LUX/LZ Dark Matter
Experiment & Neutron Calibration
Author: Madan K. Sharma
Timalsina
The LUX Dark Matter Experiment has performed the most sensitive
direct search for weakly-interacting massive dark matter particles
(so-called WIMPs). The successor experiment LZ will also be located underground
at SURF (Sanford Underground Research Facility) in Lead/SD. The LZ central
detector will not only be an order of magnitude larger than
the existing LUX inner detector, but its sensitivity for direct dark matter
searches will be 100 times better than LUX. If WIMPs exist, they could
interact in the cryogenic liquid xenon of the detector's core by bouncing into
a xenon nucleus, which will then recoil and produce scintillation light
and electric charge. The ratio of the directly
detected scintillation light and the delayed charge detection is
characteristic of such a nuclear recoil, and differs
significantly from an electron recoil produced
by undesired background reactions. However, the precise
knowledge of the critical ratio value, for which the electron recoil-dominated regime transitions into the nuclear recoil dominated regime, is
key.
Dedicated neutron calibration sources, such as DD-generator guns, AmLi and AmBe
neutron sources, and a new mono-energetic Y/Be neutron source, are
essential tools for precisely mapping the nuclear recoil region. That way, it can be
demonstrated what a possible WIMP detection would look like in the LUX/LZ
detectors.
The precise neutron fluxes of the various neutron calibration sources
have to be measured before the actual deployments of the sources are
performed, to assess the detection efficiency in the detector.
A new neutron monitor system, utilizing He-3 proportional counter tubes, is
being developed within the framework of the LUX/LZ project.