6533b7dafe1ef96bd126ed92

RESEARCH PRODUCT

Search for the effect of massive bodies on atomic spectra and constraints on Yukawa-type interactions of scalar particles

Yevgeny V. StadnikNathan LeeferDmitry BudkerDmitry BudkerDmitry BudkerAndreas GerhardusVictor V. FlambaumVictor V. Flambaum

subject

Particle physicsGeneral PhysicsPhotonAtomic Physics (physics.atom-ph)General Physics and Astronomychemistry.chemical_elementFOS: Physical sciencesElectron01 natural sciencesphysics.atom-phMathematical SciencesPhysics - Atomic PhysicsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)EngineeringHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsSpectroscopyPhysics010308 nuclear & particles physicshep-exScalar (physics)Yukawa potentialhep-phHigh Energy Physics - PhenomenologychemistryPhysical SciencesDysprosiumNucleonScalar field

description

We propose a new method to search for hypothetical scalar particles that have feeble interactions with Standard-Model particles. In the presence of massive bodies, these interactions produce a non-zero Yukawa-type scalar-field magnitude. Using radio-frequency spectroscopy data of atomic dysprosium, as well as atomic clock spectroscopy data, we constrain the Yukawa-type interactions of a scalar field with the photon, electron, and nucleons for a range of scalar-particle masses corresponding to length scales $ > 10$ cm. In the limit as the scalar-particle mass $m_\phi \to 0$, our derived limits on the Yukawa-type interaction parameters are: $\Lambda_\gamma \gtrsim 8 \times 10^{19}$ GeV, $\Lambda_e \gtrsim 1.3 \times 10^{19}$ GeV, and $\Lambda_N \gtrsim 6 \times 10^{20}$ GeV. Our measurements also constrain combinations of interaction parameters, which cannot otherwise be probed with traditional anomalous-force measurements. We suggest further measurements to improve on the current level of sensitivity.

10.1103/physrevlett.117.271601http://arxiv.org/abs/1607.04956