Black holes and non-relativistic quantum systems
| dc.creator | Kovtun, Pavel | |
| dc.creator | Nickel, Dominik | |
| dc.date | 2008-09-11 | |
| dc.date | 2008-09-22 | |
| dc.date.accessioned | 2026-07-07T12:44:47Z | |
| dc.date.available | 2026-07-07T12:44:47Z | |
| dc.description | We describe black holes in d+3 dimensions, whose thermodynamic properties correspond to those of a scale invariant non-relativistic d+1 dimensional quantum system with dynamical exponent z=2. The gravitational model involves a massive abelian vector field and a scalar field, in addition to the metric. The energy per particle in the dual theory is $|μ| d/(d+2)$, exactly as in a non-interacting Fermi gas, while the ratio of shear viscosity to entropy density is $\hbar/4π$. | |
| dc.description | 8 pages; v2: discussion modified | |
| dc.identifier | https://arxiv.org/abs/0809.2020 | |
| dc.identifier | http://arxiv.org/abs/0809.2020 | |
| dc.identifier | Phys.Rev.Lett.102:011602,2009 | |
| dc.identifier | doi:10.1103/PhysRevLett.102.011602 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/220892 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Black holes and non-relativistic quantum systems | |
| dc.type | text |