Volume 74, Number 6, June 2006
|Page(s)||978 - 984|
|Section||The physics of elementary particles and fields|
|Published online||26 May 2006|
Gravitoelectromagnetically induced transitions in charged boson nebulae
Department of Solid State and Theoretical Physics, Faculty of Physics “Al. I. Cuza” University - Bd. Carol I no. 11, 700506 Iaşi, Romania
Corresponding author: email@example.com
Accepted: 26 April 2006
We derive approximating analytical solutions to the system of Klein-Gordon-Maxwell-Einstein equations, describing a minimally coupled charged boson to a spherically symmetric spacetime. Within a first-order perturbative approach, we generalize some previous results and write down the effective potential and the current, for the non-vanishing radial-momentum case. These can be actually employed in computing quantum transitions, such as the ones related to gravitoelectric particle creation. It can be noticed that the non-vanishing radial wave number affects both the effective potential, by a gravity-based dipole contribution, and the current. These lead to serious consequences regarding the actual dispersion, the continuity equation and the growth, and respectively decay, of the quantum mode-excitations.
PACS: 11.27.+d – Extended classical solutions; cosmic strings, domain walls, texture / 04.40.Nr – Einstein-Maxwell spacetimes, spacetimes with fluids, radiation or classical fields / 04.20.Jb – Exact solutions
© EDP Sciences, 2006
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