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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...
Autores principales: | , |
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Lenguaje: | eng |
Publicado: |
1995
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Acceso en línea: | https://dx.doi.org/10.1016/0550-3213(95)00245-N http://cds.cern.ch/record/276490 |
_version_ | 1780887561560915968 |
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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. |
id | cern-276490 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1995 |
record_format | invenio |
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 AT tseytlinarkadya exactlysolvablestringmodelsofcurvedspacetimebackgrounds |