Charged scalar bosons in a Bonnor-Melvin- universe at conical approximation
arXiv:2405.09471 · doi:10.1140/epjc/s10052-024-12911-6
Abstract
The quantum dynamics of charged scalar bosons in a Bonnor-Melvin- universe is considered. In this study, the behavior of charged scalar bosons is explored within the framework of the Duffin-Kemmer-Petiau (DKP) formalism. Adopting a conical approximation (), we are considered two scenarios for the vector potential: a linear and quadratic vector potentials. In particular, the effects of this background in the equation of motion, phase shift, -matrix, energy spectrum and DKP spinor are analyzed and discussed.
arXiv comment11 pages, 5 figures
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Cited by in corpus (5)
- On the Klein-Gordon bosonic fields in the Bonnor-Melvin spacetime with a cosmological constant in rainbow gravity: Bonnor-Melvin Domain Walls
- Comment on "Neutrino interaction with matter in a noninertial frame"
- Properties of the magnetic universe with positive cosmological constant
- Scalar and vector bosons in a Bonnor-Melvin- spacetime: an exact Duffin-Kemmer-Petiau analysis
- Bound-state solutions for the charged Dirac oscillator in a rotating frame in the Bonnor-Melvin-Lambda spacetime