Induced fermionic current in AdS spacetime in the presence of a cosmic string and a compactified dimension

Abstract In this paper, we consider a massive charged fermionic quantum field and investigate the current densities induced by a magnetic flux running along the core of an idealized cosmic string in the background geometry of a 5-dimensional anti-de Sitter spacetime, assuming that an extra dimension...

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Main Authors: S. Bellucci, W. Oliveira dos Santos, E. R. Bezerra de Mello
Format: Article
Language:English
Published: SpringerOpen 2020-10-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-020-08505-7
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spelling doaj-8e896d9febac43528aa5dddd1fe976d22020-11-25T03:40:44ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522020-10-01801011410.1140/epjc/s10052-020-08505-7Induced fermionic current in AdS spacetime in the presence of a cosmic string and a compactified dimensionS. Bellucci0W. Oliveira dos Santos1E. R. Bezerra de Mello2INFN, Laboratori Nazionali di FrascatiINFN, Laboratori Nazionali di FrascatiDepartamento de Física, Universidade Federal da ParaíbaAbstract In this paper, we consider a massive charged fermionic quantum field and investigate the current densities induced by a magnetic flux running along the core of an idealized cosmic string in the background geometry of a 5-dimensional anti-de Sitter spacetime, assuming that an extra dimension is compactified. Along the compact dimension quasi-periodicity condition is imposed on the field with a general phase. Moreover, we admit the presence of a magnetic flux enclosed by the compactified axis. The latter gives rise to Ahanorov–Bohm-like effect on the vacuum expectation value of the currents. In this setup, only azimuthal and axial current densities take place. The former presents two contributions, with the first one due to the cosmic string in a 5-dimensional AdS spacetime without compact dimension, and the second one being induced by the compactification itself. The latter is an odd function of the magnetic flux along the cosmic string and an even function of the magnetic flux enclosed by the compactified axis with period equal to the quantum flux. As to the induced axial current, it is an even function of the magnetic flux along the string’s core and an odd function of the magnetic flux enclosed by the compactification perimeter. For untwisted and twisted field along compact dimension, the axial current vanishes. The massless field case is presented as well some asymptotic limits for the parameters of the model.http://link.springer.com/article/10.1140/epjc/s10052-020-08505-7
collection DOAJ
language English
format Article
sources DOAJ
author S. Bellucci
W. Oliveira dos Santos
E. R. Bezerra de Mello
spellingShingle S. Bellucci
W. Oliveira dos Santos
E. R. Bezerra de Mello
Induced fermionic current in AdS spacetime in the presence of a cosmic string and a compactified dimension
European Physical Journal C: Particles and Fields
author_facet S. Bellucci
W. Oliveira dos Santos
E. R. Bezerra de Mello
author_sort S. Bellucci
title Induced fermionic current in AdS spacetime in the presence of a cosmic string and a compactified dimension
title_short Induced fermionic current in AdS spacetime in the presence of a cosmic string and a compactified dimension
title_full Induced fermionic current in AdS spacetime in the presence of a cosmic string and a compactified dimension
title_fullStr Induced fermionic current in AdS spacetime in the presence of a cosmic string and a compactified dimension
title_full_unstemmed Induced fermionic current in AdS spacetime in the presence of a cosmic string and a compactified dimension
title_sort induced fermionic current in ads spacetime in the presence of a cosmic string and a compactified dimension
publisher SpringerOpen
series European Physical Journal C: Particles and Fields
issn 1434-6044
1434-6052
publishDate 2020-10-01
description Abstract In this paper, we consider a massive charged fermionic quantum field and investigate the current densities induced by a magnetic flux running along the core of an idealized cosmic string in the background geometry of a 5-dimensional anti-de Sitter spacetime, assuming that an extra dimension is compactified. Along the compact dimension quasi-periodicity condition is imposed on the field with a general phase. Moreover, we admit the presence of a magnetic flux enclosed by the compactified axis. The latter gives rise to Ahanorov–Bohm-like effect on the vacuum expectation value of the currents. In this setup, only azimuthal and axial current densities take place. The former presents two contributions, with the first one due to the cosmic string in a 5-dimensional AdS spacetime without compact dimension, and the second one being induced by the compactification itself. The latter is an odd function of the magnetic flux along the cosmic string and an even function of the magnetic flux enclosed by the compactified axis with period equal to the quantum flux. As to the induced axial current, it is an even function of the magnetic flux along the string’s core and an odd function of the magnetic flux enclosed by the compactification perimeter. For untwisted and twisted field along compact dimension, the axial current vanishes. The massless field case is presented as well some asymptotic limits for the parameters of the model.
url http://link.springer.com/article/10.1140/epjc/s10052-020-08505-7
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