2022
DOI: 10.1103/physrevd.106.105010
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Magnetic flux in the vacuum of quantum bosonic matter in the cosmic string background

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(2 citation statements)
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“…We conclude that relation (17) based on the direct usage of the field solutions (7) is not suitable for the computations of the vacuum polarization outside the impenetrable thin tube (π‘šπ‘Ÿ 0 β‰ͺ 1). In this case, more appropriate, in our opinion, should be the technique of computation with the help of a transformation in the complex plane, when the Bessel functions 𝐽 𝜈 (𝑦) and π‘Œ 𝜈 (𝑦) transform to the modified Bessel 𝐼 𝜈 (𝑦) and Macdonald 𝐾 𝜈 (𝑦) functions, see, e.g., [31].…”
Section: Discussionmentioning
confidence: 99%
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“…We conclude that relation (17) based on the direct usage of the field solutions (7) is not suitable for the computations of the vacuum polarization outside the impenetrable thin tube (π‘šπ‘Ÿ 0 β‰ͺ 1). In this case, more appropriate, in our opinion, should be the technique of computation with the help of a transformation in the complex plane, when the Bessel functions 𝐽 𝜈 (𝑦) and π‘Œ 𝜈 (𝑦) transform to the modified Bessel 𝐼 𝜈 (𝑦) and Macdonald 𝐾 𝜈 (𝑦) functions, see, e.g., [31].…”
Section: Discussionmentioning
confidence: 99%
“…For the induced vacuum energy, the case of the Dirichlet boundary condition was considered in [26][27][28]. For the induced vacuum current and magnetic flux, the case of the Dirichlet boundary condition was considered in [29], the case of the Neumann boundary condition was considered in [30], and the general case for the arbitrary value of the parameter πœƒ was considered in [31].…”
Section: Introductionmentioning
confidence: 99%