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Searching for solar KDAR with DUNE
The observation of 236 MeV muon neutrinos from kaon-decay-at-rest (KDAR) originating in the core of the Sun would provide a unique signature of dark matter annihilation. Since excellent angle and energy reconstruction are necessary to detect this monoenergetic, directional neutrino flux, DUNE with i...
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Published in: | arXiv.org 2021-10 |
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creator | Acciarri, R Back, A Baldi, P Bazo Alba, J L C Benitez Montiel Berger, J Braga, D Brunetti, G Chatterjee, A Cherdack, D Chi, C Chisnall, G Choubey, S Clarke, P Conley, E Corwin, L Dawson, J Dias, M Diwan, M Duarte, L Duffy, K Flight, R Franco, D Gabrielli, A Gandrajula, R Gastler, D Gomes, R A Gran, R Green, P Groh, M Grudzinski, J Hamacher-Baumann, P Hertel, L Hill, T Holin, A Hourlier, A Hristova, I James, E Jediny, F Jung, C K F Kashur, L Koerner, L W Kumar, P Lang, K Larkin, J Lazanu, I L Li Loew, T Madera, A Manenti, L Marchan, M Marfatia, D Martinez Caicedo, D A Menary, S Meyer, H Molina, J Moon, J Morris, C W Mu Muir, A Musser, J Nandakumar, R Nesbit, J Nishimura, K Oberling, M Onishchuk, Y Paudel, A Perry, J Pessina, G Petti, R Poppi, F Rademacker, J Real, J S Rigaut, Y Rossella, M Rott, C Savage, G Sgalaberna, D Sinev, G Sobel, H Soto-Oton, J Spitz, J Strauss, T Surdo, A Susic, V Szczerbinska, B B Tapia Oregui Tatar, E Thorn, C Toups, M Tsverava, N Valdiviesso, G A Vergani, S Wallbank, M Wascko, M O Wei, H J Yu Zito, M Zucchelli, S |
description | The observation of 236 MeV muon neutrinos from kaon-decay-at-rest (KDAR) originating in the core of the Sun would provide a unique signature of dark matter annihilation. Since excellent angle and energy reconstruction are necessary to detect this monoenergetic, directional neutrino flux, DUNE with its vast volume and reconstruction capabilities, is a promising candidate for a KDAR neutrino search. In this work, we evaluate the proposed KDAR neutrino search strategies by realistically modeling both neutrino-nucleus interactions and the response of DUNE. We find that, although reconstruction of the neutrino energy and direction is difficult with current techniques in the relevant energy range, the superb energy resolution, angular resolution, and particle identification offered by DUNE can still permit great signal/background discrimination. Moreover, there are non-standard scenarios in which searches at DUNE for KDAR in the Sun can probe dark matter interactions. |
doi_str_mv | 10.48550/arxiv.2107.09109 |
format | article |
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Since excellent angle and energy reconstruction are necessary to detect this monoenergetic, directional neutrino flux, DUNE with its vast volume and reconstruction capabilities, is a promising candidate for a KDAR neutrino search. In this work, we evaluate the proposed KDAR neutrino search strategies by realistically modeling both neutrino-nucleus interactions and the response of DUNE. We find that, although reconstruction of the neutrino energy and direction is difficult with current techniques in the relevant energy range, the superb energy resolution, angular resolution, and particle identification offered by DUNE can still permit great signal/background discrimination. 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DUNE</title><title>arXiv.org</title><description>The observation of 236 MeV muon neutrinos from kaon-decay-at-rest (KDAR) originating in the core of the Sun would provide a unique signature of dark matter annihilation. Since excellent angle and energy reconstruction are necessary to detect this monoenergetic, directional neutrino flux, DUNE with its vast volume and reconstruction capabilities, is a promising candidate for a KDAR neutrino search. In this work, we evaluate the proposed KDAR neutrino search strategies by realistically modeling both neutrino-nucleus interactions and the response of DUNE. We find that, although reconstruction of the neutrino energy and direction is difficult with current techniques in the relevant energy range, the superb energy resolution, angular resolution, and particle identification offered by DUNE can still permit great signal/background discrimination. Moreover, there are non-standard scenarios in which searches at DUNE for KDAR in the Sun can probe dark matter interactions.