2012
DOI: 10.1103/physrevd.85.045016
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Fermionic Casimir densities in a conical space with a circular boundary and magnetic flux

Abstract: The vacuum expectation value (VEV) of the energy-momentum tensor for a massive fermionic field is investigated in a (2 þ 1)-dimensional conical spacetime in the presence of a circular boundary and an infinitely thin magnetic flux located at the cone apex. The MIT bag boundary condition is assumed on the circle. At the cone apex we consider a special case of boundary conditions for irregular modes, when the MIT bag boundary condition is imposed at a finite radius, which is then taken to zero. The presence of th… Show more

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Cited by 24 publications
(14 citation statements)
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“…where the parameterα is given in terms of the linear mass density of the cosmic string µ byα = 1 − 4µ/c 2 , which is smaller than the unity. Moreover, the metric in (11) is locally flat, but globally it is not [23,24] and through the metric (11), among others effects [25][26][27][28][29], we can study the gravitational analog of the Aharonov-Bohm effect [30][31][32]. It is known that the curvature tensor of the metric (10), when considered as a distribution, is of the form [33]…”
Section: Motion In a Aharonov-bohm Potentialmentioning
confidence: 99%
See 1 more Smart Citation
“…where the parameterα is given in terms of the linear mass density of the cosmic string µ byα = 1 − 4µ/c 2 , which is smaller than the unity. Moreover, the metric in (11) is locally flat, but globally it is not [23,24] and through the metric (11), among others effects [25][26][27][28][29], we can study the gravitational analog of the Aharonov-Bohm effect [30][31][32]. It is known that the curvature tensor of the metric (10), when considered as a distribution, is of the form [33]…”
Section: Motion In a Aharonov-bohm Potentialmentioning
confidence: 99%
“…Thus, Eq. (27) implies that the only allowable value for the angular momentum is m+φ, meaning that we have a single bound state. In other words, when the δ -function potential is repulsive (α < 1) an attractive effective potential potential assures one bound state (m + φ = 0).…”
Section: Quantum Dynamics On An Anti-conementioning
confidence: 99%
“…A cosmic string and topological defect relationship is studied where the topological defects are located at arbitrary positions on the graphene plane [5]. In line with the efforts to combine general relativity theory with quantum mechanics, these studies are of great interest [6][7][8]. Cosmic strings were introduced by Kibble in 1976 [9], and the geometry of the massless cosmic strings is examined in the large scale limit of the model given in [10].…”
Section: Introductionmentioning
confidence: 99%
“…For 0 r  the geometry (2) is flat and the curvature tensor has delta type singularity at 0 r  for 0 0   . In(1) the22  Dirac matrices are given in polar coordinates ( , ).…”
mentioning
confidence: 99%