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相关论文: Kerr-de Sitter Black Hole Revisited

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The Event Horizon Telescope collaboration has revealed the first direct image of a black hole, as per the shadow of a Kerr black hole of general relativity. However, other Kerr-like rotating black holes of modified gravity theories cannot…

广义相对论与量子宇宙学 · 物理学 2022-01-21 Misba Afrin , Sushant G. Ghosh

To explore the influence of the cosmological constant on black hole images, we have developed a comprehensive analytical method for simulating images of Kerr-de Sitter black holes illuminated by equatorial thin accretion disks. Through the…

广义相对论与量子宇宙学 · 物理学 2024-05-01 Ke Wang , Chao-Jun Feng , Towe Wang

In the de Sitter-invariant approach to gravitation, all solutions to the gravitational field equations are spacetimes that reduce locally to de Sitter. Consequently, besides including an event horizon, the de Sitter-invariant black hole…

广义相对论与量子宇宙学 · 物理学 2025-09-10 D. F. López , S. Abarghouei Nejad , José G. Pereira

A four-dimensional black hole solution of the Einstein equations with a positive cosmological constant, coupled to a conformal scalar field, is given. There is a curvature singularity at the origin, and scalar field diverges inside the…

高能物理 - 理论 · 物理学 2009-11-07 Cristian Martinez , Ricardo Troncoso , Jorge Zanelli

It is now widely accepted that the universe as we understand it is accelerating in expansion and fits the de Sitter model rather well. As such, a realistic assumption of black holes must place them on a de Sitter background and not…

广义相对论与量子宇宙学 · 物理学 2011-04-04 Sarp Akcay , Richard Matzner

We present solutions of DHOST theories describing a rotating black hole embedded in an expanding universe. The solution is constructed by conformal transformation of a stealth Kerr(-de Sitter) black hole. The conformal factor depends…

广义相对论与量子宇宙学 · 物理学 2023-05-29 Eugeny Babichev , Christos Charmousis , Nicolas Lecoeur

In this paper, we prove a series of results concerning the uniqueness of Kerr-de Sitter as a family of smooth stationary black hole solutions to the nonlinear Einstein vacuum equations with positive cosmological constant $\Lambda$. The…

广义相对论与量子宇宙学 · 物理学 2025-09-09 Allen Juntao Fang

Using perturbative techniques, we investigate the existence and properties of a new static solution for the Einstein equation with a negative cosmological constant, which we call the deformed black hole. We derive a solution for a static…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Hirotaka Yoshino , Tohru Ohba , Akira Tomimatsu

We propose possible properties of quantum gravity in de Sitter space, and find that they relate the value of the cosmological constant to parameters of the Standard Model. In de Sitter space we suggest (i) that the most sharply defined…

高能物理 - 理论 · 物理学 2023-06-07 Mark P. Hertzberg , Abraham Loeb

We study the thermodynamic properties associated with the black hole event horizon and the cosmological horizon for black hole solutions in asymptotically de Sitter spacetimes. We examine thermodynamics of these horizons on the basis of the…

高能物理 - 理论 · 物理学 2007-05-23 Yuichi Sekiwa

In this paper we present a regular black hole with a positive cosmological constant. The regular black hole considered is the well known Bardeen black hole and it is a solution to the Einstein equations coupled to non-linear electrodynamics…

广义相对论与量子宇宙学 · 物理学 2017-06-15 Sharmanthie Fernando

In the context of $f(R)$ theories of gravity, we address the problem of finding static and spherically symmetric black hole solutions. Several aspects of constant curvature solutions with and without electric charge are discussed. We also…

广义相对论与量子宇宙学 · 物理学 2010-01-15 A. de la Cruz-Dombriz , A. Dobado , A. L. Maroto

The Kerr solution is the cornerstone of General Relativity (GR) for modelling astrophysical rotating black holes and for testing GR through gravitational-wave observations and black hole imaging. Understanding how the Kerr geometry is…

广义相对论与量子宇宙学 · 物理学 2026-01-13 Jibril Ben Achour , Adolfo Cisterna , Hugo Roussille

The theory of f(R)-gravity is one of the theories of modified Einstein gravity. The vacuum solution, on the other hand, of the field equation is the solution for black hole geometry. We establish here an asymptotically flat rotating black…

广义相对论与量子宇宙学 · 物理学 2022-11-07 Arghya Ranjan Das , Banibrata Mukhopadhyay

We investigate a slowly rotating black hole in four-dimensional extended Chern-Simons modified gravity. We obtain an approximate solution that reduces to the Kerr solution when a coupling constant vanishes. The Chern-Simons correction…

广义相对论与量子宇宙学 · 物理学 2009-11-19 Kohkichi Konno , Toyoki Matsuyama , Satoshi Tanda

A curved static de Sitter-like metric is analyzed. The source of curvature is rooted from a constant stress tensor with positive energy density and negative pressures. All the curvature invariants are constant everywhere and the geometry is…

广义相对论与量子宇宙学 · 物理学 2013-04-22 Hristu Culetu

In this paper we study a new symmetry argument that results in a vacuum state with strictly vanishing vacuum energy. This argument exploits the well-known feature that de Sitter and Anti- de Sitter space are related by analytic…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Gerard 't Hooft , Stefan Nobbenhuis

We investigate the evaporation process of a Kerr-de Sitter black hole with the Unruh-Hawking-like vacuum state, which is a realistic vacuum state modelling the evaporation process of a black hole originating from gravitational collapse. We…

广义相对论与量子宇宙学 · 物理学 2021-10-12 Ruth Gregory , Ian G. Moss , Naritaka Oshita , Sam Patrick

We revisit here a recent work on regular rotating black holes. We introduce a new mass function generalizing the commonly used Bardeen and Hayward mass functions and extend the recently proposed solutions in order to accommodate a…

广义相对论与量子宇宙学 · 物理学 2014-05-23 J. C. S. Neves , Alberto Saa

The null geodesics that describe photon orbits in the spacetime of a rotating electrically charged black hole (Kerr-Newman) are solved exactly including the contribution from the cosmological constant. We derive elegant closed form…

广义相对论与量子宇宙学 · 物理学 2015-02-27 G. V. Kraniotis
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