activity
19962026
most citedBig-Bang nucleosynthesis (Particle Data Group mini-review)

4.1k citations · 15.2k across the 123 of their papers we have counts for

collaborators
Showing 2022Show all

10 papers · 1 filter

nucl-ex2022★ 7 cited

Neutrinoless Double Beta Decay

C. Adams, K. Alfonso, C. Andreoiu +229

This White Paper, prepared for the Fundamental Symmetries, Neutrons, and Neutrinos Town Meeting related to the 2023 Nuclear Physics Long Range Plan, makes the case for double beta…

hep-ex2022★ 38 cited

Background Determination for the LUX-ZEPLIN (LZ) Dark Matter Experiment

J. Aalbers, D. S. Akerib, A. K. Al Musalhi +200

The LUX-ZEPLIN experiment recently reported limits on WIMP-nucleus interactions from its initial science run, down to cm for the spin-independent interactio…

physics.ins-det2022★ 26 cited

Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO

G. Gallina, Y. Guan, F. Retiere +162

Liquid xenon time projection chambers are promising detectors to search for neutrinoless double beta decay (0), due to their response uniformity, monolithic sensitive volume,…

hep-ex2022★ 747 cited

First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment

J. Aalbers, D. S. Akerib, C. W. Akerlof +344

The LUX-ZEPLIN experiment is a dark matter detector centered on a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility in Lead, South Dak…

hep-ex2022★ 12 cited

Search for MeV Electron Recoils from Dark Matter in EXO-200

200 Collaboration, S. Al Kharusi, G. Anton +104

We present a search for electron-recoil signatures from the charged-current absorption of fermionic dark matter using the EXO-200 detector. We report an average electron recoil bac…

hep-ex2022★ 2 cited

Snowmass2021 Cosmic Frontier White Paper: Calibrations and backgrounds for dark matter direct detection

Daniel Baxter, Raymond Bunker, Sally Shaw +48

Future dark matter direct detection experiments will reach unprecedented levels of sensitivity. Achieving this sensitivity will require more precise models of signal and background…