Abstract

In this work, using two scalar fields (ϕ, ψ) coupled to 4 + 1 dimensional gravity, we construct novel topological brane solutions through an explicit U(1) symmetry breaking term. The potential of this model is constructed so that two distinct degenerate vacua in the ϕ field exist, in analogy to the ϕ4 potential. Therefore, brane solutions appear due to the vacuum structure of the ϕ field. However, the topology and vacuum structure in the ψ direction depends on the symmetry breaking parameter β2, which leads to different types of branes. As a result, one can interpret the present model as a combination of a ϕ4 brane with an auxiliary field, which leads to deviations from the ϕ4 system with the brane achieving a richer internal structure. Furthermore, we analyse in detail the behaviour of the superpotentials, the warp factors, the Ricci and Kretschmann scalars and the Einstein tensor components. In addition to this, we explore the stability of the brane in terms of the free parameters of the model. The analysis presented here complements previous work and is sufficiently novel to be interesting.

Details

Title
Novel thick brane solutions with U(1) symmetry breaking
Author
Peyravi Marzieh 1   VIAFID ORCID Logo  ; Riazi Nematollah 2 ; Lobo Francisco S N 3   VIAFID ORCID Logo 

 Ferdowsi University of Mashhad, Department of Physics, School of Sciences, Mashhad, Iran (GRID:grid.411301.6) (ISNI:0000 0001 0666 1211) 
 Shahid Beheshti University, Physics Department, Tehran, Iran (GRID:grid.412502.0) (ISNI:0000 0001 0686 4748) 
 Faculdade de Ciências da Universidade de Lisboa, Instituto de Astrofísica e Ciências do Espaço, Lisbon, Portugal (GRID:grid.9983.b) (ISNI:0000 0001 2181 4263) 
Publication year
2021
Publication date
Mar 2021
Publisher
Springer Nature B.V.
ISSN
14346044
e-ISSN
14346052
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2496965594
Copyright
© The Author(s) 2021. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.