Laboratory tests of the Galileon

被引：62

作者：

Brax, Philippe ^{[1
]}

Burrage, Clare ^{[2
,3
]}

Davis, Anne-Christine ^{[4
]}

机构：

[1] CEA, Inst Phys Theor, IPhT, CNRS,URA2306, F-91191 Gif Sur Yvette, France

[2] Univ Geneva, Ctr Astroparticle Phys, CH-1211 Geneva 4, Switzerland

[3] Univ Geneva, Dept Phys Theor, CH-1211 Geneva 4, Switzerland

[4] Ctr Math Sci, Dept Appl Math & Theoret Phys, Cambridge CB3 0WA, England

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2011年 / 09期

关键词：

modified gravity; dark energy experiments; dark energy theory; MASS;

D O I：

10.1088/1475-7516/2011/09/020

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Galileon model is a ghost free scalar effective field theory containing higher derivative terms that are protected by the Galileon symmetry. The presence of a Vainshtein screening mechanism allows the scalar field to couple to matter without mediating unacceptably large fifth forces in the solar system. We describe how laboratory measurements of the Casimir effect and possible deviations from Newtonian gravity can be used to search for Galileon scalar fields. Current experimental measurements are used to bound a previously unconstrained combination of Galileon parameters.

引用

页数：14

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