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相关论文: On the gravitational entropy of accelerating black…

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We analyze the gravitational entropy defined by the Weyl curvature for the Hayward black hole, which is one of the regular black holes without singularity in the event horizon. Using the definition by the ratio of the Weyl curvature scalar…

广义相对论与量子宇宙学 · 物理学 2025-04-16 Hideo Iguchi

Pure thermodynamical considerations to describe the entropic evolution of the universe seem to violate the Second Law of Thermodynamics. This suggests that the gravitational field itself has entropy. In this paper we expand recent work done…

宇宙学与河外天体物理 · 物理学 2015-03-19 Gustavo E. Romero , Romain Thomas , Daniela Pérez

Partly motivated by the arrow of time problem in cosmology and the Weyl curvature hypothesis formulated by Roger Penrose, previous works in the literature have proposed - among other possibilities - the square of the Weyl curvature, as…

广义相对论与量子宇宙学 · 物理学 2022-05-12 Daniele Gregoris , Yen Chin Ong

Classical invariants of General Relativity can be used to approximate the entropy of the gravitational field. In this work, we study two proposed estimators based on scalars constructed out from the Weyl tensor, in Kerr spacetime. In order…

广义相对论与量子宇宙学 · 物理学 2015-06-22 Daniela Pérez , Gustavo E. Romero

Here the Weyl curvature hypothesis is examined using the gravitational entropy (GE). We have considered the family of C-metric accelerating black holes and evaluated their corresponding gravitational entropy. Then we studied the GE in some…

广义相对论与量子宇宙学 · 物理学 2024-01-23 Samarjit Chakraborty

There are several reasons to support the idea that entropy might be associated to gravity itself. In the absence of a quantum theory of gravity, classical estimators for the gravitational entropy have been proposed. Any viable description…

广义相对论与量子宇宙学 · 物理学 2025-04-17 Alan Alejandro Pánuco Liñán , Daniela Pérez , Carlos Luna , Gustavo E. Romero

We propose the use of a gravitational uncertainty principle for gravitation. We define the corresponding gravitational Planck's constant and the gravitational quantum of mass. We define entropy in terms of the quantum of gravity with the…

广义相对论与量子宇宙学 · 物理学 2015-06-25 Antonio Alfonso-Faus

We investigate the entropy of black holes in Gauss-Bonnet and Lovelock gravity using the Noether charge approach, in which the entropy is given as the integral of a suitable (n-2) form charge over the event horizon. We compare the results…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Tim Clunan , Simon F. Ross , Douglas J. Smith

The concept of entropy forms the backbone of the principles of thermodynamics. R.C. Tolman initiated the correlation between gravity and thermodynamics. The development of black hole thermodynamics and the generalized second law of…

广义相对论与量子宇宙学 · 物理学 2023-06-27 Sarbari Guha

We formulate the classical gravitational entropy of a horizon as a Noether charge that does not require the notion of a temperature, and which is applicable to horizons that are not necessarily associated with black holes. This introduces a…

高能物理 - 理论 · 物理学 2025-10-06 Sangmin Choi , Malcolm J. Perry

A short overview of black hole entropy in alternative gravitational theories is presented. Motivated by the recent attempts to explain the cosmic acceleration without dark energy, we focus on metric and Palatini f(R) gravity and on…

广义相对论与量子宇宙学 · 物理学 2015-05-19 Valerio Faraoni

Assuming that the near horizon geometry of the black hole solution of the gravity dual to the ABJM model, in the presence of a coupling between the Weyl tensor and the field strength, is $AdS_{2}\times S^{2}$, we compute Sen's entropy…

高能物理 - 理论 · 物理学 2015-04-28 Prieslei Goulart , Horatiu Nastase

We present a class of exact analytic and static, spherically symmetric black hole solutions in the semi-classical Einstein equations with Weyl anomaly. The solutions have two branches, one is asymptotically flat and the other asymptotically…

高能物理 - 理论 · 物理学 2010-04-30 Rong-Gen Cai , Li-Ming Cao , Nobuyoshi Ohta

The universe today, with structure such as stars, galaxies and black holes, seems to have evolved from a very homogeneous initial state. From this it appears as if the entropy of the universe is decreasing, in violation of the second law of…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Oystein Rudjord , Oyvind Gron

We propose a thermodynamically motivated measure of gravitational entropy based on the Bel-Robinson tensor, which has a natural interpretation as the effective super-energy-momentum tensor of free gravitational fields. The specific form of…

广义相对论与量子宇宙学 · 物理学 2015-06-15 Timothy Clifton , George F R Ellis , Reza Tavakol

We explore the quadratic form of the $f(R)=R+bR^2$ gravitational theory to derive rotating $N$-dimensions black hole solutions with $a_i, i\geq 1$ rotation parameters. Here, $R$ is the Ricci scalar, and $b$ is the dimensional parameter. We…

广义相对论与量子宇宙学 · 物理学 2021-03-11 G. G. L. Nashed , Kazuharu Bamba

Penrose suggested that issues with the origin of the second law of thermodynamics and the remarkable homogeneous and isotropic nature of the universe on large scales can be resolved with a concept of an entropy for gravitational fields…

广义相对论与量子宇宙学 · 物理学 2021-11-16 Taha A Malik , Rafael Lopez-Mobilia

We consider numerical black hole solutions in the Weyl conformal geometry, and its associated conformally invariant Weyl quadratic gravity. In this model Einstein gravity (with a positive cosmological constant) is recovered in the…

广义相对论与量子宇宙学 · 物理学 2024-11-18 Jin-Zhao Yang , Shahab Shahidi , Tiberiu Harko

We present and analyze a class of exact spacetimes which describe accelerating black holes with a NUT parameter. First, we verify that the intricate metric found by Chng, Mann and Stelea in 2006 indeed solves Einstein's vacuum field…

广义相对论与量子宇宙学 · 物理学 2020-10-14 Jiri Podolsky , Adam Vratny

Two techniques for computing black hole entropy in generally covariant gravity theories including arbitrary higher derivative interactions are studied. The techniques are Wald's Noether charge approach introduced recently, and a field…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Ted Jacobson , Gungwon Kang , Robert C. Myers
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