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相关论文: Tolman-Bayin type static charged fluid spheres in …

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In this article, Einstein-Maxwell space-time has been considered in connection to some of the astrophysical solutions as previously obtained by Tolman (1939) and Bayin (1978). The effect of inclusion of charge into these solutions has been…

天体物理学 · 物理学 2009-06-23 Saibal Ray , Basanti Das , Farook Rahaman , Subharthi Ray

Some known solutions for static charged fluid spheres of Tolman-VI type in general relativity are reexamined. The gravitational mass that appears in the Pant and Sah \cite{pan79} and Tikekar \cite{tik84} solutions is shown to be of…

天体物理学 · 物理学 2008-11-26 Saibal Ray , Basanti Das

A new class of exact solutions of the Einstein-Maxwell system is found in closed form. This is achieved by choosing a generalised form for one of the gravitational potentials and a particular form for the electric field intensity. For…

广义相对论与量子宇宙学 · 物理学 2009-11-13 S. Thirukkanesh , S. D. Maharaj

Static spherically symmetric anisotropic source has been studied for the Einstein-Maxwell field equations assuming the erstwhile cosmological constant $ \Lambda $ to be a space-variable scalar, viz., $ \Lambda = \Lambda(r) $. Two cases have…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Saibal Ray , Sumana Bhadra , Anand S. Sengupta

Within the framework of General Relativity a model approach to a description of spherical gravitating static fluid balls with an electric charge is considered. The metric interval is written in Bondi's radiation coordinates. The total…

广义相对论与量子宇宙学 · 物理学 2012-01-24 Alexandre M. Baranov , Zakhar V. Vlasov

This paper aims to explore a class of static stellar equilibrium configuration of relativistic charged spheres made of a charged perfect fluid. Solving the Einstein-Maxwell field equations, we consider a particularized metric potential,…

广义相对论与量子宇宙学 · 物理学 2021-05-11 J. Kumar , S. K. Maurya , A. K. Prasad , Ayan Banerjee

A new class of solutions to the coupled, spherically symmetric Einstein-Maxwell equations for a compact material source is constructed. Some of these solutions can be made to satisfy a number of requirements for being physically relevant,…

广义相对论与量子宇宙学 · 物理学 2009-10-20 J. Burke , D. Hobill

Under the static spherically symmetric Einstein-Maxwell spacetime of embedding class one we explore possibility of electromagnetic mass model where mass and other physical parameters have purely electromagnetic origin (Tiwari 1984, Gautreau…

广义相对论与量子宇宙学 · 物理学 2016-10-19 S. K. Maurya , Y. K. Gupta , Saibal Ray , Vikram Chatterjee

We consider the static and spherically symmetric field equations of general relativity for charged perfect fluid spheres in the presence of a cosmological constant. Following work by Florides (1983) we find new exact solutions of the field…

广义相对论与量子宇宙学 · 物理学 2011-10-19 Christian G. Boehmer , Atifah Mussa

We study boson stars in a theory of complex scalar field coupled to Einstein gravity with the potential: $V(|\Phi|) := m^{2} |\Phi|^2 +2 \lambda |\Phi|$ (where $m^2$ and $\lambda$ are positive constant parameters). This could be considered…

高能物理 - 理论 · 物理学 2016-05-24 Sanjeev Kumar , Usha Kulshreshtha , Daya Shankar Kulshreshtha

In this paper we study the isotropic cases of static charged fluid spheres in general relativity. For this purpose we consider two different specialization and under these we solve the Einstein-Maxwell field equations in isotropic…

广义相对论与量子宇宙学 · 物理学 2011-08-25 Basanti Das , Pratap Chandra Ray , Irina Radinschi , Farook Rahaman , Saibal Ray

A class of exact solutions for the Einstein-Maxwell field equations are obtained by assuming the erstwhile cosmological constant $ \Lambda $ to be a space-variable scalar, viz., $ \Lambda =\Lambda(r) $. The source considered here is static,…

广义相对论与量子宇宙学 · 物理学 2011-03-04 R. N. Tiwari , Saibal Ray , Sumana Bhadra

We establish the existence of a family of static, spherically symmetric spacetimes that are solutions of the Einstein Field Equations of General Relativity coupled to the electric field of a static point charge obeying the equations of…

广义相对论与量子宇宙学 · 物理学 2025-08-11 Erik Amorim

We present new results concerning the existence of static, electrically charged, perfect fluid spheres that have a regular interior and are arbitrarily close to a maximally charged black-hole state. These configurations are described by…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Fernando de Felice , Liu Siming , Yu Yunqiang

We present new exact solutions for the Einstein-Maxwell system in static spherically symmetric interior spacetimes. For a particular form of the gravitational potentials and the electric field intensity, it is possible to integrate the…

广义相对论与量子宇宙学 · 物理学 2009-10-16 S. D. Maharaj , S. Thirukkanesh

In this work some families of relativistic anisotropic charged fluid spheres have been obtained by solving Einstein-Maxwell field equations with preferred form of one of the metric potentials, a suitable forms of electric charge…

广义相对论与量子宇宙学 · 物理学 2014-09-02 Mohammad Hassan Murad , Saba Fatema

In this article, we provide a pedagogical review of the Tolman-Oppenheimer-Volkoff (TOV) equation and its solutions which describe static, spherically symmetric gaseous stars in general relativity. Our discussion starts with a systematic…

广义相对论与量子宇宙学 · 物理学 2021-06-15 Emmanuel Chavez Nambo , Olivier Sarbach

Approximate solutions representing the gravitational-electrostatic balance of two arbitrary point sources in general relativity have led to contradictory arguments in the literature with respect to the condition of balance. Up to the…

广义相对论与量子宇宙学 · 物理学 2011-07-19 G. P. Perry , F. I. Cooperstock

Static, spherically symmetric solutions representing stars made of barotropic perfect fluid are studied in the context of two theories of type-II minimally modified gravity, VCDM and VCCDM. Both of these theories share the property that no…

广义相对论与量子宇宙学 · 物理学 2022-05-25 Antonio De Felice , Shinji Mukohyama , Masroor C. Pookkillath

We study boson shells and boson stars in a theory of complex scalar field coupled to the $U(1)$ gauge field $A_{\mu}$ and Einstein gravity with the potential: $V(|\Phi|) := \frac{1}{2} m^{2} \left(|\Phi|+ a \right)^2$. This could be…

高能物理 - 理论 · 物理学 2016-06-08 Sanjeev Kumar , Usha Kulshreshtha , Daya Shankar Kulshreshtha
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