</description><subject>Angular resolution</subject><subject>Dark matter</subject><subject>Energy resolution</subject><subject>Kaons</subject><subject>Neutrinos</subject><subject>Reconstruction</subject><subject>Search methods</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNotjstOAjEYRhsTEwnyAO4aXM_wX3qZLgkgGIkmimtSOh0ZQhhtQX18Jbr6zuqcT4gbhFJVWsPIp-_2syQEW4JDcBeiR8xYVIroSgxy3gEAGUtac08MX6JPYdse3mTTJZm7vU_yYTp-ll_tcSunr4-za3HZ-H2Og__ti9XdbDVZFMun-f1kvCy8JiyiZVCOY1Ubi3QGpSO4TYjO1AaxCRAsaIyNt75WtTXIyBYj6xAoIPfF7Z_2PXUfp5iP6113Soff4vp81TA5jfwDxXE9ug</recordid><startdate>20211027</startdate><enddate>20211027</enddate><creator>Acciarri, R</creator><creator>Back, A</creator><creator>Baldi, P</creator><creator>Bazo Alba, J 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arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20211027</creationdate><title>Searching for solar KDAR with DUNE</title><author>Acciarri, R ; Back, A ; Baldi, P ; Bazo Alba, J L ; C Benitez Montiel ; Berger, J ; Braga, D ; Brunetti, G ; Chatterjee, A ; Cherdack, D ; Chi, C ; Chisnall, G ; Choubey, S ; Clarke, P ; Conley, E ; Corwin, L ; Dawson, J ; Dias, M ; Diwan, M ; Duarte, L ; Duffy, K ; Flight, R ; Franco, D ; Gabrielli, A ; Gandrajula, R ; Gastler, D ; Gomes, R A ; Gran, R ; Green, P ; Groh, M ; Grudzinski, J ; Hamacher-Baumann, P ; Hertel, L ; Hill, T ; Holin, A ; Hourlier, A ; Hristova, I ; James, E ; Jediny, F ; Jung, C K ; F ; Kashur, L ; Koerner, L W ; Kumar, P ; Lang, K ; Larkin, J ; Lazanu, I ; L Li ; Loew, T ; Madera, A ; Manenti, L ; Marchan, M ; Marfatia, D ; Martinez Caicedo, D A ; Menary, S ; Meyer, H ; Molina, J ; Moon, J ; Morris, C ; W Mu ; Muir, A ; Musser, J ; Nandakumar, R ; Nesbit, J ; Nishimura, K ; Oberling, M ; Onishchuk, Y ; Paudel, A ; Perry, J ; Pessina, G ; Petti, R ; Poppi, F ; Rademacker, J ; Real, J S ; Rigaut, Y ; Rossella, M ; Rott, C ; Savage, G ; Sgalaberna, D ; Sinev, G ; Sobel, H ; Soto-Oton, J ; Spitz, J ; Strauss, T ; Surdo, A ; Susic, V ; Szczerbinska, B ; B Tapia Oregui ; Tatar, E ; Thorn, C ; Toups, M ; Tsverava, N ; Valdiviesso, G A ; Vergani, S ; Wallbank, M ; Wascko, M O ; Wei, H ; J Yu ; Zito, M ; Zucchelli, 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L</au><au>Marchan, M</au><au>Marfatia, D</au><au>Martinez Caicedo, D A</au><au>Menary, S</au><au>Meyer, H</au><au>Molina, J</au><au>Moon, J</au><au>Morris, C</au><au>W Mu</au><au>Muir, A</au><au>Musser, J</au><au>Nandakumar, R</au><au>Nesbit, J</au><au>Nishimura, K</au><au>Oberling, M</au><au>Onishchuk, Y</au><au>Paudel, A</au><au>Perry, J</au><au>Pessina, G</au><au>Petti, R</au><au>Poppi, F</au><au>Rademacker, J</au><au>Real, J S</au><au>Rigaut, Y</au><au>Rossella, M</au><au>Rott, C</au><au>Savage, G</au><au>Sgalaberna, D</au><au>Sinev, G</au><au>Sobel, H</au><au>Soto-Oton, J</au><au>Spitz, J</au><au>Strauss, T</au><au>Surdo, A</au><au>Susic, V</au><au>Szczerbinska, B</au><au>B Tapia Oregui</au><au>Tatar, E</au><au>Thorn, C</au><au>Toups, M</au><au>Tsverava, N</au><au>Valdiviesso, G A</au><au>Vergani, S</au><au>Wallbank, M</au><au>Wascko, M O</au><au>Wei, H</au><au>J Yu</au><au>Zito, M</au><au>Zucchelli, S</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Searching for solar KDAR with DUNE</atitle><jtitle>arXiv.org</jtitle><date>2021-10-27</date><risdate>2021</risdate><eissn>2331-8422</eissn><abstract>The observation of 236 MeV muon neutrinos from kaon-decay-at-rest (KDAR) originating in the core of the Sun would provide a unique signature of dark matter annihilation. Since excellent angle and energy reconstruction are necessary to detect this monoenergetic, directional neutrino flux, DUNE with its vast volume and reconstruction capabilities, is a promising candidate for a KDAR neutrino search. In this work, we evaluate the proposed KDAR neutrino search strategies by realistically modeling both neutrino-nucleus interactions and the response of DUNE. We find that, although reconstruction of the neutrino energy and direction is difficult with current techniques in the relevant energy range, the superb energy resolution, angular resolution, and particle identification offered by DUNE can still permit great signal/background discrimination. Moreover, there are non-standard scenarios in which searches at DUNE for KDAR in the Sun can probe dark matter interactions.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2107.09109</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2021-10 |
issn | 2331-8422 |
language | eng |
recordid | cdi_proquest_journals_2553632951 |
source | Publicly Available Content Database (Proquest) (PQ_SDU_P3) |
subjects | Angular resolution Dark matter Energy resolution Kaons Neutrinos Reconstruction Search methods |
title | Searching for solar KDAR with DUNE |
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