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4 results on '"Collar JI"'

1. Observation of coherent elastic neutrino-nucleus scattering

Author

Akimov, D, Albert, JB, An, P, Awe, C, Barbeau, PS, Becker, B, Belov, V, Brown, A, Bolozdynya, A, Cabrera-Palmer, B, Cervantes, M, Collar, JI, Cooper, RJ, Cooper, RL, Cuesta, C, Dean, DJ, Detwiler, JA, Eberhardt, A, Efremenko, Y, Elliott, SR, Erkela, EM, Fabris, L, Febbraro, M, Fields, NE, Fox, W, Fu, Z, Galindo-Uribarri, A, Green, MP, Hai, M, Heath, MR, Hedges, S, Hornback, D, Hossbach, TW, Iverson, EB, Kaufman, LJ, Ki, S, Klein, SR, Khromov, A, Konovalov, A, Kremer, M, Kumpan, A, Leadbetter, C, Li, L, Lu, W, Mann, K, Markoff, DM, Miller, K, Moreno, H, Mueller, PE, Newby, J, Orrell, JL, Overman, CT, Parno, DS, Penttila, S, Perumpilly, G, Ray, H, Raybern, J, Reyna, D, Rich, GC, Rimal, D, Rudik, D, Scholberg, K, Scholz, BJ, Sinev, G, Snow, WM, Sosnovtsev, V, Shakirov, A, Suchyta, S, Suh, B, Tayloe, R, Thornton, RT, Tolstukhin, I, and Vanderwerp, J

Subjects
Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Experiment
Abstract

© 2017, American Association for the Advancement of Science. All rights reserved. The coherent elastic scattering of neutrinos off nuclei has eluded detection for four decades, even though its predicted cross section is by far the largest of all low-energy neutrino couplings. This mode of interaction offers new opportunities to study neutrino properties and leads to a miniaturization of detector size, with potential technological applications. We observed this process at a 6.7s confidence level, using a low-background, 14.6-kilogram CsI[Na] scintillator exposed to the neutrino emissions from the Spallation Neutron Source at Oak Ridge National Laboratory. Characteristic signatures in energy and time, predicted by the standard model for this process, were observed in high signal-to-background conditions. Improved constraints on nonstandard neutrino interactions with quarks are derived from this initial data set.

Published
2017
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2. Observation of coherent elastic neutrino-nucleus scattering

Author

Akimov, D, Albert, JB, An, P, Awe, C, Barbeau, PS, Becker, B, Belov, V, Brown, A, Bolozdynya, A, Cabrera-Palmer, B, Cervantes, M, Collar, JI, Cooper, RJ, Cooper, RL, Cuesta, C, Dean, DJ, Detwiler, JA, Eberhardt, A, Efremenko, Y, Elliott, SR, Erkela, EM, Fabris, L, Febbraro, M, Fields, NE, Fox, W, Fu, Z, Galindo-Uribarri, A, Green, MP, Hai, M, Heath, MR, Hedges, S, Hornback, D, Hossbach, TW, Iverson, EB, Kaufman, LJ, Ki, S, Klein, SR, Khromov, A, Konovalov, A, Kremer, M, Kumpan, A, Leadbetter, C, Li, L, Lu, W, Mann, K, Markoff, DM, Miller, K, Moreno, H, Mueller, PE, Newby, J, Orrell, JL, Overman, CT, Parno, DS, Penttila, S, Perumpilly, G, Ray, H, Raybern, J, Reyna, D, Rich, GC, Rimal, D, Rudik, D, Scholberg, K, Scholz, BJ, Sinev, G, Snow, WM, Sosnovtsev, V, Shakirov, A, Suchyta, S, Suh, B, Tayloe, R, Thornton, RT, Tolstukhin, I, Vanderwerp, J, Varner, RL, Virtue, CJ, Wan, Z, Yoo, J, Yu, C-H, Zawada, A, Zettlemoyer, J, Zderic, AM, and COHERENT Collaboration

Subjects
nucl-th, Physics::Instrumentation and Detectors, hep-ex, General Science & Technology, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Experiment, hep-ph, COHERENT Collaboration, nucl-ex
Abstract

The coherent elastic scattering of neutrinos off nuclei has eluded detection for four decades, even though its predicted cross section is by far the largest of all low-energy neutrino couplings. This mode of interaction offers new opportunities to study neutrino properties and leads to a miniaturization of detector size, with potential technological applications. We observed this process at a 6.7σ confidence level, using a low-background, 14.6-kilogram CsI[Na] scintillator exposed to the neutrino emissions from the Spallation Neutron Source at Oak Ridge National Laboratory. Characteristic signatures in energy and time, predicted by the standard model for this process, were observed in high signal-to-background conditions. Improved constraints on nonstandard neutrino interactions with quarks are derived from this initial data set.

