Asymptotic quasinormal modes of a noncommutative geometry inspired Schwarzschild black hole
| dc.creator | Giri, Pulak Ranjan | |
| dc.date | 2006-04-25 | |
| dc.date | 2007-02-01 | |
| dc.date.accessioned | 2026-07-07T10:25:57Z | |
| dc.date.available | 2026-07-07T10:25:57Z | |
| dc.description | We study the asymptotic quasi-normal modes for the scalar perturbation of the non-commutative geometry inspired Schwarzschild black hole in (3+1) dimensions. We have considered $M\geq M_0$, which effectively correspond to a single horizon Schwarzschild black hole with correction due to non-commutativity. We have shown that for this situation the real part of the asymptotic quasi-normal frequency is proportional to $\ln (3)$. The effect of non-commutativity of spacetime on quasi-normal frequency arises through the constant of proportionality, which is Hawking temperature $T_H(θ)$. We also consider the two horizon case and show that in this case also the real part of the asymptotic quasi-normal frequency is proportional to $\ln(3)$. | |
| dc.description | Accepted in Int. J. Mod. Phys. A | |
| dc.identifier | https://arxiv.org/abs/hep-th/0604188 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0604188 | |
| dc.identifier | Int.J.Mod.Phys.A22:2047-2056,2007 | |
| dc.identifier | doi:10.1142/S0217751X07036245 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/176714 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Asymptotic quasinormal modes of a noncommutative geometry inspired Schwarzschild black hole | |
| dc.type | text |