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most citedResults from the Final Exposure of the CDMS II Experiment

814 citations · 7.6k across the 74 of their papers we have counts for

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hep-ex2023★ 56 cited

A search for new physics in low-energy electron recoils from the first LZ exposure

The LZ Collaboration, J. Aalbers, D. S. Akerib +200

The LUX-ZEPLIN (LZ) experiment is a dark matter detector centered on a dual-phase xenon time projection chamber. We report searches for new physics appearing through few-keV-scale…

hep-ex2023★ 34 cited

A Search for Low-mass Dark Matter via Bremsstrahlung Radiation and the Migdal Effect in SuperCDMS

M. F. Albakry, I. Alkhatib, D. Alonso +130

We present a new analysis of previously published of SuperCDMS data using a profile likelihood framework to search for sub-GeV dark matter (DM) particles through two inelastic scat…

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…

hep-ex2022★ 2 cited

Supporting Capabilities For Underground Facilities

Alvine Kamaha, Brianna Mount, Richard Schnee

The 2021 particle physics community study, known as "Snowmass 2021", has brought together particle physicists around the world to create a unified vision for the field over the nex…

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★ 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…