2022
DOI: 10.1007/s00601-022-01786-6
|View full text |Cite
|
Sign up to set email alerts
|

Relativistic Quantum Dynamics of Scalar Massive Charged Bosons in Topologically Nontrivial Space–Time and AB-Effect

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
1
0

Year Published

2023
2023
2023
2023

Publication Types

Select...
3

Relationship

2
1

Authors

Journals

citations
Cited by 3 publications
(1 citation statement)
references
References 62 publications
0
1
0
Order By: Relevance
“…The quantum dynamics of spin-0 scalar bosons are described by the KG-equation and the spin-half fermions by the Dirac equation. The quantum motions of spin-zero scalar bosons with scalar and vector potential of various kinds and external magnetic and quantum flux fields have been investigated in the background of curved space-times, such as Gödel universe [1], the Som-Raychaudhri space-time [1,2], Ellis-Bronnikov-type wormhole space-time, charged and rotating black hole space-time [3], the Kerr-Newman black holes background [4], topologically trivial space-time [5], and topologically non-trivial space-time [6]. Moreover, the quantum dynamics of spin-half particles have been studied in curved space-time backgrounds as well as in other space-times, such as charged and rotating black hole metric [7], the Kerr spacetime [8], the Kerr-Newman-AdS black hole metric [9], Rindler space-time [10], the Kerr-Newman Space-time [11], and topologically trivial space-time [12] and many more in the literature.…”
Section: Introductionmentioning
confidence: 99%
“…The quantum dynamics of spin-0 scalar bosons are described by the KG-equation and the spin-half fermions by the Dirac equation. The quantum motions of spin-zero scalar bosons with scalar and vector potential of various kinds and external magnetic and quantum flux fields have been investigated in the background of curved space-times, such as Gödel universe [1], the Som-Raychaudhri space-time [1,2], Ellis-Bronnikov-type wormhole space-time, charged and rotating black hole space-time [3], the Kerr-Newman black holes background [4], topologically trivial space-time [5], and topologically non-trivial space-time [6]. Moreover, the quantum dynamics of spin-half particles have been studied in curved space-time backgrounds as well as in other space-times, such as charged and rotating black hole metric [7], the Kerr spacetime [8], the Kerr-Newman-AdS black hole metric [9], Rindler space-time [10], the Kerr-Newman Space-time [11], and topologically trivial space-time [12] and many more in the literature.…”
Section: Introductionmentioning
confidence: 99%