6533b7d6fe1ef96bd1265d99
RESEARCH PRODUCT
Limiting P-odd interactions of cosmic fields with electrons, protons and neutrons
V. A. DzubaVictor V. FlambaumYevgeny V. StadnikBenjamin RobertsNathan LeeferDmitry Budkersubject
PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)ProtonNuclear TheoryAtomic Physics (physics.atom-ph)Dark matterNuclear TheoryGeneral Physics and AstronomyFOS: Physical sciencesElectronSpace Physics (physics.space-ph)Physics - Atomic PhysicsNuclear physicsPseudoscalarNuclear Theory (nucl-th)DipoleHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Physics - Space PhysicsNeutronPseudovectorAstrophysics - Cosmology and Nongalactic Astrophysicsdescription
We propose methods for extracting limits on the strength of P-odd interactions of pseudoscalar and pseudovector cosmic fields with electrons, protons and neutrons. Candidates for such fields are dark matter (including axions) and dark energy, as well as several more exotic sources described by standard-model extensions. Calculations of parity nonconserving amplitudes and atomic electric dipole moments induced by these fields are performed for H, Li, Na, K, Rb, Cs, Ba+, Tl, Dy, Fr, and Ra+. From these calculations and existing measurements in Dy, Cs and Tl, we constrain the interaction strengths of the parity-violating static pseudovector cosmic field to be 7*10^(-15) GeV with an electron, and 3*10^(-8) GeV with a proton.
year | journal | country | edition | language |
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2014-04-10 |