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Is BTZ a separate superselection sector of CTMG?

Deser, S. and Franklin, J. (2010) Is BTZ a separate superselection sector of CTMG? Physics Letters B, 693 (5). pp. 609-611. ISSN 0370-2693. https://resolver.caltech.edu/CaltechAUTHORS:20101209-081925006

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Abstract

We exhibit exact solutions of (positive) matter coupled to original “wrong G-sign” cosmological TMG. They all evolve to conical singularity, rather than to black hole – here negative mass – BTZ. This provides evidence that the latter constitute a separate “superselection” sector, one that unlike in GR, is not reachable by physical sources.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1016/j.physletb.2010.09.019 DOIArticle
https://arxiv.org/abs/1007.2637arXivDiscussion Paper
ORCID:
AuthorORCID
Deser, S.0000-0001-9285-9434
Additional Information:© 2010 Elsevier B.V. Received 15 July 2010; revised 3 September 2010; accepted 8 September 2010. Available online 16 September 2010. Editor: M. Cvetič. S.D. thanks S. Carlip for essential discussions at this project’s inception, and acknowledges support from NSF PHY 07-57190 and DOE DE-FG02-164 92ER40701 grants.
Group:Caltech Theory
Funders:
Funding AgencyGrant Number
NSFPHY 07-57190
Department of Energy (DOE)DE-FG02-16492ER40701
Subject Keywords:BTZ black holes; Topologically massive gravity; D=3 cosmological gravity
Other Numbering System:
Other Numbering System NameOther Numbering System ID
CALT68-2798
BRXTH-623
Issue or Number:5
Record Number:CaltechAUTHORS:20101209-081925006
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20101209-081925006
Official Citation:Deser, S. and J. Franklin (2010). "Is BTZ a separate superselection sector of CTMG?" Physics Letters B 693(5): 609-611.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:21254
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:14 Dec 2010 23:27
Last Modified:03 Oct 2019 02:21

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