Quantum chameleons

被引:22
作者
Brax, Philippe [1 ]
Fichet, Sylvain [2 ,3 ,4 ]
机构
[1] Univ Paris Saclay, Inst Phys Theor, CEA, CNRS, F-91191 Gif Sur Yvette, France
[2] CALTECH, Walter Burke Inst Theoret Phys, Pasadena, CA 91125 USA
[3] ICTP SAIFR, Rua Dr Bento Teobaldo Ferraz 271, Sao Paulo, Brazil
[4] Univ Estadual Paulista, IFT, Rua Dr Bento Teobaldo Ferraz 271, Sao Paulo, Brazil
来源
PHYSICAL REVIEW D | 2019年 / 99卷 / 10期
基金
欧盟地平线“2020”; 巴西圣保罗研究基金会;
关键词
INTERFEROMETRY;
D O I
10.1103/PhysRevD.99.104049
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We initiate a quantum treatment of chameleonlike particles, deriving classical and quantum forces directly from the path integral. It is found that the quantum force can potentially dominate the classical one by many orders of magnitude. We calculate the quantum chameleon pressure between infinite plates, which is found to interpolate between the Casimir and the integrated Casimir-Polder pressures, respectively in the limits of full screening and no screening. To this end we calculate the chameleon propagator in the presence of an arbitrary number of one-dimensional layers of material. For the Eot-Wash experiment, the five-layer propagator is used to take into account the intermediate shielding sheet, and it is found that the presence of the sheet enhances the quantum pressure by two orders of magnitude. As an example of implication, we show that in both the standard chameleon and symmetron models, large and previously unconstrained regions of the parameter space are excluded once the quantum pressure is taken into account.
引用
收藏
页数:12
相关论文
共 45 条
[1]   Particle-physics implications of a recent test of the gravitational inverse-square law [J].
Adelberger, E. G. ;
Heckel, B. R. ;
Hoedl, S. ;
Hoyle, C. D. ;
Kapner, D. J. ;
Upadhye, A. .
PHYSICAL REVIEW LETTERS, 2007, 98 (13)
[2]   Force sensor for chameleon and Casimir force experiments with parallel-plate configuration [J].
Almasi, Attaallah ;
Brax, Philippe ;
Iannuzzi, Davide ;
Sedmik, Rene I. P. .
PHYSICAL REVIEW D, 2015, 91 (10)
[3]  
[Anonymous], About the Press
[4]   A test of general relativity using radio links with the Cassini spacecraft [J].
Bertotti, B ;
Iess, L ;
Tortora, P .
NATURE, 2003, 425 (6956) :374-376
[5]  
Bordag M., 2009, ADV CASIMIR EFFECT, DOI [10.1093/acprof:oso/9780199238743.001.0001/acprof-, DOI 10.1093/ACPROF:OSO/9780199238743.001.0001/ACPROF-]
[6]   Detecting dark energy in orbit: The cosmological chameleon [J].
Brax, P ;
van de Bruck, C ;
Davis, AC ;
Khoury, J ;
Weltman, A .
PHYSICAL REVIEW D, 2004, 70 (12) :18
[7]   Is the radion a chameleon? [J].
Brax, P ;
van de Bruck, C ;
Davis, AC .
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2004, (11) :45-61
[8]   Tuning the Mass of Chameleon Fields in Casimir Force Experiments [J].
Brax, Ph. ;
van de Bruck, C. ;
Davis, A. C. ;
Shaw, D. J. ;
Iannuzzi, D. .
PHYSICAL REVIEW LETTERS, 2010, 104 (24)
[9]   Bounding quantum dark forces [J].
Brax, Philippe ;
Fichet, Sylvain ;
Pignol, Guillaume .
PHYSICAL REVIEW D, 2018, 97 (11)
[10]   Constraining screened fifth forces with the electron magnetic moment [J].
Brax, Philippe ;
Davis, Anne-Christine ;
Elder, Benjamin ;
Wong, Leong Khim .
PHYSICAL REVIEW D, 2018, 97 (08)