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We establish a direct connection between the interior curvature structure of nonsingular black holes (BHs) with a Minkowski core and their observable optical signatures. By classifying these spacetimes into three fundamental types, Type I…

广义相对论与量子宇宙学 · 物理学 2025-12-25 Ming-Xin Li , Jin Pu , Yi Ling , Guo-Ping Li

In this work we study the spectral dimensionality of spacetime around a radiating Schwarzschild black hole using a recently introduced formalism of quantum gravity, where the alterations of the gravitational field produced by the radiation…

广义相对论与量子宇宙学 · 物理学 2025-05-07 Mauricio Bellini , Juan Ignacio Musmarra , Pablo Alejandro Sanchez , Alan Sebastian Morales

Scale dependence at the level of the effective action is a generic result of quantum field theory. Allowing for scale dependence of the gravitational couplings leads to a generalization of the corresponding field equations. In this work,…

高能物理 - 理论 · 物理学 2016-10-27 Benjamin Koch , Ignacio A. Reyes , Angel Rincon

This paper reviews the basic features of the theory of curvature perturbations in Kerr spacetime, which is customarily written in terms of gauge invariant components of the Weyl tensor which satisfy a perturbation equation known as the…

广义相对论与量子宇宙学 · 物理学 2011-04-15 Ramon Lopez-Aleman

The one-loop contributions to the entropy for a massive scalar field in a Kerr black hole are investigated using an approximation of the metric, which, after a conformal transformation, permits to work in a Rindler-like spacetime. Of…

广义相对论与量子宇宙学 · 物理学 2009-10-30 Guido Cognola

We consider the thermodynamics of minimally coupled massive scalar field in 3+1 dimensional constant curvature black hole background. The brick wall model of 't Hooft is used. When Schwarzschild like coordinates are used it is found that…

广义相对论与量子宇宙学 · 物理学 2007-05-23 K. Ghosh

Black hole entropy is identified with the counting of the dynamical degrees of freedom of trapped gravitational modes continually sourced by the Hawking-Unruh process. In the context of linear perturbations of Schwarzschild spacetime the…

广义相对论与量子宇宙学 · 物理学 2026-01-14 Seth Major , Daniel Rodriguez , Thomas Takis

We construct a static spherically symmetric regular black hole with a Minkowski core, and a degenerate inner horizon with vanishing surface gravity. The spacetime contains a non-extremal outer horizon and exhibits two notable features.…

广义相对论与量子宇宙学 · 物理学 2026-05-18 Zhong-Wen Feng , Hong-Lin Liu , Yi Ling , Qing-Quan Jiang

We provide an invariant characterization of the physical properties of the Kerr spacetime. We introduce two dimensionless invariants, constructed out of some known curvature invariants, that act as detectors for the event horizon and…

广义相对论与量子宇宙学 · 物理学 2015-04-14 Majd Abdelqader , Kayll Lake

We solve the problem of expressing the Weyl scalars $\psi $ that describe gravitational perturbations of a Kerr black hole in terms of Cauchy data. To do so we use geometrical identities (like the Gauss-Codazzi relations) as well as…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Manuela Campanelli , Carlos O. Lousto , John Baker , Gaurav Khanna , Jorge Pullin

Considering corrections to all orders in the Planck length on the quantum state density from a generalized uncertainty principle (GUP), we calculate the statistical entropy of the scalar field on the background of the Schwarzschild black…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Yong-Wan Kim , Young-Jai Park

Combining insights from both the effective field theory of quantum gravity and black hole thermodynamics, we derive two novel consistency relations to be satisfied by any quantum theory of gravity. First, we show that a particular…

广义相对论与量子宇宙学 · 物理学 2020-02-05 Basem Kamal El-Menoufi , Sonali Mohapatra

It is usually stated that the information storing region associated with the Bekenstein-Hawking entropy is enclosed by a sphere of diameter equal twice the Schwarzschild radius. We point out that this cannot apply to a quantum black hole.…

高能物理 - 理论 · 物理学 2024-01-26 Abram Akal

We construct exact initial data for closed cosmological models filled with regularly arranged black holes in the presence of $\Lambda$. The intrinsic geometry of the 3-dimensional space described by this data is a sum of simple closed-form…

广义相对论与量子宇宙学 · 物理学 2017-03-15 Jessie Durk , Timothy Clifton

Space-time singularities, viz. Big bang, Big crunch and black holes have been shown to follow from the singularity theorems of General relativity. Whether the entropy at such infinite proper-time objects can be other than zero has also been…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Akinbo Ojo

We reconsider space-time singularities in classical Einsteinian general relativity: with the help of several new co-ordinate systems we show that the Schwarzschild solution can be extended beyond the curvature singularity at r=0. The…

广义相对论与量子宇宙学 · 物理学 2010-04-06 K. Peeters , C. Schweigert , J. W. van Holten

The divergence of curvature invariants at a given point signals the impossibility of extending the spacetime to that point, with the derivative order of these diverging invariants determining the differentiability class of the considered…

广义相对论与量子宇宙学 · 物理学 2026-03-06 Tommaso Antonelli , Marco Sebastianutti

We propose a fundamental duality between the geometric properties of spacetime and the informational content of quantum fields. Specifically, we establish that the curvature of spacetime is directly related to the entanglement entropy of…

广义相对论与量子宇宙学 · 物理学 2025-05-01 Florian Neukart

We first present an overview of the Schwarzschild vacuum spacetime within general relativity, with particular emphasis on the role of scalar polynomial invariants and the null frame approach (and the related Cartan invariants), that…

广义相对论与量子宇宙学 · 物理学 2025-03-18 Alan A. Coley , Nicholas T. Layden , Diego F. Lopez

Critical collapse of a massless scalar field in spherical symmetry is systematically studied. We combine numerical simulations and asymptotic analysis, and synthesize critical collapse, spacetime singularities, and complex science. First…

广义相对论与量子宇宙学 · 物理学 2019-07-30 Jun-Qi Guo , Hongsheng Zhang