X iv : g r - qc / 9 90 20 63 v 2 2 6 M ay 1 99 9 Remarks on Conserved Quantities and Entropy of BTZ Black Hole Solutions . Part I : the General Setting

نویسندگان

  • L. Fatibene
  • M. Ferraris
  • M. Francaviglia
چکیده

The BTZ stationary black hole solution is considered and its mass and angular momentum are calculated by means of Nöther theorem. In particular, relative conserved quantities with respect to a suitably fixed background are discussed. Entropy is then computed in a geometric and macroscopic framework, so that it satisfies the first principle of thermodynamics. In order to compare this more general framework to the prescription by Wald et al. we construct the maximal extension of the BTZ horizon by means of Kruskal–like coordinates. A discussion about the different features of the two methods for computing entropy is finally developed.

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

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Fe b 19 99 Remarks on Conserved Quantities and Entropy of BTZ Black Hole Solutions . Part I : the General Setting

The BTZ stationary black hole solution is considered and its mass and angular momentum are calculated by means of Nöther theorem. In particular, relative conserved quantities with respect to a suitably fixed background are discussed. Entropy is then computed in a geometric and macroscopic framework, so that it satisfies the first principle of thermodynamics. In order to compare this more genera...

متن کامل

ar X iv : g r - qc / 9 40 40 14 v 1 8 A pr 1 99 4 EXOTIC BLACK HOLES ∗

Black hole solutions can be used to shed light on general issues in General Relativity and Quantum Physics. Black–hole hair, entropy and naked singularities are considered here, along with some implications for the inflationary universe scenario.

متن کامل

65 v 1 2 2 Fe b 19 99 Remarks on Conserved Quantities and Entropy of BTZ Black Hole Solutions . Part II : BCEA Theory

The BTZ black hole solution for (2 + 1)-spacetime is considered as a solution of a triad-affine theory (BCEA) in which topological matter is introduced to replace the cosmological constant in the model. Conserved quantities and entropy are calculated via Nöther theorem, reproducing in a geometrical and global framework earlier results found in the literature using local formalisms. Ambiguities ...

متن کامل

ar X iv : h ep - t h / 98 10 03 9 v 1 6 O ct 1 99 8 Remarks on Nöther charges and black holes en - tropy

We criticize and generalize some properties of Nöther charges presented in a paper by V. Iyer and R. M. Wald and their application to entropy of black holes. The first law of black holes thermodynamics is proven for any gauge-natural field theory. As an application charged Kerr-Newman solutions are considered. As a further example we consider a (1 + 2) black hole solution. 1

متن کامل

ar X iv : g r - qc / 9 90 40 34 v 2 1 7 M ay 1 99 9 SU - ITP / 99 - 18 4 D quantum black hole physics from 2 D models ?

Minimally coupled 4D scalar fields in Schwarzschild space-time are considered. Dimensional reduction to 2D leads to a well known anomaly induced effective action, which we consider here in a local form with the introduction of auxiliary fields. Boundary conditions are imposed on them in order to select the appropriate quantum states (Boulware, Unruh annd Israel-Hartle-Hawking). The stress tenso...

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

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

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 1999