Geometrical and hydrodynamic aspects of five-dimensional Schwarzschild black hole

نویسندگان

چکیده

برای دانلود رایگان 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

Scalar gravitational perturbations and quasinormal modes in the five dimensional Schwarzschild black hole

We calculate the quasinormal modes (QNMs) for gravitational perturbations of the Schwarzschild black hole in the five dimensional (5D) spacetime with a continued fraction method. As shown by Kodama and Ishibashi, the gravitational perturbations of higher-dimensional (higher-D) Schwarzschild black holes can be divided into three decoupled classes, namely scalar-gravitational, vectorgravitational...

متن کامل

Entropy of Schwarzschild black hole and string-black hole correspondence

The string-black hole correspondence is considered in the context of the correspondence principle proposed recently by Horowitz and Polchinski [7]. We demonstrate that the entropy of string states and the entropy of a Schwarzschild black hole can be matched including the subleading terms which depend on mass logarithmically. We argue the necessity to include the string interaction (with couplin...

متن کامل

Entropy of the three dimensional Schwarzschild - de Sitter black hole

We study the three dimensional Schwarzschild-de Sitter (SdS3) black hole which corresponds essentially to a conical defect. We compute the mass of the SdS3 black hole from the correct definition of the mass in asymptotically de Sitter space. Then we clarify the relation between the mass, entropy and temperature for this black hole without any ambiguity. Also we establish the SdS3/CFT2-correspon...

متن کامل

Schwarzschild Black Hole and Area Law

Using a graphical analysis, we show that for the horizon radius rh & 4.8 √ θ, the standard semiclassical Bekenstein-Hawking area law for noncommutative Schwarzschild black hole exactly holds for all orders of θ. We also give the corrections to the area law to get the exact nature of the Bekenstein-Hawking entropy when rh < 4.8 √ θ till the extremal point rh = 3.0 √ θ. The familiar notion of bla...

متن کامل

Area spectrum of the Schwarzschild black hole.

We consider a Hamiltonian theory of spherically symmetric vacuum Einstein gravity under Kruskal-like boundary conditions in variables associated with the Einstein-Rosen wormhole throat. The configuration variable in the reduced classical theory is the radius of the throat, in a foliation that is frozen at the left hand side infinity but asymptotically Minkowski at the right hand side infinity, ...

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: Journal of the Korean Physical Society

سال: 2014

ISSN: 0374-4884,1976-8524

DOI: 10.3938/jkps.64.1928