Time Variation of the Fine Structure Constant in the Spacetime of a Domain Wall
| dc.creator | Campanelli, L. | |
| dc.creator | Cea, P. | |
| dc.creator | Tedesco, L. | |
| dc.date | 2005-10-29 | |
| dc.date | 2007-03-01 | |
| dc.date.accessioned | 2026-07-07T10:27:41Z | |
| dc.date.available | 2026-07-07T10:27:41Z | |
| dc.description | The gravitational field produced by a domain wall acts as a medium with spacetime-dependent permittivity ε. Therefore, the fine structure constant α= e^2/4 πεwill be a time-dependent function at fixed position. The most stringent constraint on the time-variation of αcomes from the natural reactor Oklo and gives |\dotα/α| < few 10^{-17} yr^{-1}. This limit constrains the tension of a cosmic domain wall to be less than σ\lesssim 10^{-2} MeV^3, and then represents the most severe limit on the energy density of a cosmic wall stretching our Universe. | |
| dc.description | New version, accepted for publication in MPLA | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0510825 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0510825 | |
| dc.identifier | Mod.Phys.Lett.A22:1013-1018,2007 | |
| dc.identifier | doi:10.1142/S0217732307023006 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/177223 | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Time Variation of the Fine Structure Constant in the Spacetime of a Domain Wall | |
| dc.type | text |