Kavli Institute for Cosmological Physics and Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA.
Phys Rev Lett. 2013 May 24;110(21):211101. doi: 10.1103/PhysRevLett.110.211101. Epub 2013 May 23.
The low-energy monochromatic neutron emission from an (88)Y/Be source can be exploited to mimic the few keV(nr) nuclear recoils expected from low-mass weakly interacting massive particles and coherent scattering of neutrinos off nuclei. Using this source, a </~10% quenching factor is measured for sodium recoils below 24 keV(nr) in NaI[Tl]. This is considerably smaller than the 30% typically adopted in the interpretation of the DAMA/LIBRA dark matter experiment, resulting in a marked increase of its tension with other searches, under the standard set of phenomenological assumptions. The method is illustrated for other target materials (superheated and noble liquids).
(88)Y/Be 源产生的低能单能中子发射可用于模拟低质量弱相互作用大质量粒子和中微子与核的相干散射所预期的几 keV(nr)核反冲。利用这种源,在碘化钠铊(NaI[Tl])中测量到低于 24 keV(nr)的钠反冲的 </~10%淬灭因子。这比 DAMA/LIBRA 暗物质实验解释中通常采用的 30%要小得多,在标准的现象学假设下,这导致其与其他搜索的紧张关系明显增加。该方法还说明了其他靶材料(过冷和惰性液体)的情况。