New Limits on Bosonic Dark Matter, Solar Axions, Pauli Exclusion Principle Violation, and Electron Decay from the Majorana Demonstrator

(Majorana Collaboration)

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Abstract

We present new limits on exotic keV-scale physics based on 478 kg d of Majorana Demonstrator commissioning data. Constraints at the 90% confidence level are derived on bosonic dark matter (DM) and solar axion couplings, Pauli exclusion principle violating (PEPV) decay, and electron decay using monoenergetic peak signal limits above our background. Our most stringent DM constraints are set for 11.8 keV mass particles, limiting gAe<4.5×10-13 for pseudoscalars and (α′/α)<9.7×10-28 for vectors. We also report a 14.4 keV solar axion coupling limit of gANeff×gAe<3.8×10-17, a 12β2<8.5×10-48 limit on the strength of PEPV electron transitions, and a lower limit on the electron lifetime of τe>1.2×1024 yr for e-→ invisible.

Original languageEnglish
Article number161801
JournalPhysical Review Letters
Volume118
Issue number16
DOIs
StatePublished - Apr 21 2017

Funding

This material is based upon work supported by the U.S. Department of Energy (DOE), Office of Science, Office of Nuclear Physics under Awards No.DE-AC02-05CH11231, No.DE-AC52-06NA25396, No.DE-FG02-97ER41041, No.DE-FG02-97ER41033, No.DE-FG02-97ER41042, No.DE-SC0012612, No.DE-FG02-10ER41715, No.DE-SC0010254, and No.DE-FG02-97ER41020. We acknowledge support from the Particle Astrophysics Program and Nuclear Physics Program of the National Science Foundation through Grants No.PHY-0919270, No.PHY-1003940, No.0855314, No.PHY-1202950, No.MRI 0923142, and No.1003399. We acknowledge support from the Russian Foundation for Basic Research, Grant No.15-02-02919. We acknowledge the support of the U.S. Department of Energy through the Los Alamos National Lab (LANL)/ Laboratory Directed Research and Development (LDRD) Program. This research used resources of the Oak Ridge Leadership Computing Facility, which is a DOE Office of Science User Facility supported under Contract No.DE-AC05-00OR22725. This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported under Contract No.DE-AC02-05CH11231. We thank our hosts and colleagues at the Sanford Underground Research Facility for their support.

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