A longitudinal component in massive gravitational waves arising from a bimetric theory of gravity
| dc.creator | Corda, Christian | |
| dc.date | 2008-11-06 | |
| dc.date.accessioned | 2026-07-07T11:56:21Z | |
| dc.date.available | 2026-07-07T11:56:21Z | |
| dc.description | After a brief review of the work of de Paula, Miranda and Marinho on massive gravitational waves arising from a bimetric theory of gravity, in this paper it is shown that the presence of the mass generates a longi- tudinal component in a particular polarization of the wave. The effect of this polarization on test masses is performed using the geodesic deviation. A the end of this paper the detectability of this particular polarization is also discussed, showing that its angular dependence could, in princi- ple, discriminate such polarization with respect the two ones of general relativity, if present or future detectors will achieve a high sensitivity. | |
| dc.description | Published in Astroparticle Physics | |
| dc.identifier | https://arxiv.org/abs/0811.0985 | |
| dc.identifier | http://arxiv.org/abs/0811.0985 | |
| dc.identifier | Astropart.Phys.28:247-250,2007 | |
| dc.identifier | doi:10.1016/j.astropartphys.2007.05.009 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/205557 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | A longitudinal component in massive gravitational waves arising from a bimetric theory of gravity | |
| dc.type | text |