Monitoring the SNS basement neutron background with the MARS detector
Monitoring the SNS basement neutron background with the MARS detector
复制标题
使用 MARS 探测器监测 SNS 基底中子本底
DOI：
10.1088/1748-0221/17/03/p03021
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发表时间：
2022
影响因子：
1.3
通讯作者：
Bolozdynya, A.
中科院分区：
文献类型：
--
作者：
Akimov, D.;An, P.;Awe, C.;Barbeau, P.S.;Becker, B.;Belov, V.;Bernardi, I.;Blackston, M.A.;Bock, C.;Bolozdynya, A.
我们介绍了部署在橡树岭国家实验室散裂中子源（SNS）的火星中子探测器收集的第一个数据集的分析和结果，该数据集用于监测和表征相干协作的束相关中子（BRN）背景。MARS被放置在SNS地下室走廊的COH-CsI相干弹性中微子核散射探测器旁边。这是最接近SNS目标的地下室位置，因此中微子通量最高，但它也被填充混凝土和砾石很好地屏蔽了BRN通量。这些数据显示，探测器每天大约记录一个BRN。利用MARS测量的探测效率，对于中子能量高于~ 3.5 MeV和高达几十MeV的中子，估计入射的BRN通量为1.20±0.56中子/m^ 2/MWh。我们将我们的结果与其他中子探测器报道的SNS地下室走廊的BRN测量结果进行了比较。
We present the analysis and results of the first dataset collected with the MARS neutron detector deployed at the Oak Ridge National Laboratory Spallation Neutron Source (SNS) for the purpose of monitoring and characterizing the beam-related neutron (BRN) background for the COHERENT collaboration. MARS was positioned next to the COH-CsI coherent elastic neutrino-nucleus scattering detector in the SNS basement corridor. This is the basement location of closest proximity to the SNS target and thus, of highest neutrino flux, but it is also well shielded from the BRN flux by infill concrete and gravel. These data show the detector registered roughly one BRN per day. Using MARS'measured detection efficiency, the incoming BRN flux is estimated to be 1.20±0.56 neutrons/m^ 2/MWh for neutron energies above∼ 3.5 MeV and up to a few tens of MeV. We compare our results with previous BRN measurements in the SNS basement corridor reported by other neutron detectors.
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DOI：
--
发表时间：
2018-03
期刊：
arXiv: Instrumentation and Detectors
影响因子：
--
作者：
D. Akimov;J. Albert;Peibo An;C. Awe;P. Barbeau;B. Becker;V. Belov;M. Blackston;A. Bolozdynya;A. Brown;A. Burenkov;B. Cabrera-Palmer;M. Cervantes;J. Collar;R. Cooper;R. Cooper;J. Daughhetee;D. Dean;M. D. V. Coello;J. Detwiler;M. D'Onofrio;Y. Efremenko;S. Elliott;E. Erkela;A. Etenko;L. Fabris;M. Febbraro;N. Fields;W. Fox;A. Galindo-Uribarri;M. Green;M. Heath;S. Hedges;E. Iverson;M. Kaemingk;L. Kaufman;S. Klein;A. Khromov;S. Ki;A. Konovalov;A. Kovalenko;A. Kumpan;L. Li;W. Lu;K. Mann;Y. Melikyan;D. Markoff;H. Moreno;P. Mueller;P. Naumov;J. Newby;D. Parno;S. Penttila;G. Perumpilly;D. Radford;R. Rapp;H. Ray;J. Raybern;D. Reyna;G. Rich;D. Rimal;D. Rudik;D. Salvat;K. Scholberg;B. Scholz;G. Sinev;W. Snow;V. Sosnovtsev;A. Shakirov;B. Suh;R. Tayloe;R. Thornton;I. Tolstukhin;J. Vanderwerp;R. Varner;C. Virtue;J. Yoo;C.-H. Yu;J. Zettlemoyer
