Gravitomagnetism in Brane-Worlds
| dc.creator | Nayeri, Ali | |
| dc.creator | Reynolds, Adam | |
| dc.date | 2001-07-23 | |
| dc.date.accessioned | 2026-07-07T04:12:01Z | |
| dc.date.available | 2026-07-07T04:12:01Z | |
| dc.description | In this paper we discuss a physical observable which is drastically different in a brane-world scenario. To date, the Randall-Sundrum model seems to be consistent with all experimental tests of general relativity. Specifically, we examine the so-called gravitomagnetic effect in the context of the Randall-Sundrum (RS) model. This treatment, of course, assumes the recovery of the Kerr metric in brane-worlds which we have found to the first order in the ratio of the brane separation to the radius of the AdS$_5$, $(\ell/r)$. We first show that the second Randall-Sundrum model of one brane leaves the gravitomagnetic effect unchanged. Then, we consider the two-brane scenario of the original Randall-Sundrum proposal and show that the magnitude of the gravitomagnetic effect depends heavily on the ratio of $(\ell/r)$. Such dependence is a result of the geometrodynamic spacetime and does not appear in static scenarios. We hope that we will be able to test this proposal experimentally with data from NASA's Gravity Probe B (GP-B)and possibly disprove either the Randall-Sundrum two-brane scenario or standard general relativity. | |
| dc.description | 5 pages, revtex style | |
| dc.identifier | https://arxiv.org/abs/hep-th/0107201 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0107201 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/50805 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Gravitomagnetism in Brane-Worlds | |
| dc.type | text |