2015
DOI: 10.1103/physrevd.91.035007
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Dark forces and atomic electric dipole moments

Abstract: Postulating the existence of a finite-mass mediator of T,P-odd coupling between atomic electrons and nucleons we consider its effect on permanent electric dipole moment (EDM) of diamagnetic atoms. We present both numerical and analytical analysis for such mediator-induced EDMs and compare it with EDM results for the conventional contact interaction. Based on this analysis we derive limits on coupling strengths and carrier masses from experimental limits on EDM of 199 Hg atom.

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Cited by 12 publications
(25 citation statements)
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References 25 publications
(39 reference statements)
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“…However, we present them again here to highlight the reasons for which differences between the RPA and CCSD results occur. This could justify the intention for calculating the C χ T coupling coefficients due to the exchange of dark matter candidate χ using the CCSD method, which were determined earlier by the RPA method [36]. It is worth mentioning here that our DHF and RPA results given in the above table agree well with another calculation reported in Ref.…”
Section: Resultssupporting
confidence: 87%
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“…However, we present them again here to highlight the reasons for which differences between the RPA and CCSD results occur. This could justify the intention for calculating the C χ T coupling coefficients due to the exchange of dark matter candidate χ using the CCSD method, which were determined earlier by the RPA method [36]. It is worth mentioning here that our DHF and RPA results given in the above table agree well with another calculation reported in Ref.…”
Section: Resultssupporting
confidence: 87%
“…in fm-3 Distance, r in fm For m χ =∞ For m χ =1000 MeV/c2 For m χ =100 MeV/c 2 For m χ =50 MeV/c (Color online) Behavior of ρ χ N values with the distance from the origin of the nucleus of 199 Hg in the uniform charge distribution for different values of mχ (in MeV/c 2 . This is perfectly in agreement with the findings of Ref [36]…”
supporting
confidence: 94%
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“…It would be interesting to explore deviations from the contact limit in this lower mass regime (see e.g. [24]). However, once the relevant mass scale becomes too small, (100 keV and smaller), typically, very strong astrophysical bounds on portal couplings can be imposed, leaving little scope for interesting sensitivity via EDM observables.…”
Section: Discussionmentioning
confidence: 99%