de Broglie–Bohm FRW universes in quantum string cosmology

Detalhes bibliográficos
Autor(a) principal: Marto, João
Data de Publicação: 2001
Outros Autores: Moniz, Paulo
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Texto Completo: http://hdl.handle.net/10400.6/6489
Resumo: The purpose of this paper is to establish possible implications of the de Broglie–Bohm interpretation of quantum mechanics towards superstring cosmological dynamics. In this context, we investigate spatially flat FRW models retrieved from scalar-tensor theories of gravity with a cosmological constant present in the gravitational sector. These models are further characterized by the presence of different types of de Broglie– Bohm quantum potential terms. These are constructed from various classes of wave packets formed by superpositions of Bessel functions of different imaginary orders. As far as pre-big-bang scenarios are concerned, we find that quantum potentials yield varied types of an amplified influence of the singular classical boundary into the FRW early dynamics. Some consequences of the de Broglie–Bohm program towards pre-big-bang inflation and the graceful exit problem are then discussed. Other cosmological scenarios are also studied by means of modulation effects extracted from additional wave packets. We subsequently obtain a broader set of new solutions. Among the new solutions we find that they could still be related by duality properties, although a separation into pre- and post-big-bang classes is less clear. Some solutions show a cyclical behavior. Inflationary solutions can be identified and some of their dynamical features are subsequently analyzed. In particular, we discuss some of the differences between string inspired inflationary cosmologies with quantum potentials. The results suggest that de Broglie–Bohm quantum gravitational terms slow down inflation, constituting an effect similar to others previously described in the literature.
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spelling de Broglie–Bohm FRW universes in quantum string cosmologyQuantum string cosmologyThe purpose of this paper is to establish possible implications of the de Broglie–Bohm interpretation of quantum mechanics towards superstring cosmological dynamics. In this context, we investigate spatially flat FRW models retrieved from scalar-tensor theories of gravity with a cosmological constant present in the gravitational sector. These models are further characterized by the presence of different types of de Broglie– Bohm quantum potential terms. These are constructed from various classes of wave packets formed by superpositions of Bessel functions of different imaginary orders. As far as pre-big-bang scenarios are concerned, we find that quantum potentials yield varied types of an amplified influence of the singular classical boundary into the FRW early dynamics. Some consequences of the de Broglie–Bohm program towards pre-big-bang inflation and the graceful exit problem are then discussed. Other cosmological scenarios are also studied by means of modulation effects extracted from additional wave packets. We subsequently obtain a broader set of new solutions. Among the new solutions we find that they could still be related by duality properties, although a separation into pre- and post-big-bang classes is less clear. Some solutions show a cyclical behavior. Inflationary solutions can be identified and some of their dynamical features are subsequently analyzed. In particular, we discuss some of the differences between string inspired inflationary cosmologies with quantum potentials. The results suggest that de Broglie–Bohm quantum gravitational terms slow down inflation, constituting an effect similar to others previously described in the literature.This research work was supported by grants ESO/PRO/ 1258/98, CERN/P/FIS/15190/1999 and POCTI/32327/P/FIS/ 2000 as well as by financial assistance from the Gulbenkian Foundation.American Physical SocietyuBibliorumMarto, JoãoMoniz, Paulo2018-11-26T11:47:02Z20012001-01-01T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10400.6/6489eng10.1103/PhysRevD.65.023516metadata only accessinfo:eu-repo/semantics/openAccessreponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãoinstacron:RCAAP2023-12-15T09:44:58Zoai:ubibliorum.ubi.pt:10400.6/6489Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-20T00:47:12.268142Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãofalse
dc.title.none.fl_str_mv de Broglie–Bohm FRW universes in quantum string cosmology
title de Broglie–Bohm FRW universes in quantum string cosmology
spellingShingle de Broglie–Bohm FRW universes in quantum string cosmology
Marto, João
Quantum string cosmology
title_short de Broglie–Bohm FRW universes in quantum string cosmology
title_full de Broglie–Bohm FRW universes in quantum string cosmology
title_fullStr de Broglie–Bohm FRW universes in quantum string cosmology
title_full_unstemmed de Broglie–Bohm FRW universes in quantum string cosmology
title_sort de Broglie–Bohm FRW universes in quantum string cosmology
author Marto, João
author_facet Marto, João
Moniz, Paulo
author_role author
author2 Moniz, Paulo
author2_role author
dc.contributor.none.fl_str_mv uBibliorum
dc.contributor.author.fl_str_mv Marto, João
Moniz, Paulo
dc.subject.por.fl_str_mv Quantum string cosmology
topic Quantum string cosmology
description The purpose of this paper is to establish possible implications of the de Broglie–Bohm interpretation of quantum mechanics towards superstring cosmological dynamics. In this context, we investigate spatially flat FRW models retrieved from scalar-tensor theories of gravity with a cosmological constant present in the gravitational sector. These models are further characterized by the presence of different types of de Broglie– Bohm quantum potential terms. These are constructed from various classes of wave packets formed by superpositions of Bessel functions of different imaginary orders. As far as pre-big-bang scenarios are concerned, we find that quantum potentials yield varied types of an amplified influence of the singular classical boundary into the FRW early dynamics. Some consequences of the de Broglie–Bohm program towards pre-big-bang inflation and the graceful exit problem are then discussed. Other cosmological scenarios are also studied by means of modulation effects extracted from additional wave packets. We subsequently obtain a broader set of new solutions. Among the new solutions we find that they could still be related by duality properties, although a separation into pre- and post-big-bang classes is less clear. Some solutions show a cyclical behavior. Inflationary solutions can be identified and some of their dynamical features are subsequently analyzed. In particular, we discuss some of the differences between string inspired inflationary cosmologies with quantum potentials. The results suggest that de Broglie–Bohm quantum gravitational terms slow down inflation, constituting an effect similar to others previously described in the literature.
publishDate 2001
dc.date.none.fl_str_mv 2001
2001-01-01T00:00:00Z
2018-11-26T11:47:02Z
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