field equations are…

广义相对论与量子宇宙学 · 物理学 2022-02-11 N. Hulke , G. P. Singh , Binaya K Bishi

In this work, gravitational collapse of a spherical cloud, consists of both dark matter and dark energy in the form of modified Chaplygin gas is studied. It is found that dark energy alone in the form of modified Chaplygin gas forms black…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Ujjal Debnath , Subenoy Chakraborty

We review the theoretical framework underlying models of asymmetric dark matter, describe astrophysical constraints which arise from observations of neutron stars, and discuss the prospects for detecting asymmetric dark matter.

高能物理 - 唯象学 · 物理学 2015-06-16 Jason Kumar

The generalized Chaplygin gas model is characterized by the equation of state $p = - \frac{A}{\rho^\alpha}$. It is generally stated that the case $\alpha = 0$ is equivalent to a model with cosmological constant and dust ($\Lambda CDM$). In…

天体物理学 · 物理学 2009-11-10 J. C. Fabris , S. V. B. Gonçalves , R. de Sá Ribeiro

Unified dark matter cosmologies economically combine missing matter and energy in a single fluid. Of these models, the standard Chaplygin gas is theoretically motivated, but faces problems in explaining large scale structure if linear…

宇宙学与河外天体物理 · 物理学 2022-10-12 Abdelrahman Abdullah , Amr El-Zant , Ali Ellithi

The cosmological model of the modified Chaplygin gas interacting with cold dark matter is studied. Our attention is focused on the final state of universe in the model. It turns out that there exists a stable scaling solution, which…

广义相对论与量子宇宙学 · 物理学 2009-12-04 Song Li , Yongge Ma , Yun Chen

The expansion of the Universe is accelerating, as testified by observations of supernovae of type Ia as a function of redshift. Explanations are of two types: modifications of Einstein gravity or new forms of energy, coined dark energy.The…

天体物理学 · 物理学 2007-05-23 Matts Roos

As a potential candidate for the late-time accelerating expansion of the Universe, the Chaplygin gas and its generalized models have significant implications to modern cosmology. In this work we investigate the effects of dark energy on the…

高能天体物理现象 · 物理学 2024-01-22 Juan M. Z. Pretel , Mariana Dutra , Sergio B. Duarte

In this paper, we study the existence of strange star in the background of f (T) modified gravity where T is a scalar torsion. In KB metric space, we derive the equations of motion using anisotropic property within the spherically strange…

广义相对论与量子宇宙学 · 物理学 2018-10-25 Pameli Saha , Ujjal Debnath

The properties of a spherically symmetric static space-time permeated of dark energy are worked out. Dark energy is viewed as the strain energy of an elastically deformable four dimensional manifold. The metric is worked out in the vacuum…

广义相对论与量子宇宙学 · 物理学 2015-06-04 N. Radicella , M. Sereno , A. Tartaglia

We show that the observed rotation curves of spiral galaxies constrain the sound speed of the dark matter to be $c_s < 10^{-4} c$, where $c$ is the speed of light in vacuum. Using the Modified Chaplygin Gas as a representative example of a…

宇宙学与河外天体物理 · 物理学 2015-05-06 P. P. Avelino , V. M. C. Ferreira

We consider the general case of an accelerating, expanding and shearing model of a radiating relativistic star using Lie symmetries. We obtain the Lie symmetry generators that leave the equation for the junction condition invariant, and…

广义相对论与量子宇宙学 · 物理学 2015-06-23 G. Z. Abebe , S. D. Maharaj , K. S. Govinder

We model the cosmic medium as the mixture of a generalized Chaplygin gas and a pressureless matter component. Within a neo-Newtonian approach we compute the matter power spectrum. The 2dFGRS data are used to discriminate between unified…

天体物理学 · 物理学 2015-05-13 J. C. Fabris , S. V. B. Goncalves , H. E. S. Velten , W. Zimdahl

Unified cosmological models have received a lot of attention in astrophysics community for explaining both the dark matter and dark energy evolution. The Chaplygin cosmologies, a well known name in this group have been investigated matched…

广义相对论与量子宇宙学 · 物理学 2019-10-09 Weiqiang Yang , Supriya Pan , Andronikos Paliathanasis , Subir Ghosh , Yabo Wu

The postulation of Dark energy and Dark matter on the basis of observational results does not end the mystery of their existence. Theoretically new insights into dark matter have been achieved analyzing recent experimental data from the…

综合物理 · 物理学 2010-07-21 Julie Saikia , Balendra Kr. Dev Choudhury

In present paper a spherically symmetric stellar configuration has been analyzed by assuming the matter distribution of the stellar configuration is anisotropic in nature and compared with the realistic objects, namely, the low mass X-ray…

广义相对论与量子宇宙学 · 物理学 2021-08-26 Piyali Bhar , Tuhina Manna , Farook Rahaman , Ayan Banerjee

In this work we investigate the background dynamics when dark energy is coupled to dark matter with a suitable interaction in the universe described by Einstein-Aether gravity. Dark energy in the form of Modified Chaplygin gas is…

综合物理 · 物理学 2014-08-21 Chayan Ranjit , Prabir Rudra , Sujata Kundu

The generalized Chaplygin gas cosmology provides a prime example for the class of unified dark matter models, which substitute the two dark components of the standard cosmological LCDM concordance model by a single dark component. The…

宇宙学与河外天体物理 · 物理学 2017-11-28 Ralf Aurich , Sven Lustig

We investigate exotic stars composed of dark energy within the context of Einstein's General Relativity, by applying an extended Chaplygin gas equation-of-state. To account for anisotropies, we utilize a formalism based on the complexity…

广义相对论与量子宇宙学 · 物理学 2023-02-23 Á. Rincón , G. Panotopoulos , I. Lopes

We studied the Euler--Poisson equation system in the case of cylindrical symmetry with the von Neumann--Sedov--Taylor type of self-similar Ansatz and present scaling solutions. We have analyzed the scenario governed by Chaplygin's equation…

数学物理 · 物理学 2025-03-26 Balázs Endre Szigeti , Imre Ferenc Barna , Gergely Gábor Barnaföldi