activity
20092026
most citedResults from a search for dark matter in the complete LUX exposure

1.6k citations · 4.4k across the 48 of their papers we have counts for

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Showing 2011Show all

7 papers · 1 filter

physics.ins-det2011★ 6 cited

Further Developments in Gold-stud Bump Bonding

C. Neher, R. L. Lander, A. Moskaleva +3

As silicon detectors in high energy physics experiments require increasingly complex assembly procedures, the availability of a wide variety of interconnect technologies provides m…

physics.ins-det2011

Development of Readout Interconnections for the Si-W Calorimeter of SiD

M. Woods, R. G. Fields, B. Holbrook +15

The SiD collaboration is developing a Si-W sampling electromagnetic calorimeter, with anticipated application for the International Linear Collider. Assembling the modules for such…

physics.data-an2011★ 38 cited

LUXSim: A Component-Centric Approach to Low-Background Simulations

D. S. Akerib, X. Bai, S. Bedikian +60

Geant4 has been used throughout the nuclear and high-energy physics community to simulate energy depositions in various detectors and materials. These simulations have mostly been…

hep-ex2011★ 76 cited

The 2010 Interim Report of the Long-Baseline Neutrino Experiment Collaboration Physics Working Groups

The LBNE Collaboration, T. Akiri, D. Allspach +329

In early 2010, the Long-Baseline Neutrino Experiment (LBNE) science collaboration initiated a study to investigate the physics potential of the experiment with a broad set of diffe…

physics.ins-det2011★ 6 cited

Study of wavelength-shifting chemicals for use in large-scale water Cherenkov detectors

M. Sweany, A. Bernstein, S. Dazeley +4

Cherenkov detectors employ various methods to maximize light collection at the photomultiplier tubes (PMTs). These generally involve the use of highly reflective materials lining t…

astro-ph.IM2011★ 58 cited

After LUX: The LZ Program

D. C. Malling, D. S. Akerib, H. M. Araujo +71

The LZ program consists of two stages of direct dark matter searches using liquid Xe detectors. The first stage will be a 1.5-3 tonne detector, while the last stage will be a 20 to…