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dc.date.accessioned 2021-09-08T13:09:23Z
dc.date.available 2021-09-08T13:09:23Z
dc.date.issued 2019
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/124372
dc.description.abstract In a previous paper [Phys. Rev. D 97, 104044 (2018)] we pointed out some shortcomings of the standard approach to chameleon theories consisting in treating the small bodies used to test the weak equivalence principle (WEP) as test particles, whose presence do not modify the chameleon field configuration. In that paper we developed an alternative method to determine the relevant field configuration which takes into account the influence of both test and source bodies, and computed the chamaleon mediated force. Relying on that analysis we showed that the effective acceleration of test bodies is composition dependent even when the model is based on universal couplings. In this paper, we improve our method by using a more suitable approximation for the effective chameleon potential in situations where the bodies are in the so-called "thick shell regime". We then find new and more restrictive bounds on the model' s parametres by confronting the new theoretical predictions with the empirical bounds on Eotvos parameter comming from the lunar laser ranging experiments. en
dc.language en es
dc.subject Acceleration es
dc.subject Field (physics) es
dc.subject Weak equivalence es
dc.subject Shell (structure) es
dc.subject Two-body problem es
dc.subject Laser ranging es
dc.subject Alternative methods es
dc.subject Classical mechanics es
dc.title Thick shell regime in the chameleon two-body problem en
dc.type Articulo es
sedici.identifier.other arXiv:1904.05431 es
sedici.identifier.other doi:10.1103/physrevd.99.083516 es
sedici.identifier.issn 2470-0010 es
sedici.identifier.issn 2470-0029 es
sedici.creator.person Kraiselburd, Lucila es
sedici.creator.person Landau, Susana J. es
sedici.creator.person Salgado, Marcelo es
sedici.creator.person Sudarsky, Daniel es
sedici.creator.person Vucetich, Héctor es
sedici.subject.materias Ciencias Astronómicas es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Preprint es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Physical Review D es
sedici.relation.journalVolumeAndIssue vol. 99, no. 8 es


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