Thermal flow in the gravitational O(n) model
| dc.creator | Kostov, Ivan K. | |
| dc.date | 2006-02-07 | |
| dc.date | 2006-02-16 | |
| dc.date.accessioned | 2026-07-07T07:02:51Z | |
| dc.date.available | 2026-07-07T07:02:51Z | |
| dc.description | We study the massless flow from the critical point (dilute loops) to the low-temperature phase (dense loops) of the O(n) loop gas model when the model is coupled to 2D gravity. The flow is generated by the gravitationally dressed thermal operator Φ_{1,3} coupled to the renormalized loop tension λ~ T-T_c. We find that the susceptibility as a function of the thermal coupling λand the cosmological constant μsatisfies a simple transcendental equation. | |
| dc.description | 14 pages, 2 figures; contribution to QTS-4, Varna, Bulgaria | |
| dc.identifier | https://arxiv.org/abs/hep-th/0602075 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0602075 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/108755 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Thermal flow in the gravitational O(n) model | |
| dc.type | text |