Cargando…

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...

Descripción completa

Detalles Bibliográficos
Autor principal: Angelantonj, Carlo
Lenguaje:eng
Publicado: 1999
Materias:
Acceso en línea:https://dx.doi.org/10.22323/1.002.0015
http://cds.cern.ch/record/393044
_version_ 1780893790644469760
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