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Suppressing the Cosmological Constant in Non-Supersymmetric Type I Strings

We construct non-supersymmetric type I string models which correspond to consistent flat-space solutions of all classical equations of motion. Moreover, the one-loop vacuum energy is naturally fixed by the size of compact extra dimensions which, in the two-dimensional case, can be lowered to a fract...

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Detalles Bibliográficos
Autores principales: Angelantonj, Carlo, Antoniadis, Ignatios
Lenguaje:eng
Publicado: 2003
Materias:
Acceso en línea:https://dx.doi.org/10.1016/j.nuclphysb.2003.09.047
http://cds.cern.ch/record/630349
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author Angelantonj, Carlo
Antoniadis, Ignatios
author_facet Angelantonj, Carlo
Antoniadis, Ignatios
author_sort Angelantonj, Carlo
collection CERN
description We construct non-supersymmetric type I string models which correspond to consistent flat-space solutions of all classical equations of motion. Moreover, the one-loop vacuum energy is naturally fixed by the size of compact extra dimensions which, in the two-dimensional case, can be lowered to a fraction of a millimetre. This class of models has interesting non-abelian gauge groups and can accommodate chiral fermions. In the large radius limit, supersymmetry is recovered in the bulk, while D-brane excitations, although non-supersymmetric, exhibit Fermi-Bose degeneracy at all mass levels. We also give some evidence for a suppression of higher-loop corrections to the vacuum energy.
id cern-630349
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2003
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spelling cern-6303492023-03-14T20:38:30Zdoi:10.1016/j.nuclphysb.2003.09.047http://cds.cern.ch/record/630349engAngelantonj, CarloAntoniadis, IgnatiosSuppressing the Cosmological Constant in Non-Supersymmetric Type I StringsParticle Physics - TheoryWe construct non-supersymmetric type I string models which correspond to consistent flat-space solutions of all classical equations of motion. Moreover, the one-loop vacuum energy is naturally fixed by the size of compact extra dimensions which, in the two-dimensional case, can be lowered to a fraction of a millimetre. This class of models has interesting non-abelian gauge groups and can accommodate chiral fermions. In the large radius limit, supersymmetry is recovered in the bulk, while D-brane excitations, although non-supersymmetric, exhibit Fermi-Bose degeneracy at all mass levels. We also give some evidence for a suppression of higher-loop corrections to the vacuum energy.We construct non-supersymmetric type I string models which correspond to consistent flat-space solutions of all classical equations of motion. Moreover, the one-loop vacuum energy is naturally fixed by the size of compact extra dimensions which, in the two-dimensional case, can be lowered to a fraction of a millimetre. This class of models has interesting non-abelian gauge groups and can accommodate chiral fermions. In the large radius limit, supersymmetry is recovered in the bulk, while D-brane excitations, although non-supersymmetric, exhibit Fermi-Bose degeneracy at all mass levels. We also give some evidence for a suppression of higher-loop corrections to the vacuum energy.We construct non-supersymmetric type I string models which correspond to consistent flat-space solutions of all classical equations of motion. Moreover, the one-loop vacuum energy is naturally fixed by the size of compact extra dimensions which, in the two-dimensional case, can be lowered to a fraction of a millimetre. This class of models has interesting non-abelian gauge groups and can accommodate chiral fermions. In the large radius limit, supersymmetry is recovered in the bulk, while D-brane excitations, although non-supersymmetric, exhibit Fermi-Bose degeneracy at all mass levels. We also give some evidence for a suppression of higher-loop corrections to the vacuum energy.We construct non-supersymmetric type I string models which correspond to consistent flat-space solutions of all classical equations of motion. Moreover, the one-loop vacuum energy is naturally fixed by the size of compact extra dimensions which, in the two-dimensional case, can be lowered to a fraction of a millimetre. This class of models has interesting non-Abelian gauge groups and can accommodate chiral fermions. In the large-radius limit, supersymmetry is recovered in the bulk, while D-brane excitations, although non-supersymmetric, exhibit Fermi–Bose degeneracy at all mass levels. We also give some evidence for a suppression of higher-loop corrections to the vacuum energy.hep-th/0307254CERN-TH-2003-165CERN-TH-2003-165oai:cds.cern.ch:6303492003-07-25
spellingShingle Particle Physics - Theory
Angelantonj, Carlo
Antoniadis, Ignatios
Suppressing the Cosmological Constant in Non-Supersymmetric Type I Strings
title Suppressing the Cosmological Constant in Non-Supersymmetric Type I Strings
title_full Suppressing the Cosmological Constant in Non-Supersymmetric Type I Strings
title_fullStr Suppressing the Cosmological Constant in Non-Supersymmetric Type I Strings
title_full_unstemmed Suppressing the Cosmological Constant in Non-Supersymmetric Type I Strings
title_short Suppressing the Cosmological Constant in Non-Supersymmetric Type I Strings
title_sort suppressing the cosmological constant in non-supersymmetric type i strings
topic Particle Physics - Theory
url https://dx.doi.org/10.1016/j.nuclphysb.2003.09.047
http://cds.cern.ch/record/630349
work_keys_str_mv AT angelantonjcarlo suppressingthecosmologicalconstantinnonsupersymmetrictypeistrings
AT antoniadisignatios suppressingthecosmologicalconstantinnonsupersymmetrictypeistrings