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Title: Ten-dimensional black hole and the D0-brane threshold bound state

Abstract

We discuss the ten-dimensional (10D) black holes made of D0-branes in the regime where the effective coupling is large, and yet the 11D geometry is unimportant. We suggest that these black holes can be interpreted as excitations over the threshold bound state. Thus, the entropy formula for the former is used to predict a scaling region of the wave function of the latter. The horizon radius and the mass gap predicted in this picture agree with the formulas derived from the classical geometry. [copyright] [ital 1999] [ital The American Physical Society]

Authors:
 [1]
  1. (Enrico Fermi Institute, University of Chicago, 5640 South Ellis Avenue, Chicago, Illinois 60637 (United States))
Publication Date:
OSTI Identifier:
6470776
Alternate Identifier(s):
OSTI ID: 6470776
Resource Type:
Journal Article
Journal Name:
Physical Review, D
Additional Journal Information:
Journal Volume: 60:6; Journal ID: ISSN 0556-2821
Country of Publication:
United States
Language:
English
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; BLACK HOLES; BOUND STATE; ENTROPY; EXTENDED PARTICLE MODEL; GEOMETRY; SCALING LAWS; STRING MODELS; WAVE FUNCTIONS; COMPOSITE MODELS; FUNCTIONS; MATHEMATICAL MODELS; MATHEMATICS; PARTICLE MODELS; PHYSICAL PROPERTIES; QUARK MODEL; THERMODYNAMIC PROPERTIES 661310* -- Relativity & Gravitation-- (1992-)

Citation Formats

Li, M. Ten-dimensional black hole and the D0-brane threshold bound state. United States: N. p., 1999. Web. doi:10.1103/PhysRevD.60.066002.
Li, M. Ten-dimensional black hole and the D0-brane threshold bound state. United States. doi:10.1103/PhysRevD.60.066002.
Li, M. Wed . "Ten-dimensional black hole and the D0-brane threshold bound state". United States. doi:10.1103/PhysRevD.60.066002.
@article{osti_6470776,
title = {Ten-dimensional black hole and the D0-brane threshold bound state},
author = {Li, M.},
abstractNote = {We discuss the ten-dimensional (10D) black holes made of D0-branes in the regime where the effective coupling is large, and yet the 11D geometry is unimportant. We suggest that these black holes can be interpreted as excitations over the threshold bound state. Thus, the entropy formula for the former is used to predict a scaling region of the wave function of the latter. The horizon radius and the mass gap predicted in this picture agree with the formulas derived from the classical geometry. [copyright] [ital 1999] [ital The American Physical Society]},
doi = {10.1103/PhysRevD.60.066002},
journal = {Physical Review, D},
issn = {0556-2821},
number = ,
volume = 60:6,
place = {United States},
year = {1999},
month = {9}
}