Cylindrical boundary induced current in the cosmic string spacetime

Fuente: arXiv
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Autores principales: de Mello, E. R. Bezerra, Mota, H. F. Santana, Santos, W. Oliveira dos
Formato: Preprint
Publicado: 2025
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author de Mello, E. R. Bezerra
Mota, H. F. Santana
Santos, W. Oliveira dos
author_facet de Mello, E. R. Bezerra
Mota, H. F. Santana
Santos, W. Oliveira dos
contents In this paper we investigate the vacuum current associated with a charged bosonic field operator, induced by a cylindrical boundary in the idealized cosmic string spacetime. In this setup we assume that the cylindrical boundary is coaxial with the string, that by its turn carry a magnetic flux along its core. In order to develop this analysis, we calculate the positive frequency Wightman functions for both regions, inside and outside the boundary. Moreover, we assume that the bosonic field obeys the Robin boundary condition on the cylindrical shell. Using this approach, the analytical expressions for the vacuum bosonic currents are presented in the form of the sum of boundary-free and boundary-induced parts. Because the boundary-free contribution is very well established in literature, our focus here is in the boundary-dependent part. As we will see, our general results are presented in a cylindrically symmetric static structure. Some asymptotic behaviors for the boundary-induced vacuum currents are investigated in various limiting cases. In order to provide a better understanding of these currents, we provide some graphs exhibiting their behavior as function of the distance to the string's core, and on the intensity of the magnetic flux running along it. These plots also present how the parameter associated with the planar angle deficit interfere in the intensity of the corresponding current.
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id arxiv_https___arxiv_org_abs_2503_24281
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Cylindrical boundary induced current in the cosmic string spacetime
de Mello, E. R. Bezerra
Mota, H. F. Santana
Santos, W. Oliveira dos
High Energy Physics - Theory
General Relativity and Quantum Cosmology
In this paper we investigate the vacuum current associated with a charged bosonic field operator, induced by a cylindrical boundary in the idealized cosmic string spacetime. In this setup we assume that the cylindrical boundary is coaxial with the string, that by its turn carry a magnetic flux along its core. In order to develop this analysis, we calculate the positive frequency Wightman functions for both regions, inside and outside the boundary. Moreover, we assume that the bosonic field obeys the Robin boundary condition on the cylindrical shell. Using this approach, the analytical expressions for the vacuum bosonic currents are presented in the form of the sum of boundary-free and boundary-induced parts. Because the boundary-free contribution is very well established in literature, our focus here is in the boundary-dependent part. As we will see, our general results are presented in a cylindrically symmetric static structure. Some asymptotic behaviors for the boundary-induced vacuum currents are investigated in various limiting cases. In order to provide a better understanding of these currents, we provide some graphs exhibiting their behavior as function of the distance to the string's core, and on the intensity of the magnetic flux running along it. These plots also present how the parameter associated with the planar angle deficit interfere in the intensity of the corresponding current.
title Cylindrical boundary induced current in the cosmic string spacetime
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2503.24281