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Expanding and contracting universes in third quantized string cosmology

We discuss the possibility of quantum transitions from the string perturbative vacuum to cosmological configurations characterized by isotropic contraction and decreasing dilaton. When the dilaton potential preserves the sign of the Hubble factor throughout the evolution, such transitions can be rep...

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Detalles Bibliográficos
Autores principales: Buonanno, A., Gasperini, M., Maggiore, M., Ungarelli, C.
Lenguaje:eng
Publicado: 1997
Materias:
Acceso en línea:https://dx.doi.org/10.1088/0264-9381/14/5/005
http://cds.cern.ch/record/319106
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author Buonanno, A.
Gasperini, M.
Maggiore, M.
Ungarelli, C.
author_facet Buonanno, A.
Gasperini, M.
Maggiore, M.
Ungarelli, C.
author_sort Buonanno, A.
collection CERN
description We discuss the possibility of quantum transitions from the string perturbative vacuum to cosmological configurations characterized by isotropic contraction and decreasing dilaton. When the dilaton potential preserves the sign of the Hubble factor throughout the evolution, such transitions can be represented as an anti-tunnelling of the Wheeler--De Witt wave function in minisuperspace or, in a third-quantization language, as the production of pairs of universes out of the vacuum.
id cern-319106
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1997
record_format invenio
spelling cern-3191062023-03-12T05:57:42Zdoi:10.1088/0264-9381/14/5/005http://cds.cern.ch/record/319106engBuonanno, A.Gasperini, M.Maggiore, M.Ungarelli, C.Expanding and contracting universes in third quantized string cosmologyParticle Physics - TheoryWe discuss the possibility of quantum transitions from the string perturbative vacuum to cosmological configurations characterized by isotropic contraction and decreasing dilaton. When the dilaton potential preserves the sign of the Hubble factor throughout the evolution, such transitions can be represented as an anti-tunnelling of the Wheeler--De Witt wave function in minisuperspace or, in a third-quantization language, as the production of pairs of universes out of the vacuum.We discuss the possibility of quantum transitions from the string perturbative vacuum to cosmological configurations characterized by isotropic contraction and decreasing dilaton. When the dilaton potential preserves the sign of the Hubble factor throughout the evolution, such transitions can be represented as an anti-tunnelling of the Wheeler--De Witt wave function in minisuperspace or, in a third-quantization language, as the production of pairs of universes out of the vacuum.We discuss the possibility of quantum transitions from the string perturbative vacuum to cosmological configurations characterized by isotropic contraction and decreasing dilaton. When the dilaton potential preserves the sign of the Hubble factor throughout the evolution, such transitions can be represented as an anti-tunnelling of the Wheeler--De Witt wave function in minisuperspace or, in a third-quantization language, as the production of pairs of universes out of the vacuum.We discuss the possibility of quantum transitions from the string perturbative vacuum to cosmological configurations characterized by isotropic contraction and decreasing dilaton. When the dilaton potential preserves the sign of the Hubble factor throughout the evolution, such transitions can be represented as an anti-tunnelling of the Wheeler--De Witt wave function in minisuperspace or, in a third-quantization language, as the production of pairs of universes out of the vacuum.hep-th/9701146CERN-TH-96-322IFUP-TH-96-65CERN-TH/96-322CERN-TH-96-322IFUP-TH-96-65oai:cds.cern.ch:3191061997-01-27
spellingShingle Particle Physics - Theory
Buonanno, A.
Gasperini, M.
Maggiore, M.
Ungarelli, C.
Expanding and contracting universes in third quantized string cosmology
title Expanding and contracting universes in third quantized string cosmology
title_full Expanding and contracting universes in third quantized string cosmology
title_fullStr Expanding and contracting universes in third quantized string cosmology
title_full_unstemmed Expanding and contracting universes in third quantized string cosmology
title_short Expanding and contracting universes in third quantized string cosmology
title_sort expanding and contracting universes in third quantized string cosmology
topic Particle Physics - Theory
url https://dx.doi.org/10.1088/0264-9381/14/5/005
http://cds.cern.ch/record/319106
work_keys_str_mv AT buonannoa expandingandcontractinguniversesinthirdquantizedstringcosmology
AT gasperinim expandingandcontractinguniversesinthirdquantizedstringcosmology
AT maggiorem expandingandcontractinguniversesinthirdquantizedstringcosmology
AT ungarellic expandingandcontractinguniversesinthirdquantizedstringcosmology