Internal space structure generalization of the quintom cosmological scenario

We introduce the Lagrangian for a multiscalar-field configuration in an N-dimensional internal space endowed with a constant metric Qik, and generalize the quintom cosmological scenario. We find the energy momentum tensor of the model and show that the set of dual transformations, which preserve the...

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Autores principales: Chimento, L.P., Forte, M., Lazkoz, R., Richarte, M.G.
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_15507998_v79_n4_p_Chimento
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spelling todo:paper_15507998_v79_n4_p_Chimento2023-10-03T16:24:11Z Internal space structure generalization of the quintom cosmological scenario Chimento, L.P. Forte, M. Lazkoz, R. Richarte, M.G. We introduce the Lagrangian for a multiscalar-field configuration in an N-dimensional internal space endowed with a constant metric Qik, and generalize the quintom cosmological scenario. We find the energy momentum tensor of the model and show that the set of dual transformations, which preserve the form of the Einstein equations in the Friedmann-Robertson-Walker cosmology, is enlarged. We show that the stability of the power-law solutions leads to an exponential potential which is invariant under linear transformations in the internal space. Moreover, we obtain the general exact solution of the Einstein-Klein-Gordon equations for that potential. There exist solutions that cross the phantom divide and solutions that blow up at a finite time, exhibiting a superaccelerated behavior and ending in a big rip. We show that the quintom model with a separable potential can be identified with a mixture of several fluids. This framework includes the ΛCDM model, a bouncing model, and a setting sourced by a cosmic string network plus a cosmological constant. Then we concentrate on the case where the dimension of the internal quintessence sector Nq exceeds the dimension of the internal phantom sector Nph. For (Nq,Nph)=(2,1) the dark energy density derived from the 3-scalar field crosses the phantom divide, and its negative component plays the role of the negative part of a classical Dirac field. © 2009 The American Physical Society. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_15507998_v79_n4_p_Chimento
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 introduce the Lagrangian for a multiscalar-field configuration in an N-dimensional internal space endowed with a constant metric Qik, and generalize the quintom cosmological scenario. We find the energy momentum tensor of the model and show that the set of dual transformations, which preserve the form of the Einstein equations in the Friedmann-Robertson-Walker cosmology, is enlarged. We show that the stability of the power-law solutions leads to an exponential potential which is invariant under linear transformations in the internal space. Moreover, we obtain the general exact solution of the Einstein-Klein-Gordon equations for that potential. There exist solutions that cross the phantom divide and solutions that blow up at a finite time, exhibiting a superaccelerated behavior and ending in a big rip. We show that the quintom model with a separable potential can be identified with a mixture of several fluids. This framework includes the ΛCDM model, a bouncing model, and a setting sourced by a cosmic string network plus a cosmological constant. Then we concentrate on the case where the dimension of the internal quintessence sector Nq exceeds the dimension of the internal phantom sector Nph. For (Nq,Nph)=(2,1) the dark energy density derived from the 3-scalar field crosses the phantom divide, and its negative component plays the role of the negative part of a classical Dirac field. © 2009 The American Physical Society.
format JOUR
author Chimento, L.P.
Forte, M.
Lazkoz, R.
Richarte, M.G.
spellingShingle Chimento, L.P.
Forte, M.
Lazkoz, R.
Richarte, M.G.
Internal space structure generalization of the quintom cosmological scenario
author_facet Chimento, L.P.
Forte, M.
Lazkoz, R.
Richarte, M.G.
author_sort Chimento, L.P.
title Internal space structure generalization of the quintom cosmological scenario
title_short Internal space structure generalization of the quintom cosmological scenario
title_full Internal space structure generalization of the quintom cosmological scenario
title_fullStr Internal space structure generalization of the quintom cosmological scenario
title_full_unstemmed Internal space structure generalization of the quintom cosmological scenario
title_sort internal space structure generalization of the quintom cosmological scenario
url http://hdl.handle.net/20.500.12110/paper_15507998_v79_n4_p_Chimento
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AT lazkozr internalspacestructuregeneralizationofthequintomcosmologicalscenario
AT richartemg internalspacestructuregeneralizationofthequintomcosmologicalscenario
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