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Non-Supersymmetric Open String Vacua
We review the construction of non-supersymmetric open string vacua in various dimensions. They can be obtained either projecting the (compactified) non-supersymmetric 0B theory, or applying the Scherk-Schwarz mechanism to open strings. Generically, these vacua generate a non-vanishing cosmological c...
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Lenguaje: | eng |
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1999
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Acceso en línea: | https://dx.doi.org/10.22323/1.002.0015 http://cds.cern.ch/record/393044 |
_version_ | 1780893790644469760 |
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author | Angelantonj, Carlo |
author_facet | Angelantonj, Carlo |
author_sort | Angelantonj, Carlo |
collection | CERN |
description | We review the construction of non-supersymmetric open string vacua in various dimensions. They can be obtained either projecting the (compactified) non-supersymmetric 0B theory, or applying the Scherk-Schwarz mechanism to open strings. Generically, these vacua generate a non-vanishing cosmological constant. However, one can construct particular kinds of Scherk-Schwarz compactifications with vanishing cosmological constant, at least for low orders, based on asymmetric orbifolds. A generic feature of these models is that supersymmetry remains unbroken on the branes at all mass level, while it is broken in the bulk in a way that preserves Fermi-Bose degeneracy at each mass level in the perturbative string spectrum. |
id | cern-393044 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1999 |
record_format | invenio |
spelling | cern-3930442019-09-30T06:29:59Zdoi:10.22323/1.002.0015http://cds.cern.ch/record/393044engAngelantonj, CarloNon-Supersymmetric Open String VacuaParticle Physics - TheoryWe review the construction of non-supersymmetric open string vacua in various dimensions. They can be obtained either projecting the (compactified) non-supersymmetric 0B theory, or applying the Scherk-Schwarz mechanism to open strings. Generically, these vacua generate a non-vanishing cosmological constant. However, one can construct particular kinds of Scherk-Schwarz compactifications with vanishing cosmological constant, at least for low orders, based on asymmetric orbifolds. A generic feature of these models is that supersymmetry remains unbroken on the branes at all mass level, while it is broken in the bulk in a way that preserves Fermi-Bose degeneracy at each mass level in the perturbative string spectrum.hep-th/9907054CPHT-722oai:cds.cern.ch:3930441999-07-09 |
spellingShingle | Particle Physics - Theory Angelantonj, Carlo Non-Supersymmetric Open String Vacua |
title | Non-Supersymmetric Open String Vacua |
title_full | Non-Supersymmetric Open String Vacua |
title_fullStr | Non-Supersymmetric Open String Vacua |
title_full_unstemmed | Non-Supersymmetric Open String Vacua |
title_short | Non-Supersymmetric Open String Vacua |
title_sort | non-supersymmetric open string vacua |
topic | Particle Physics - Theory |
url | https://dx.doi.org/10.22323/1.002.0015 http://cds.cern.ch/record/393044 |
work_keys_str_mv | AT angelantonjcarlo nonsupersymmetricopenstringvacua |