通讯作者：
D. Akimov;J. Albert;Peibo An;C. Awe;P. Barbeau;B. Becker;V. Belov;M. Blackston;A. Bolozdynya;A. Brown;A. Burenkov;B. Cabrera-Palmer;M. Cervantes;J. Collar;R. Cooper;R. Cooper;J. Daughhetee;D. Dean;M. D. V. Coello;J. Detwiler;M. D'Onofrio;Y. Efremenko;S. Elliott;E. Erkela;A. Etenko;L. Fabris;M. Febbraro;N. Fields;W. Fox;A. Galindo-Uribarri;M. Green;M. Heath;S. Hedges;E. Iverson;M. Kaemingk;L. Kaufman;S. Klein;A. Khromov;S. Ki;A. Konovalov;A. Kovalenko;A. Kumpan;L. Li;W. Lu;K. Mann;Y. Melikyan;D. Markoff;H. Moreno;P. Mueller;P. Naumov;J. Newby;D. Parno;S. Penttila;G. Perumpilly;D. Radford;R. Rapp;H. Ray;J. Raybern;D. Reyna;G. Rich;D. Rimal;D. Rudik;D. Salvat;K. Scholberg;B. Scholz;G. Sinev;W. Snow;V. Sosnovtsev;A. Shakirov;B. Suh;R. Tayloe;R. Thornton;I. Tolstukhin;J. Vanderwerp;R. Varner;C. Virtue;J. Yoo;C.-H. Yu;J. Zettlemoyer
带有多通道准直器的闪烁相机。
影响因子：
9.3
作者：
H. Anger
通讯作者：
H. Anger
影响因子：
5
作者：
K. Nakamura;K. Hagiwara;K. Hikasa;H. Murayama;M. Tanabashi;T. Watari;C. Amsler;M. Antonelli
通讯作者：
K. Nakamura;K. Hagiwara;K. Hikasa;H. Murayama;M. Tanabashi;T. Watari;C. Amsler;M. Antonelli
DOI：
10.1103/physrevd.102.052007
发表时间：
2019-11
期刊：
arXiv: High Energy Physics - Experiment
影响因子：
--
作者：
C. C. D. Akimov-C.;Peibo An;C. Awe;P. Barbeau;B. Becker;V. Belov;M. Blackston;A. Bolozdynya;B. Cabrera-Palmer;N. Chen;E. Conley;R. Cooper;J. Daughhetee;M. D. V. Coello;J. Detwiler;M. Durand;Y. Efremenko;S. Elliott;L. Fabris;M. Febbraro;W. Fox;A. Galindo-Uribarri;M. Green;K. S. Hansen;M. Heath;S. Hedges;T. Johnson;M. Kaemingk;L. Kaufman;A. Khromov;A. Konovalov;E. Kozlova;A. Kumpan;L. Li;J. Librande;J. Link;J. Liu;K. Mann;D. Markoff;H. Moreno;P. Mueller;J. Newby;D. Parno;S. Penttila;D. Pershey;D. Radford;R. Rapp;H. Ray;J. Raybern;O. Razuvaeva;D. Reyna;G. Rich;D. Rudik;J. Runge;D. Salvat;K. Scholberg;A. Shakirov;G. Simakov;G. Sinev;W. Snow;V. Sosnovtsev;B. Suh;R. Tayloe;K. Tellez-Giron-Flores;R. Thornton;I. Tolstukhin;J. Vanderwerp;R. Varner;C. Virtue;G. Visser;C. Wiseman;T. Wongjirad;J. Yang;Y. Yen;J. Yoo;C.-H. Yu;J. Zettlemoyer
通讯作者：
