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20002025
most citedResults from the Final Exposure of the CDMS II Experiment

814 citations · 7.5k across the 78 of their papers we have counts for

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Showing 2022Show all

13 papers · 1 filter

hep-ph2022★ 34 cited

Report of the Topical Group on Particle Dark Matter for Snowmass 2021

Jodi Cooley, Tongyan Lin, W. Hugh Lippincott +71

This report summarizes the findings of the CF1 Topical Subgroup to Snowmass 2021, which was focused on particle dark matter. One of the most important scientific goals of the next…

physics.ins-det2022★ 30 cited

A Stress Induced Source of Phonon Bursts and Quasiparticle Poisoning

Robin Anthony-Petersen, Andreas Biekert, Raymond Bunker +43

The performance of superconducting qubits is degraded by a poorly characterized set of energy sources breaking the Cooper pairs responsible for superconductivity, creating a condit…

physics.ins-det2022★ 1 cited

Exploration of Methods to Remove Implanted Pb and Po Contamination from Silicon Surfaces

Isaac J. Arnquist, Raymond Bunker, Zdenek Dohnalek +2

Radioactive contaminants on the surfaces of detector components can be a problematic source of background events for physics experiments searching for rare processes. Exposure to r…

astro-ph.CO2022★ 4 cited

Effective Field Theory Analysis of CDMSlite Run 2 Data

SuperCDMS Collaboration, M. F. Albakry, I. Alkhatib +127

CDMSlite Run 2 was a search for weakly interacting massive particles (WIMPs) with a cryogenic 600 g Ge detector operated in a high-voltage mode to optimize sensitivity to WIMPs of…

physics.ins-det2022★ 8 cited

The level-1 trigger for the SuperCDMS experiment at SNOLAB

Jonathan S. Wilson, Hanno Meyer zu Theenhausen, Belina von Krosigk +15

The SuperCDMS SNOLAB dark matter search experiment aims to be sensitive to energy depositions down to O(1 eV). This imposes requirements on the resolution, signal efficiency, and n…

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…