New Atomic Methods for Dark Matter Detection

29th International Conference on Photonic, Electronic, and Atomic Collisions

Roberts, B.M.^1 ; Stadnik, Y.V.^1 ; Dzuba, V.A.^2 ; Flambaum, V.V.^1 ; Leefer, N.^2 ; Budker, D.^2,3,4

School of Physics, University of New South Wales, Sydney

2052, Australia^1

Helmholtz Institute Mainz, Johannes Gutenberg University, Mainz

55099, Germany^2

Department of Physics, University of California at Berkeley, Berkeley

CA

94720-7300, United States^3

Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley

CA

94720, United States^4

关键词: Dark energy;    Dark matter;    Dark matter detection;    Time reversal;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/635/2/022033/pdf
DOI  :  10.1088/1742-6596/635/2/022033

来源: IOP

【 摘 要 】

We calculate the parity and time-reversal violating effects that are induced in atoms, nuclei, and molecules by their interaction with various background cosmic fields, such as axion dark matter or dark energy.