Jump to content

RST model

From Wikipedia, the free encyclopedia
This is an old revision of this page, as edited by Mazdatribute (talk | contribs) at 16:48, 23 January 2021 (The main goal of the RST model is described to take care of conformal anomalies. More importantly, the modification of RST wrt CGHS is that the model becomes analytically solvable.). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

The Russo–Susskind–Thorlacius model[1] or RST model in short is a modification of the CGHS model to take care of conformal anomalies and render it analytically soluble. In the CGHS model, if we include Faddeev-Popov ghosts to gauge-fix diffeomorphisms in the conformal gauge, they contribute an anomaly of -24. Each matter field contributes an anomaly of 1. So, unless N=24, we will have gravitational anomalies. To the CGHS action

, the following term

is added, where κ is either or depending upon whether ghosts are considered. The nonlocal term leads to nonlocality. In the conformal gauge,

.

It might appear as if the theory is local in the conformal gauge, but this overlooks the fact that the Raychaudhuri equations are still nonlocal.

References

  1. ^ Russo, Jorge; Susskind, Leonard; Thorlacius, Lárus (15 Oct 1992). "The Endpoint of Hawking Evaporation". Physical Review. D. 46 (8): 3444–3449. arXiv:hep-th/9206070. Bibcode:1992PhRvD..46.3444R. doi:10.1103/PhysRevD.46.3444. PMID 10015289.