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dc.contributor.authorSilvestri, Alessandra
dc.date.accessioned2011-10-04T20:47:48Z
dc.date.available2011-10-04T20:47:48Z
dc.date.issued2011-06
dc.date.submitted2011-03
dc.identifier.issn0031-9007
dc.identifier.urihttp://hdl.handle.net/1721.1/66181
dc.description.abstractI study the profile of the chameleon field around a radially pulsating mass. Focusing on the case in which the background (static) chameleon profile exhibits a thin shell, I add small perturbations to the source in the form of time-dependent radial pulsations. It is found that the chameleon field inherits a time dependence and there is a resultant scalar radiation from the region of the source. This has several interesting and potentially testable consequences.en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant no. AST-0708501)en_US
dc.language.isoen_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevLett.106.251101en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceAPSen_US
dc.titleScalar Radiation from Chameleon-Shielded Regionsen_US
dc.typeArticleen_US
dc.identifier.citationSilvestri, Alessandra. “Scalar Radiation from Chameleon-Shielded Regions.” Physical Review Letters 106,251101 (2011): n. pag. © 2011 American Physical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.approverSilvestri, Alessandra
dc.contributor.mitauthorSilvestri, Alessandra
dc.relation.journalPhysical review lettersen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsSilvestri, Alessandraen
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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