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Measurement of the ionization yield of nuclear recoils in liquid argon at 80 and 233 keV
The energy calibration of nuclear recoil detectors is of primary importance
to rare-event experiments such as those of direct dark matter search and
coherent neutrino-nucleus scattering. In particular, such a calibration is
performed by measuring the ionization yield of nuclear recoils in liquid Ar and
Xe detection media, using neutron elastic scattering off nuclei. In the present
work, the ionization yield for nuclear recoils in liquid Ar has for the first
time been measured in the higher energy range, at 80 and 233 keV, using a
two-phase Cryogenic Avalanche Detector (CRAD) and DD neutron generator. The
ionization yield in liquid Ar at an electric field of 2.3 kV/cm amounted to
7.8+/-1.1 and 9.7+/-1.3 e-/keV at 80 and 233 keV respectively. The Jaffe model
for nuclear recoil-induced ionization, in contrast to that Thomas-Imel, can
probably consistently describe the energy dependence of the ionization yield.Comment: 6 pages, 6 figures. Fig. 6 changed. Submitted to EP
The first light of Mini-MegaTORTORA wide-field monitoring system
Here we describe the first light of the novel 9-channel wide-field optical
monitoring system with sub-second temporal resolution, Mini-MegaTORTORA, which
is being tested now at Special Astrophysical Observatory on Russian Caucasus.
The system is able to observe the sky simultaneously in either wide (~900
square degrees) or narrow (~100 square degrees) fields of view, either in clear
light or with any combination of color (Johnson B, V or R) polarimetric filters
installed, with exposure times ranging from 100 ms to 100 s. The primary goal
of the system is the detection of rapid -- with sub-second characteristic
time-scales -- optical transients, but it may be also used for studying the
variability of the sky objects on longer time scales.Comment: 9 pages, 9 figures, based on the talk presented on "Modern stellar
astronomy-2014" (Rostov-on-Don
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