C. C. D. Akimov-C.;Peibo An;C. Awe;P. Barbeau;B. Becker;V. Belov;M. Blackston;A. Bolozdynya;B. Cabrera-Palmer;N. Chen;E. Conley;R. Cooper;J. Daughhetee;M. D. V. Coello;J. Detwiler;M. Durand;Y. Efremenko;S. Elliott;L. Fabris;M. Febbraro;W. Fox;A. Galindo-Uribarri;M. Green;K. S. Hansen;M. Heath;S. Hedges;T. Johnson;M. Kaemingk;L. Kaufman;A. Khromov;A. Konovalov;E. Kozlova;A. Kumpan;L. Li;J. Librande;J. Link;J. Liu;K. Mann;D. Markoff;H. Moreno;P. Mueller;J. Newby;D. Parno;S. Penttila;D. Pershey;D. Radford;R. Rapp;H. Ray;J. Raybern;O. Razuvaeva;D. Reyna;G. Rich;D. Rudik;J. Runge;D. Salvat;K. Scholberg;A. Shakirov;G. Simakov;G. Sinev;W. Snow;V. Sosnovtsev;B. Suh;R. Tayloe;K. Tellez-Giron-Flores;R. Thornton;I. Tolstukhin;J. Vanderwerp;R. Varner;C. Virtue;G. Visser;C. Wiseman;T. Wongjirad;J. Yang;Y. Yen;J. Yoo;C.-H. Yu;J. Zettlemoyer
DOI：
10.2172/1222694
发表时间：
2015-09
期刊：
arXiv: Instrumentation and Detectors
影响因子：
--
作者：
C. C. D. Akimov-C.;Peibo An;C. Awe;P. Barbeau;P. Barton;B. Becker;V. Belov;A. Bolozdynya;A. Burenkov;B. Cabrera-Palmer;J. Collar;R. Cooper;R. Cooper;C. Cuesta;D. Dean;J. Detwiler;A. Dolgolenko;Y. Efremenko;S. Elliott;A. Etenko;N. Fields;W. Fox;A. Galindo-Uribarri;M. Green;M. Heath;S. Hedges;D. Hornback;E. Iverson;L. Kaufman;S. Klein;A. Khromov;A. Konovalov;A. Kovalenko;A. Kumpan;C. Leadbetter;L. Li;W. Lu;Y. Melikyan;D. Markoff;K. Miller;M. Middlebrook;P. Mueller;P. Naumov;J. Newby;D. Parno;S. Penttila;G. Perumpilly;D. Radford;H. Ray;J. Raybern;D. Reyna;G. Rich;D. Rimal;D. Rudik;K. Scholberg;B. Scholz;W. Snow;A. Sosnovtsev;A. Shakirov;S. Suchyta;B. Suh;R. Tayloe;R. Thornton;A. Tolstukhin;K. Vetter;C. -. Yu
通讯作者：
C. C. D. Akimov-C.;Peibo An;C. Awe;P. Barbeau;P. Barton;B. Becker;V. Belov;A. Bolozdynya;A. Burenkov;B. Cabrera-Palmer;J. Collar;R. Cooper;R. Cooper;C. Cuesta;D. Dean;J. Detwiler;A. Dolgolenko;Y. Efremenko;S. Elliott;A. Etenko;N. Fields;W. Fox;A. Galindo-Uribarri;M. Green;M. Heath;S. Hedges;D. Hornback;E. Iverson;L. Kaufman;S. Klein;A. Khromov;A. Konovalov;A. Kovalenko;A. Kumpan;C. Leadbetter;L. Li;W. Lu;Y. Melikyan;D. Markoff;K. Miller;M. Middlebrook;P. Mueller;P. Naumov;J. Newby;D. Parno;S. Penttila;G. Perumpilly;D. Radford;H. Ray;J. Raybern;D. Reyna;G. Rich;D. Rimal;D. Rudik;K. Scholberg;B. Scholz;W. Snow;A. Sosnovtsev;A. Shakirov;S. Suchyta;B. Suh;R. Tayloe;R. Thornton;A. Tolstukhin;K. Vetter;C. -. Yu