Gravitomagnetism in superconductors and compact stars
| dc.creator | Bambi, Cosimo | |
| dc.date | 2007-10-10 | |
| dc.date.accessioned | 2026-07-07T11:37:58Z | |
| dc.date.available | 2026-07-07T11:37:58Z | |
| dc.description | There are three experimentally observed effects in rotating superconductors that are so far unexplained. Some authors have tried to interpret such a phenomena as possible new gravitational properties of coherent quantum systems: in particular, they suggest that the gravitomagnetic field of that kind of matter may be many orders of magnitude stronger than the one expected in the standard theory. Here I show that this interpretation would be in conflict with the common belief that neutron stars have neutrons in superfluid state and protons in superconductive one. | |
| dc.description | 9 pages, no figure | |
| dc.identifier | https://arxiv.org/abs/0710.2042 | |
| dc.identifier | http://arxiv.org/abs/0710.2042 | |
| dc.identifier | Int.J.Mod.Phys.D17:327-336,2008 | |
| dc.identifier | doi:10.1142/S0218271808012036 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/199399 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Gravitomagnetism in superconductors and compact stars | |
| dc.type | text |