Return to search

Spacetime boundaries as orbifolds

The current excitement surrounding string theory prompted us to tackle the problem of black hole radiation. Claims have been made concerning a possible 'stringy mechanism' that would avoid the singularity problem by giving a divergent energy-dissipation rate. As a check on such arguments, the Casimir energy of the string between two infinite parallel mirrors is computed using the closed, oriented bosonic string. Such a calculation is also a prerequisite to the understanding of the more interesting situation of string behaviour in the presence of accelerating boundaries. The formalism used here is the first-quantized Polyakov approach, which most simply translates to an orbifold problem.

Identiferoai:union.ndltd.org:LACETR/oai:collectionscanada.gc.ca:QMM.59395
Date January 1989
CreatorsHambli, Noureddine
PublisherMcGill University
Source SetsLibrary and Archives Canada ETDs Repository / Centre d'archives des thèses électroniques de Bibliothèque et Archives Canada
LanguageEnglish
Detected LanguageEnglish
TypeElectronic Thesis or Dissertation
Formatapplication/pdf
CoverageMaster of Science (Department of Physics.)
RightsAll items in eScholarship@McGill are protected by copyright with all rights reserved unless otherwise indicated.
Relationalephsysno: 001067757, proquestno: AAIMM63561, Theses scanned by UMI/ProQuest.

Page generated in 0.0135 seconds