Monitoring the SNS basement neutron background with the MARS detector

dc.contributor.author

Collaboration, COHERENT

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Akimov, D

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An, P

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Awe, C

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Barbeau, PS

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Becker, B

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Belov, V

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Bernardi, I

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Blackston, MA

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Bock, C

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Bolozdynya, A

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Browning, J

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Cabrera-Palmer, B

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Chernyak, D

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Conley, E

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Daughhetee, J

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Detwiler, J

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Ding, K

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Durand, MR

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Efremenko, Y

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Elliott, SR

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Fabris, L

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Febbraro, M

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Rosso, A Gallo

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Galindo-Uribarri, A

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Green, MP

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Heath, MR

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Hedges, S

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Hoang, D

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Hughes, M

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Johnson, BA

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Johnson, T

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Khromov, A

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Konovalov, A

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Kozlova, E

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Kumpan, A

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Li, L

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Link, JM

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Liu, J

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Mann, K

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Markoff, DM

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Mastroberti, J

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Mueller, PE

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Newby, J

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Parno, DS

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Penttila, SI

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Pershey, D

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Rapp, R

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Ray, H

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Raybern, J

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Razuvaeva, O

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Reyna, D

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Rich, GC

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Ross, J

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Rudik, D

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Runge, J

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Salvat, DJ

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Salyapongse, AM

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Scholberg, K

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Shakirov, A

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Simakov, G

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Sinev, G

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Snow, WM

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Sosnovstsev, V

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Suh, B

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Tayloe, R

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Tellez-Giron-Flores, K

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Tolstukhin, I

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Ujah, E

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Vanderwerp, J

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Varner, RL

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Virtue, CJ

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Visser, G

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Wongjirad, T

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Yen, Y-R

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Yoo, J

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Yu, C-H

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Zettlemoyer, J

dc.date.accessioned

2023-09-07T12:48:00Z

dc.date.available

2023-09-07T12:48:00Z

dc.date.issued

2021-12-05

dc.date.updated

2023-09-07T12:47:59Z

dc.description.abstract

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 $1.20~\pm~0.56~\text{neutrons}/\text{m}^2/\text{MWh}$ for neutron energies above $\sim3.5$ 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.

dc.identifier.uri

https://hdl.handle.net/10161/28977

dc.relation.ispartof

JINST

dc.subject

physics.ins-det

dc.subject

physics.ins-det

dc.subject

hep-ex

dc.title

Monitoring the SNS basement neutron background with the MARS detector

dc.type

Journal article

duke.contributor.orcid

Barbeau, PS|0000-0002-8891-8988

duke.contributor.orcid

Scholberg, K|0000-0002-7007-2021

pubs.begin-page

P03021

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Duke

pubs.organisational-group

Trinity College of Arts & Sciences

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Physics

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Institutes and Provost's Academic Units

pubs.organisational-group

Initiatives

pubs.organisational-group

Duke Science & Society

pubs.volume

17

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