Published
2017

3. The Intermediate Neutrino Program

Author

Adams, C, Alonso, JR, Ankowski, AM, Asaadi, JA, Ashenfelter, J, Axani, SN, Babu, K, Backhouse, C, Band, HR, Barbeau, PS, Barros, N, Bernstein, A, Betancourt, M, Bishai, M, Blucher, E, Bouffard, J, Bowden, N, Brice, S, Bryan, C, Camilleri, L, Cao, J, Carlson, J, Carr, RE, Chatterjee, A, Chen, M, Chen, S, Chiu, M, Church, ED, Collar, JI, Collin, G, Conrad, JM, Convery, MR, Cooper, RL, Cowen, D, Davoudiasl, H, Gouvea, A De, Dean, DJ, Deichert, G, Descamps, F, DeYoung, T, Diwan, MV, Djurcic, Z, Dolinski, MJ, Dolph, J, Donnelly, B, Dwyer, DA, Dytman, S, Efremenko, Y, Everett, LL, Fava, A, Figueroa-Feliciano, E, Fleming, B, Friedland, A, Fujikawa, BK, Gaisser, TK, Galeazzi, M, Galehouse, DC, Galindo-Uribarri, A, Garvey, GT, Gautam, S, Gilje, KE, Gonzalez-Garcia, M, Goodman, MC, Gordon, H, Gramellini, E, Green, MP, Guglielmi, A, Hackenburg, RW, Hackenburg, A, Halzen, F, Han, K, Hans, S, Harris, D, Heeger, KM, Herman, M, Hill, R, Holin, A, Huber, P, Jaffe, DE, Johnson, RA, Joshi, J, Karagiorgi, G, Kaufman, LJ, Kayser, B, Kettell, SH, Kirby, BJ, Klein, JR, Kolomensky, Yu G, Kriske, RM, Lane, CE, Langford, TJ, Lankford, A, Lau, K, Learned, JG, Ling, J, Link, JM, Lissauer, D, Littenberg, L, Littlejohn, BR, and Lockwitz, S

Subjects
Physics::Instrumentation and Detectors, hep-ex, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, High Energy Physics::Experiment, nucl-ex, physics.ins-det
Abstract

The US neutrino community gathered at the Workshop on the Intermediate Neutrino Program (WINP) at Brookhaven National Laboratory February 4-6, 2015 to explore opportunities in neutrino physics over the next five to ten years. Scientists from particle, astroparticle and nuclear physics participated in the workshop. The workshop examined promising opportunities for neutrino physics in the intermediate term, including possible new small to mid-scale experiments, US contributions to large experiments, upgrades to existing experiments, R&D plans and theory. The workshop was organized into two sets of parallel working group sessions, divided by physics topics and technology. Physics working groups covered topics on Sterile Neutrinos, Neutrino Mixing, Neutrino Interactions, Neutrino Properties and Astrophysical Neutrinos. Technology sessions were organized into Theory, Short-Baseline Accelerator Neutrinos, Reactor Neutrinos, Detector R&D and Source, Cyclotron and Meson Decay at Rest sessions.This report summarizes discussion and conclusions from the workshop.

Published
2015

4. Depth Requirements for a Tonne-scale 76Ge Neutrinoless Double-beta Decay Experiment

Author

Collaboration, The MAJORANA, Aguayo, E, III, FT Avignone, Back, HO, Barabash, AS, Bergevin, M, Bertrand, FE, Boswell, M, Brudanin, V, Busch, M, Chan, Y-D, Christofferson, CD, Collar, JI, Combs, DC, Cooper, RJ, Detwiler, JA, Doe, PJ, Efremenko, Yu, Egorov, V, Ejiri, H, Elliott, SR, Esterline, J, Fast, JE, Fields, N, Finnerty, P, Fraenkle, FM, Gehman, VM, Giovanetti, GK, Green, MP, Guiseppe, VE, Gusey, K, Hallin, AL, Hazama, R, Henning, R, Hime, A, Hoppe, EW, Horton, M, Howard, S, Howe, MA, Johnson, RA, Keeter, KJ, Keillor, ME, Keller, C, Kephart, JD, Kidd, MF, Knecht, A, Kochetov, O, Konovalov, SI, Kouzes, RT, LaFerriere, BD, LaRoque, BH, Leon, J, Leviner, LE, Loach, JC, MacMullin, S, Marino, MG, Martin, RD, Mei, D-M, Merriman, JH, Miller, ML, Mizouni, L, Nomachi, M, Orrell, JL, Overman, NR, II, DG Phillips, Poon, AWP, Perumpilly, G, Prior, G, Radford, DC, Rielage, K, Robertson, RGH, Ronquest, MC, Schubert, AG, Shima, T, Shirchenko, M, Snavely, KJ, Sobolev, V, Steele, D, Strain, J, Thomas, K, Timkin, V, Tornow, W, Vanyushin, I, Varner, RL, Vetter, K, Vorren, K, Wilkerson, JF, Wolfe, BA, Yakushev, E, Young, AR, Yu, C-H, Yumatov, V, and Zhang, C

Subjects
Physics::Instrumentation and Detectors, FOS: Physical sciences, Nuclear Experiment (nucl-ex), nucl-ex, Nuclear Experiment
Abstract

Neutrinoless double-beta decay experiments can potentially determine the Majorana or Dirac nature of the neutrino, and aid in understanding the neutrino absolute mass scale and hierarchy. Future 76Ge-based searches target a half-life sensitivity of >10^27 y to explore the inverted neutrino mass hierarchy. Reaching this sensitivity will require a background rate of ~5200 mwe is required for a tonne-scale experiment with a compact shield similar to the planned 40-kg MAJORANA DEMONSTRATOR. The required overburden is highly dependent on the chosen shielding configuration and could be relaxed significantly if, for example, a liquid cryogen and water shield, or an active neutron shield were employed. Operation of the MAJORANA DEMONSTRATOR and GERDA detectors will serve to reduce the uncertainties on cosmic-ray background rates and will impact the choice of shielding style and location for a future tonne-scale experiment. 4/2013: The peer review process revealed that one of the veto rejection factors (the factor-of-4 described on p12) needs to be better established. Our reevaluation of this parameter to date has not yielded strong support for the value stated in the manuscript, and we require further study to develop a solid estimate. This further study will supersede the work described in this manuscript, and may or may not lead to the same conclusion regarding the ~>5200 mwe requirement for future tonne-scale 76Ge neutrinoless double beta decay experiments., Corresponding author: J. Detwiler (jasondet@uw.edu), 25 pages, 2 figures

Published
2011
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