gr - q c / 97 06 03 0 1 1 Ju n 19 97 1 Black Hole Entropy : a spacetime foam approach

نویسنده

  • Fabio Scardigli
چکیده

I introduce the spacetime foam structure by reviewing briefly the ideas of Wheeler, the topological fluctuations and the virtual black holes possibility. The contribution of Jacobson (the equation of state of the foam) is recalled. In the second part, I introduce a model of spacetime foam at the surface of the event horizon of a black hole. I apply these ideas to the calculus of the number of states of a black hole, of its entropy and of other thermodynamical properties. A formula for the number of microholes on the surface of the event horizon is derived. Subsequently, I extend the thermodynamical properties of the event horizon to thermodynamical properties of the space. Here I face with the problem of the maximum entropy contained in a space region of a given volume. In the end, on the basis of the results previously obtained, I briefly treat the possibility of micro black holes creation by Unruh Effect.

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

ar X iv : h ep - t h / 97 11 05 3 v 1 7 N ov 1 99 7 hep - th / 9711053 BLACK HOLE ENTROPY IN M - THEORY

Extremal black holes in M-theory compactification on M × S 1 are microscopically represented by fivebranes wrapping P × S 1 , where M is a Calabi-Yau threefold and P is a four-cycle in M. Additional spacetime charges arise from momentum around the S 1 and expectation values for the self-dual three-form field strength in the fivebrane. The microscopic entropy of the fivebrane as a function of al...

متن کامل

A Spacetime Foam Approach to the Schwarzschild-de Sitter Entropy

The entropy for a black hole in a de Sitter space is approached within the framework of spacetime foam. A simple model made by N wormholes in a semiclassical approximation, is taken under examination to compute the entropy for such a case. An extension to the extreme case when the black hole and cosmological horizons are equal is discussed.

متن کامل

30 60 97 v 1 2 1 Ju n 20 03 Notes on Choptuik Phenomena

We review the work going on in black-hole physics during the last ten years, called the Choptuik Phenomenon. * [email protected]

متن کامل

06 13 1 v 1 1 6 Ju n 20 00 Black Hole Entropy in 1 + 1 Dimensions from a Quasi - Chern Simons term

We introduce a ’quasi-topological‘ term [1] in D = 1 + 1 dimensions and the entropy for black holes is calculated [2]. The source of entropy in this case is justified by a non-null stress-energy tensor.

متن کامل

ar X iv : h ep - p h / 97 06 31 3 v 1 1 0 Ju n 19 97 Forward - Backward Asymmetry

The Forward-backward asymmetry in the angular distribution of e + e possibility of observing CP-violation through the asymmetries in these two processes is examined.

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 1997