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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...
Autores principales: | , , , |
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Lenguaje: | eng |
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1997
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/0264-9381/14/5/005 http://cds.cern.ch/record/319106 |
_version_ | 1780890541588742144 |
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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 |