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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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 |
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Phantom domain |
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Phantom domain Avelino, P. P. Ferreira, V. M. C. Silva, Josinaldo Menezes da Sousa, L. Phantom domain walls |
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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 |
_version_ |
1773963414789423104 |