Phantom domain walls

We consider a model with two real scalar fields which admits phantom domain wall solutions. We investigate the structure and evolution of these phantom domain walls in an expanding homogeneous and isotropic universe. In particular, we show that the increase of the tension of the domain walls with co...

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Principais autores: Avelino, P. P., Ferreira, V. M. C., Silva, Josinaldo Menezes da, Sousa, L.
Formato: article
Idioma:English
Publicado em: American Physical Society
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Endereço do item:https://repositorio.ufrn.br/jspui/handle/123456789/29871
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spelling ri-123456789-298712020-08-23T07:25:32Z Phantom domain walls Avelino, P. P. Ferreira, V. M. C. Silva, Josinaldo Menezes da Sousa, L. Phantom domain We consider a model with two real scalar fields which admits phantom domain wall solutions. We investigate the structure and evolution of these phantom domain walls in an expanding homogeneous and isotropic universe. In particular, we show that the increase of the tension of the domain walls with cosmic time, associated to the evolution of the phantom scalar field, is responsible for an additional damping term in their equations of motion. We describe the macroscopic dynamics of phantom domain walls, showing that extended phantom defects whose tension varies on a cosmological time scale cannot be the dark energy 2020-08-20T14:33:20Z 2020-08-20T14:33:20Z 2017 article AVELINO, P. P.; FERREIRA, V. M. C.; MENEZES, J.; SOUSA, L.. Phantom domain walls. Physical Review D, [S.L.], v. 96, n. 4, p. 043506, 9 ago. 2017. Disponível em: https://journals.aps.org/prd/abstract/10.1103/PhysRevD.96.043506. Acesso em: 03 ago. 2020. http://dx.doi.org/10.1103/physrevd.96.043506. 2470-0010 https://repositorio.ufrn.br/jspui/handle/123456789/29871 10.1103/physrevd.96.043506. en application/pdf American Physical Society
institution Repositório Institucional
collection RI - UFRN
language English
topic Phantom domain
spellingShingle Phantom domain
Avelino, P. P.
Ferreira, V. M. C.
Silva, Josinaldo Menezes da
Sousa, L.
Phantom domain walls
description We consider a model with two real scalar fields which admits phantom domain wall solutions. We investigate the structure and evolution of these phantom domain walls in an expanding homogeneous and isotropic universe. In particular, we show that the increase of the tension of the domain walls with cosmic time, associated to the evolution of the phantom scalar field, is responsible for an additional damping term in their equations of motion. We describe the macroscopic dynamics of phantom domain walls, showing that extended phantom defects whose tension varies on a cosmological time scale cannot be the dark energy
format article
author Avelino, P. P.
Ferreira, V. M. C.
Silva, Josinaldo Menezes da
Sousa, L.
author_facet Avelino, P. P.
Ferreira, V. M. C.
Silva, Josinaldo Menezes da
Sousa, L.
author_sort Avelino, P. P.
title Phantom domain walls
title_short Phantom domain walls
title_full Phantom domain walls
title_fullStr Phantom domain walls
title_full_unstemmed Phantom domain walls
title_sort phantom domain walls
publisher American Physical Society
publishDate 2020
url https://repositorio.ufrn.br/jspui/handle/123456789/29871
work_keys_str_mv AT avelinopp phantomdomainwalls
AT ferreiravmc phantomdomainwalls
AT silvajosinaldomenezesda phantomdomainwalls
AT sousal phantomdomainwalls
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