String Propagation in a Black Hole Geometry

نویسندگان

  • Robbert Dijkgraaf
  • Herman Verlinde
  • Joseph Henry
  • Erik Verlinde
چکیده

We consider string theory in the background of the two-dimensional black hole as described by the SL(2, R)/U(1) coset theory recently introduced by Witten. We study the spectrum of this conformal field theory, and give explicit representations for the tachyon vertex operators in terms of SL(2, R) matrix elements. This is used to compute the scattering of strings off the black hole and to show that the string propagator exhibits Hawking radiation. We further discuss the role of winding states and the appearance of bound states in the Euclidean solution. We find that target space duality in the Lorentzian theory interchanges the black hole horizon with the space-time singularity. We conclude with a comparison with the non-critical c = 1 string and its formulation as a gauged SL(2, R) WZW model.

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

D-Brane Propagation in Two-Dimensional Black Hole Geometries

We study propagation of D0-brane in two-dimensional Lorentzian black hole backgrounds by the method of boundary conformal field theory of SL(2,R)/U(1) supercoset at level k. Typically, such backgrounds arise as near-horizon geometries of k coincident non-extremal NS5-branes, where 1/k measures curvature of the backgrounds in string unit and hence size of string worldsheet effects. At classical ...

متن کامل

ar X iv : h ep - t h / 95 10 23 1 v 2 2 1 N ov 1 99 5 How to Create a 2 - D Black Hole

The interaction of a cosmic string with a four-dimensional stationary black hole is considered. If a part of an infinitely long string passes close to a black hole it can be captured. The final stationary configurations of such captured strings are investigated. A uniqueness theorem is proved, namely it is shown that the minimal 2-D surface Σ describing a captured stationary string coincides wi...

متن کامل

ar X iv : h ep - t h / 95 11 06 9 v 2 1 5 N ov 1 99 5 How to Create a 2 - D Black Hole

The interaction of a cosmic string with a four-dimensional stationary black hole is considered. If a part of an infinitely long string passes close to a black hole it can be captured. The final stationary configurations of such captured strings are investigated. A uniqueness theorem is proved, namely it is shown that the minimal 2-D surface Σ describing a captured stationary string coincides wi...

متن کامل

Ghost-free and Modular Invariant Spectra of a String in SL(2, R) and Three Dimensional Black Hole Geometry

Spectra of a string in SL(2, R) and three dimensional (BTZ) black hole geometry are discussed. We consider a free field realization of ŝl(2, R) different from the standard ones in treatment of zero-modes. Applying this to the string model in SL(2, R), we show that the spectrum is ghost-free. The essence of the argument is the same as Bars’ resolution to the ghost problem, but there are differen...

متن کامل

Noncommutative D3-brane, Black Holes and Attractor Mechanism

We revisit the 4D generalized black hole geometries, obtained by us [1], with a renewed interest, to unfold some aspects of effective gravity in a noncommutative D3-brane formalism. In particular, we argue for the existence of extra dimensions in the gravity decoupling limit in the theory. We show that the theory is rather described by an ordinary geometry and is governed by an effective string...

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 1991