Testing Lorentz symmetry with planetary orbital dynamics

被引：53

作者：

Hees, A. ^{[1
]}

Bailey, Q. G. ^{[2
]}

Le Poncin-Lafitte, C. ^{[3
]}

Bourgoin, A. ^{[3
]}

Rivoldini, A. ^{[4
]}

Lamine, B. ^{[5
]}

Meynadier, F. ^{[3
]}

Guerlin, C. ^{[3
,6
]}

Wolf, P. ^{[3
]}

机构：

[1] Rhodes Univ, Dept Math, ZA-6140 Grahamstown, South Africa

[2] Embry Riddle Aeronaut Univ, Dept Phys, Prescott, AZ 86301 USA

[3] Univ Paris 06, Sorbonne Univ, PSL Res Univ, SYRTE,Observ Paris,CNRS,LNE, F-75014 Paris, France

[4] Royal Observ Belgium, B-1180 Brussels, Belgium

[5] Univ Toulouse, CNRS, UPS OMP, IRAP, F-31028 Toulouse, France

[6] UPMC, Univ Paris 04, ENS PSL Res Univ, Lab Kastler Brossel,CNRS,Coll France, F-75005 Paris, France

来源：

PHYSICAL REVIEW D | 2015年 / 92卷 / 06期

关键词：

GENERAL-RELATIVITY; DARK-MATTER; EPHEMERIDES; CONSTRAINTS; EPM;

D O I：

10.1103/PhysRevD.92.064049

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Planetary ephemerides are a very powerful tool to constrain deviations from the theory of general relativity (GR) using orbital dynamics. The effective field theory framework called the Standard-Model Extension (SME) has been developed in order to systematically parametrize hypothetical violations of Lorentz symmetry (in the Standard Model and in the gravitational sector). In this communication, we use the latest determinations of the supplementary advances of the perihelia and of the nodes obtained by planetary ephemerides analysis to constrain SME coefficients from the pure gravity sector and also from gravity-matter couplings. Our results do not show any deviation from GR and they improve current constraints. Moreover, combinations with existing constraints from Lunar Laser Ranging and from atom interferometry gravimetry allow us to disentangle contributions from the pure gravity sector from the gravity-matter couplings.

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页数：12

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