Universal approach to cosmological singularities in two-dimensional dilaton gravity

We show that in a large class of two-dimensional models with conformal matter fields, the semiclassical cosmological solutions have a weak coupling singularity if the classical matter content is below a certain threshold. This threshold and the approach to the singularity are model independent. When...

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Autores principales: Martin, G.N., Mazzitelli, F.D.
Formato: JOUR
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_05562821_v50_n2_pR613_Martin
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spelling todo:paper_05562821_v50_n2_pR613_Martin2023-10-03T15:35:29Z Universal approach to cosmological singularities in two-dimensional dilaton gravity Martin, G.N. Mazzitelli, F.D. We show that in a large class of two-dimensional models with conformal matter fields, the semiclassical cosmological solutions have a weak coupling singularity if the classical matter content is below a certain threshold. This threshold and the approach to the singularity are model independent. When the matter fields are not conformally invariant, the singularity persists if the quantum state is the vacuum near the singularity, and could dissappear for other quantum states. © 1994 The American Physical Society. Fil:Martin, G.N. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Mazzitelli, F.D. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_05562821_v50_n2_pR613_Martin
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description We show that in a large class of two-dimensional models with conformal matter fields, the semiclassical cosmological solutions have a weak coupling singularity if the classical matter content is below a certain threshold. This threshold and the approach to the singularity are model independent. When the matter fields are not conformally invariant, the singularity persists if the quantum state is the vacuum near the singularity, and could dissappear for other quantum states. © 1994 The American Physical Society.
format JOUR
author Martin, G.N.
Mazzitelli, F.D.
spellingShingle Martin, G.N.
Mazzitelli, F.D.
Universal approach to cosmological singularities in two-dimensional dilaton gravity
author_facet Martin, G.N.
Mazzitelli, F.D.
author_sort Martin, G.N.
title Universal approach to cosmological singularities in two-dimensional dilaton gravity
title_short Universal approach to cosmological singularities in two-dimensional dilaton gravity
title_full Universal approach to cosmological singularities in two-dimensional dilaton gravity
title_fullStr Universal approach to cosmological singularities in two-dimensional dilaton gravity
title_full_unstemmed Universal approach to cosmological singularities in two-dimensional dilaton gravity
title_sort universal approach to cosmological singularities in two-dimensional dilaton gravity
url http://hdl.handle.net/20.500.12110/paper_05562821_v50_n2_pR613_Martin
work_keys_str_mv AT martingn universalapproachtocosmologicalsingularitiesintwodimensionaldilatongravity
AT mazzitellifd universalapproachtocosmologicalsingularitiesintwodimensionaldilatongravity
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