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Exactly solvable string models of curved space-time backgrounds

We consider a new 3-parameter class of exact 4-dimensional solutions in closed string theory and solve the corresponding string model, determining the physical spectrum and the partition function. The background fields (4-metric, antisymmetric tensor, two Kaluza-Klein vector fields, dilaton and modu...

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Detalles Bibliográficos
Autores principales: Russo, J.G., Tseytlin, Arkady A.
Lenguaje:eng
Publicado: 1995
Materias:
Acceso en línea:https://dx.doi.org/10.1016/0550-3213(95)00245-N
http://cds.cern.ch/record/276490
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author Russo, J.G.
Tseytlin, Arkady A.
author_facet Russo, J.G.
Tseytlin, Arkady A.
author_sort Russo, J.G.
collection CERN
description We consider a new 3-parameter class of exact 4-dimensional solutions in closed string theory and solve the corresponding string model, determining the physical spectrum and the partition function. The background fields (4-metric, antisymmetric tensor, two Kaluza-Klein vector fields, dilaton and modulus) generically describe axially symmetric stationary rotating (electro)magnetic flux-tube type universes. Backgrounds of this class include both the dilatonic Melvin solution and the uniform magnetic field solution discussed earlier as well as some singular space-times. Solvability of the string sigma model is related to its connection via duality to a much simpler looking model which is a "twisted" product of a flat 2-space and a space dual to 2-plane. We discuss some physical properties of this model as well as a number of generalizations leading to larger classes of exact 4-dimensional string solutions.
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spelling cern-2764902023-03-14T18:55:54Zdoi:10.1016/0550-3213(95)00245-Nhttp://cds.cern.ch/record/276490engRusso, J.G.Tseytlin, Arkady A.Exactly solvable string models of curved space-time backgroundsParticle Physics - TheoryWe consider a new 3-parameter class of exact 4-dimensional solutions in closed string theory and solve the corresponding string model, determining the physical spectrum and the partition function. The background fields (4-metric, antisymmetric tensor, two Kaluza-Klein vector fields, dilaton and modulus) generically describe axially symmetric stationary rotating (electro)magnetic flux-tube type universes. Backgrounds of this class include both the dilatonic Melvin solution and the uniform magnetic field solution discussed earlier as well as some singular space-times. Solvability of the string sigma model is related to its connection via duality to a much simpler looking model which is a "twisted" product of a flat 2-space and a space dual to 2-plane. We discuss some physical properties of this model as well as a number of generalizations leading to larger classes of exact 4-dimensional string solutions.We consider a new 3-parameter class of exact 4-dimensional solutions in closed string theory and solve the corresponding string model, determining the physical spectrum and the partition function. The background fields (4-metric, antisymmetric tensor, two Kaluza-Klein vector fields, dilaton and modulus) generically describe axially symmetric stationary rotating (electro)magnetic flux-tube type universes. Backgrounds of this class include both the dilatonic Melvin solution and the uniform magnetic field solution discussed earlier as well as some singular space-times. Solvability of the string sigma model is related to its connection via duality to a much simpler looking model which is a "twisted" product of a flat 2-space and a space dual to 2-plane. We discuss some physical properties of this model as well as a number of generalizations leading to larger classes of exact 4-dimensional string solutions.We consider a new 3-parameter class of exact 4-dimensional solutions in closed string theory and solve the corresponding string model, determining the physical spectrum and the partition function. The background fields (4-metric, antisymmetric tensor, two Kaluza-Klein vector fields, dilaton and modulus) generically describe axially symmetric stationary rotating (electro) magnetic flux-tube type universes. Backgrounds of this class include both the “dilatonic” ( a = 1) and “Kaluza-Klein” ( a = √3) Melvin solutions and the uniform magnetic field solution, as well as some singular space-times. Solvability of the string σ-model is related to its connection via duality to a simpler model which is a “twisted” product of a flat 2-space and a space dual to 2-plane. We discuss some physical properties of this model (tachyonic instabilities in the spectrum, gyromagnetic ratio, issue of singularities, etc.). It provides one of the first examples of a consistent solvable conformal string model with explicit D = 4 curved space-time interpretation.hep-th/9502038CERN-TH-95-20CERN-TH-95-020IMPERIAL-TP-94-95-17CERN-TH-95-20IMPERIAL-TP-94-95-17oai:cds.cern.ch:2764901995-02-06
spellingShingle Particle Physics - Theory
Russo, J.G.
Tseytlin, Arkady A.
Exactly solvable string models of curved space-time backgrounds
title Exactly solvable string models of curved space-time backgrounds
title_full Exactly solvable string models of curved space-time backgrounds
title_fullStr Exactly solvable string models of curved space-time backgrounds
title_full_unstemmed Exactly solvable string models of curved space-time backgrounds
title_short Exactly solvable string models of curved space-time backgrounds
title_sort exactly solvable string models of curved space-time backgrounds
topic Particle Physics - Theory
url https://dx.doi.org/10.1016/0550-3213(95)00245-N
http://cds.cern.ch/record/276490
work_keys_str_mv AT russojg exactlysolvablestringmodelsofcurvedspacetimebackgrounds
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