Diffeomorphism symmetries near a timelike surface in black hole spacetime

نویسندگان

چکیده

Recently symmetries of gravity and gauge fields in the asymptotic regions spacetime have been shown to play vital role their low energy scattering phenomena. Further, for black hole spacetime, near horizon symmetry has observed possible understanding underlying degrees freedom thermodynamic behaviour horizon. Following similar idea, this paper, we analyzed associated algebra a timelike surface which is situated at any arbitrary radial position embedded spacetime. In paper considered both Schwarzschild Kerr spacetimes. The families hypersurfaces with constant coordinate (outside horizon) these spacetimes nature divide space into two distinct regions. turned out be reminiscent Bondi-Metzner-Sach (BMS) symmetry, found null infinity.

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

On Diffeomorphism Invariance and Black Hole Entropy

The Noether-charge realization and the Hamiltonian realization for the diff(M) algebra in diffeomorphism invariant gravitational theories are studied in a covariant formalism. For the Killing vector fields, the Nother-charge realization leads to the mass formula as an entire vanishing Noether charge for the vacuum black hole spacetimes in general relativity and the corresponding first law of th...

متن کامل

Black Hole Evaporation in Noncommutative Spacetime

A toy model based upon the q-deformation description for studying the radiation spectrum of black hole is proposed. The starting point is to try to consider the spacetime noncommutativity and to realize it by using a qdeformation algebraic technique. We calculated the radiation spectrum of Schwarzschild black hole in this framework. The new distribution deviates from the standard thermal spectr...

متن کامل

Spacetime Duality of BTZ Black Hole

We consider the duality of the quasilocal black hole thermodynamics, explicitly the quasilocal black hole thermodynamic first law, in BTZ black hole solution as a special one of the three-dimensional low energy effective string theory. E-mail address : [email protected] E-mail address : [email protected] E-mail address : [email protected] 1

متن کامل

Black hole evaporation rates without spacetime.

Verlinde recently suggested that gravity, inertia, and even spacetime may be emergent properties of an underlying thermodynamic theory. This vision was motivated in part by Jacobson's 1995 surprise result that the Einstein equations of gravity follow from the thermodynamic properties of event horizons. Taking a first tentative step in such a program, we derive the evaporation rate (or radiation...

متن کامل

Supersymmetric Rotating Black Hole in a Compactified Spacetime

We construct a supersymmetric rotating black hole with asymptotically flat four-dimensional spacetime times a circle, by superposing an infinite number of BMPV black hole solutions at the same distance in one direction. The near horizon structure is the same as that of the five-dimensional BMPV black hole. The rotation of this black hole can exceed the Kerr bound in general relativity (q ≡ a/G4...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Classical and Quantum Gravity

سال: 2021

ISSN: ['1361-6382', '0264-9381']

DOI: https://doi.org/10.1088/1361-6382/ac0765