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Cosmogenic backgrounds to 0 nu beta beta in exo-200

文献类型:期刊论文

作者Albert, J. B.1,2; Auty, D. J.3,27; Barbeau, P. S.4,5; Beck, D.6; Belov, V.7; Breidenbach, M.8; Brunner, T.9,10; Burenkov, A.7; Cao, G. F.11; Chambers, C.12
刊名Journal of cosmology and astroparticle physics
出版日期2016-04-01
期号4页码:29
ISSN号1475-7516
关键词Double beta decay Cosmic ray experiments Neutrino experiments
DOI10.1088/1475-7516/2016/04/029
通讯作者Albert, j. b.(joalbert@indiana.edu)
英文摘要As neutrinoless double-beta decay experiments become more sensitive and intrinsic radioactivity in detector materials is reduced, previously minor contributions to the background must be understood and eliminated. with this in mind, cosmogenic backgrounds have been studied with the exo-200 experiment. using the exo-200 tpc, the muon flux (through a flat horizontal surface) underground at the waste isolation pilot plant (wipp) has been measured to be phi = 4.07 +/- 0.14 (sys) +/- 0.03 (stat) x 10(-7) cm(-2) s(-1), with a vertical intensity of i-v = 2.97(-0.13)(+0.14) (sys) +/- 0.02 (stat) x 10(-7) cm(-2) s(-1) sr(-1). simulations of muon-induced backgrounds identified several potential cosmogenic radionuclides, though only xe-137 is a significant background for the xe-136 0v beta beta search with exo-200. muon-induced neutron backgrounds were measured using gamma-rays from neutron capture on the detector materials. this provided a measurement of xe-137 yield, and a test of the accuracy of the neutron p roduction and transport simulations. the independently measured rates of xe-137 neutron capture and of xe-137 decay agree within uncertainties. geant4 and fluka simulations were performed to estimate neutron capture rates, and these estimates agreed to within similar to 40% or better with measurements. the ability to identify xe-136(n, gamma) events will allow for rejection of xe-137 backgrounds in future 0v beta beta analyses.
WOS关键词NUCLEAR-DATA SHEETS ; ENERGY-LEVELS ; LIGHT-NUCLEI ; SIMULATION ; GEANT4
WOS研究方向Astronomy & Astrophysics ; Physics
WOS类目Astronomy & Astrophysics ; Physics, Particles & Fields
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000393286400003
URI标识http://www.irgrid.ac.cn/handle/1471x/2176844
专题高能物理研究所
通讯作者Albert, J. B.
作者单位1.Indiana Univ, Dept Phys, Bloomington, IN 47405 USA
2.Indiana Univ, CEEM, Bloomington, IN 47405 USA
3.Univ Alabama, Dept Phys & Astron, Tuscaloosa, AL 35487 USA
4.Duke Univ, Dept Phys, Durham, NC 27708 USA
5.Triangle Univ Nucl Lab, Durham, NC 27708 USA
6.Univ Illinois, Dept Phys, 1110 W Green St, Urbana, IL 61801 USA
7.Inst Theoret & Expt Phys, Moscow, Russia
8.SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA
9.McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada
10.TRIUMF, Vancouver, BC V6T 2A3, Canada
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Albert, J. B.,Auty, D. J.,Barbeau, P. S.,et al. Cosmogenic backgrounds to 0 nu beta beta in exo-200[J]. Journal of cosmology and astroparticle physics,2016(4):29.
APA Albert, J. B..,Auty, D. J..,Barbeau, P. S..,Beck, D..,Belov, V..,...&Zeldovich, O. Ya..(2016).Cosmogenic backgrounds to 0 nu beta beta in exo-200.Journal of cosmology and astroparticle physics(4),29.
MLA Albert, J. B.,et al."Cosmogenic backgrounds to 0 nu beta beta in exo-200".Journal of cosmology and astroparticle physics .4(2016):29.

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