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Recently, Verlinde discussed that gravity can be understood as an entropic force caused by changes in the information associated with the positions of material bodies. In the Verlinde's argument, the area law of the black hole entropy plays…

广义相对论与量子宇宙学 · 物理学 2010-05-19 Ahmad Sheykhi

One proposal by Verlinde \cite{Verlinde:2010hp} is that gravity is not a fundamental, but an entropic force. In this way, Verlinde has provide us with a way to derive the Newton's law of gravitation from the Bekenstein-Hawking entropy-area…

广义相对论与量子宇宙学 · 物理学 2016-06-22 R. G. L. Aragão , C. A. S. Silva

Explicit tests are presented of the conjectured entropic origin of the gravitational force. The gravitational force on a test particle in the vicinity of the horizon of a large Schwarzschild black hole in arbitrary spacetime dimensions is…

广义相对论与量子宇宙学 · 物理学 2018-08-08 Sourav Bhattacharya , Panagiotis Charalambous , Theodore N Tomaras , Nicolaos Toumbas

Assuming the hypothesis of the entropic nature of gravity, we calculate generalized Newtonian forces, their associated potentials and field equations, when other, in general non-extensive, entropies are considered instead of the usual…

广义相对论与量子宇宙学 · 物理学 2017-06-28 Aldo Martínez-Merino , Octavio Obregón , Michael P. Ryan

With Verlinde's recent proposal which says that gravity can be identified with an entropic force and considering the effects of generalized uncertainty principle in the black hole entropy-area relation we derive the modified equations for…

广义相对论与量子宇宙学 · 物理学 2013-11-11 Barun Majumder

Recently, Chandrasekaran, Penington and Witten (CPW) have shown that the generalized entropy of the Schwarzschild black hole at the bifurcation surface equals the entropy of an extended von Neumann algebra of quantum observables in the…

高能物理 - 理论 · 物理学 2023-09-26 Mohd Ali , Vardarajan Suneeta

Considering the general quantum corrections to the area law of black hole entropy and adopting the viewpoint that gravity interprets as an entropic force, we derive the modified forms of MOND theory of gravitation and Einstein field…

高能物理 - 理论 · 物理学 2011-04-25 S. H. Hendi , A. Sheykhi

We consider corrections to the Bekenstein Hawking Area Formula for black hole entropy, which have inverse powers of the horizon area for very large horizon areas, for classical spherically symmetric black hole solutions of F(R) modified…

广义相对论与量子宇宙学 · 物理学 2026-02-05 Rohit Das , Parthasarathi Majumdar , Debadrita Mukherjee

Using on-shell amplitude methods, we derive a rotating black hole solution in a generic theory of Einstein gravity with additional terms cubic in the Riemann tensor. We give an explicit expression for the metric in Einsteinian Cubic Gravity…

高能物理 - 理论 · 物理学 2021-03-25 Daniel J. Burger , William T. Emond , Nathan Moynihan

Restricted to a black hole horizon, the ``gauge'' algebra of surface deformations in general relativity contains a Virasoro subalgebra with a calculable central charge. The fields in any quantum theory of gravity must transform accordingly,…

高能物理 - 理论 · 物理学 2010-04-28 S. Carlip

The equivalence principle and its universality enables the geometrical formulation of gravity. In the standard formulation of General Relativity \'a la Einstein, the gravitational interaction is geometrized in terms of the spacetime…

广义相对论与量子宇宙学 · 物理学 2022-11-23 Lavinia Heisenberg , Simon Kuhn , Laurens Walleghem

Wald's entropy formula allows one to find the entropy of black holes' event horizon within any diffeomorphism invariant theory of gravity. When applied to general relativity, the formula yields the Bekenstein-Hawking result but, for any…

广义相对论与量子宇宙学 · 物理学 2015-08-24 Fayçal Hammad

Newtonian gravitation with some slight modifications, along with some highly simplified ideas from quantum field theory allow us to reproduce, at least at the level of back-of-the-envelope calculations, many results of black hole physics.…

广义相对论与量子宇宙学 · 物理学 2016-11-30 Aldo Martínez-Merino , Octavio Obregón , Michael P. Ryan

Using Wilsonian procedure (renormalization group improvement) we discuss the finite quantum corrections to black hole entropy in renormalizable theories. In this way, the Wilsonian black hole entropy is found for GUTs (of asymptotically…

广义相对论与量子宇宙学 · 物理学 2009-09-17 Sergei D. Odintsov , Yongsung Yoon

We propose a new formula for the entropy of a dynamical black hole$-$valid to leading order for perturbations off of a stationary black hole background$-$in an arbitrary classical diffeomorphism covariant Lagrangian theory of gravity in $n$…

高能物理 - 理论 · 物理学 2024-04-02 Stefan Hollands , Robert M. Wald , Victor G. Zhang

We give an exact solution for the static force between two black holes at the turning points in their binary motion. The results are derived by Gibbs' principle and the Bekenstein-Hawking entropy applied to the apparent horizon surfaces in…

高能物理 - 理论 · 物理学 2015-05-28 Maurice H. P. M. van Putten

We calculate quantum gravitational corrections to the entropy of black holes using the Wald entropy formula within an effective field theory approach to quantum gravity. The corrections to the entropy are calculated to second order in…

高能物理 - 理论 · 物理学 2021-09-22 Xavier Calmet , Folkert Kuipers

A toy model of Einstein gravity with a Gauss-Bonnet classically "entropic" term mimicking a quantum correction is considered. The static black hole solution due to Tomozawa is found and generalized with the inclusion of non trivial horizon…

广义相对论与量子宇宙学 · 物理学 2013-10-15 Guido Cognola , Ratbay Myrzakulov , Lorenzo Sebastiani , Sergio Zerbini

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

Starting from an effective action for quantum gravity, we calculate the quantum gravitational corrections to the Wald entropy of a four dimensional non-extremal Reissner-Nordstr\"om (RN) black hole in the limit of small electric charge,…

高能物理 - 理论 · 物理学 2023-05-23 Ruben Campos Delgado
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