Published March 2016 | Version v1
Journal article

Xenon bubble chambers for direct dark matter detection

  • 1. University at Albany, State University of New York, 1400 Washington Ave, Albany, NY 12222 (United States)
  • 2. University of Rochester, Rochester, New York 14627 (United States)
  • 3. Stony Brook University, Stony Brook, NY 11794 (United States)

Description

The search for dark matter is one of today's most exciting fields. As bigger detectors are being built to increase their sensitivity, background reduction is an ever more challenging issue. To this end, a new type of dark matter detector is proposed, a xenon bubble chamber, which would combine the strengths of liquid xenon TPCs, namely event by event energy resolution, with those of a bubble chamber, namely insensitivity to electronic recoils. In addition, it would be the first time ever that a dark matter detector is active on all three detection channels, ionization and scintillation characteristic of xenon detectors, and heat through bubble formation in superheated fluids. Preliminary simulations show that, depending on threshold, a discrimination of 99.99% to 99.9999+% can be achieved, which is on par or better than many current experiments. A prototype is being built at the University at Albany, SUNY. The prototype is currently undergoing seals, thermal, and compression testing

Availability note (English)

Available from http://dx.doi.org/10.1088/1748-0221/11/03/C03003

Additional details

Publishing Information

Journal Title
Journal of Instrumentation
Journal Volume
11
Journal Issue
03
Journal Page Range
p. C03003
ISSN
1748-0221