| dc.contributor |
Massachusetts Institute of Technology. Department of Physics |
|
| dc.contributor |
Silvestri, Alessandra |
|
| dc.contributor |
Silvestri, Alessandra |
|
| dc.creator |
Silvestri, Alessandra |
|
| dc.date |
2011-10-04T20:47:48Z |
|
| dc.date |
2011-10-04T20:47:48Z |
|
| dc.date |
2011-06 |
|
| dc.date |
2011-03 |
|
| dc.date.accessioned |
2023-03-01T18:05:50Z |
|
| dc.date.available |
2023-03-01T18:05:50Z |
|
| dc.identifier |
0031-9007 |
|
| dc.identifier |
http://hdl.handle.net/1721.1/66181 |
|
| dc.identifier |
Silvestri, Alessandra. “Scalar Radiation from Chameleon-Shielded Regions.” Physical Review Letters 106,251101 (2011): n. pag. © 2011 American Physical Society |
|
| dc.identifier.uri |
http://localhost:8080/xmlui/handle/CUHPOERS/278733 |
|
| dc.description |
I 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. |
|
| dc.description |
National Science Foundation (U.S.) (Grant no. AST-0708501) |
|
| dc.format |
application/pdf |
|
| dc.language |
en_US |
|
| dc.publisher |
American Physical Society |
|
| dc.relation |
http://dx.doi.org/10.1103/PhysRevLett.106.251101 |
|
| dc.relation |
Physical review letters |
|
| dc.rights |
Article 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. |
|
| dc.source |
APS |
|
| dc.title |
Scalar Radiation from Chameleon-Shielded Regions |
|
| dc.type |
Article |
|
| dc.type |
http://purl.org/eprint/type/JournalArticle |
|