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Newtonian counterparts of spin 2 massless discontinuities

Deser, S. and Tekin, B. (2001) Newtonian counterparts of spin 2 massless discontinuities. Classical and Quantum Gravity, 18 (23). L171-L174. ISSN 0264-9381. https://resolver.caltech.edu/CaltechAUTHORS:20170524-132447595

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Abstract

Massive spin 2 theories in flat or cosmological (Λ≠0) backgrounds are subject to discontinuities as the masses tend to zero. We show and explain physically why their Newtonian limits do not inherit this behaviour. On the other hand, conventional 'Newtonian cosmology', where Λ is a constant source of the potential, displays discontinuities: e.g. for any finite range, Λ can be totally removed.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1088/0264-9381/18/23/103DOIArticle
http://iopscience.iop.org/article/10.1088/0264-9381/18/23/103/metaPublisherArticle
https://arxiv.org/abs/gr-qc/0109091arXivDiscussion Paper
ORCID:
AuthorORCID
Deser, S.0000-0001-9285-9434
Additional Information:© 2001 IOP Publishing Ltd. Received 28 September 2001; Published 21 November 2001. We thank A Waldron and the authors of [13] for stimulating correspondence. This work was supported by the National Science Foundation grant PHY99-73935.
Funders:
Funding AgencyGrant Number
NSFPHY99-73935
Issue or Number:23
Classification Code:PACS number: 1880
Record Number:CaltechAUTHORS:20170524-132447595
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170524-132447595
Official Citation:S Deser and B Tekin 2001 Class. Quantum Grav. 18 L171
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:77718
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:24 May 2017 21:14
Last Modified:03 Oct 2019 18:00

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