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Hauptverfasser: Lima, F. C. E., Belchior, F. M., Almeida, C. A. S., Sahoo, P. K.
Format: Preprint
Veröffentlicht: 2024
Schlagworte:
Online-Zugang:https://arxiv.org/abs/2407.14693
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author Lima, F. C. E.
Belchior, F. M.
Almeida, C. A. S.
Sahoo, P. K.
author_facet Lima, F. C. E.
Belchior, F. M.
Almeida, C. A. S.
Sahoo, P. K.
contents Revisiting Einstein's gravitational theory, we build a five-dimensional braneworld. Within this framework, one announces the appearance of symmetric and asymmetric domain walls. Furthermore, it examines the emergent four-dimensional gravity from a theory with non-canonical dynamics. Exploring the physical and mathematical aspects, e.g., brane's energy density and the Kaluza-Klein (KK) spectrum, one verifies that brane splitting is absent in the canonical and non-canonical theories. Additionally, we note the localization of the four-dimensional fluctuation projection on the 3-branes, which ensures the theory's stability. Thereby, one can conclude that the behavior of gravitational perturbations of the domain wall maintains a profile similar to a stable and non-localizable tower of massive modes. In contrast, within the brane core, the matter sector generates new barriers and potential wells, resulting in massive modes with approximately symmetric amplitudes. However, the non-canonical dynamics generate massive modes with asymmetric amplitudes far from the 3-brane.
format Preprint
id arxiv_https___arxiv_org_abs_2407_14693
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle On the asymmetric non-canonical braneworld in five dimensions
Lima, F. C. E.
Belchior, F. M.
Almeida, C. A. S.
Sahoo, P. K.
General Relativity and Quantum Cosmology
Revisiting Einstein's gravitational theory, we build a five-dimensional braneworld. Within this framework, one announces the appearance of symmetric and asymmetric domain walls. Furthermore, it examines the emergent four-dimensional gravity from a theory with non-canonical dynamics. Exploring the physical and mathematical aspects, e.g., brane's energy density and the Kaluza-Klein (KK) spectrum, one verifies that brane splitting is absent in the canonical and non-canonical theories. Additionally, we note the localization of the four-dimensional fluctuation projection on the 3-branes, which ensures the theory's stability. Thereby, one can conclude that the behavior of gravitational perturbations of the domain wall maintains a profile similar to a stable and non-localizable tower of massive modes. In contrast, within the brane core, the matter sector generates new barriers and potential wells, resulting in massive modes with approximately symmetric amplitudes. However, the non-canonical dynamics generate massive modes with asymmetric amplitudes far from the 3-brane.
title On the asymmetric non-canonical braneworld in five dimensions
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2407.14693