Jump to content

RST model

From Wikipedia, the free encyclopedia
This is an old revision of this page, as edited by Raidr (talk | contribs) at 10:01, 20 January 2011 (A first draft). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.
(diff) ← Previous revision | Latest revision (diff) | Newer revision → (diff)

The Russo-Susskind-Thorlacius model[1] or RST model in short is a modification of the CGHS model to take care of conformal anomalies. 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 or not ghosts are considered. The nonlocal term leads to nonlocality.

References

  1. ^ Russo, Jorge; Susskind, Leonard; Thorlacius, Lárus (15 Oct 1992). "The Endpoint of Hawking Evaporation". Physical Review. D. 46 (8): 3444–3449. doi:10.1103/PhysRevD.46.3444. Archived from the original on 17 June 1992.{{cite journal}}: CS1 maint: multiple names: authors list (link)

Template:Relativity stub