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Book ; Online: Molecular sieve vacuum swing adsorption purification and radon reduction system for gaseous dark matter and rare-event detectors

Gregorio, R. R. Marcelo / Spooner, N. J. C. / Dastgiri, F. / Ezeribe, A. C. / Lane, G. / McLean, A. G. / Miuchi, K. / Ogawa, H.

2023

Abstract: In the field of directional dark matter experiments, SF6 has emerged as an ideal target gas. A critical challenge with this gas, and with other proposed gases, is the effective removal of contaminant gases. This includes radon which produce unwanted ... ...

Abstract	In the field of directional dark matter experiments, SF6 has emerged as an ideal target gas. A critical challenge with this gas, and with other proposed gases, is the effective removal of contaminant gases. This includes radon which produce unwanted background events, but also common pollutants such as water, oxygen, and nitrogen, which can capture ionisation electrons, resulting in loss of detector gas gain over time. We present here a novel molecular sieve (MS) based gas recycling system for the simultaneous removal of both radon and common pollutants from SF6. The apparatus has the additional benefit of minimising gas required in experiments and utilises a Vacuum Swing Adsorption (VSA) technique for continuous, long-term operation. The gas system's capabilities were tested with a 100 L low-pressure SF6 Time Projection Chamber (TPC) detector. For the first time, we present a newly developed low-radioactive MS type 5A. This material was found to emanate radon at 98% less per radon captured compared to commercial counterparts, the lowest known MS emanation at the time of writing. Consequently, the radon activity in the TPC detector was reduced, with an upper limit of less than 7.2 mBq at a 95% confidence level (C.L.). Incorporation of MS types 3A and 4A to absorb common pollutants was found successfully to mitigate against gain deterioration while recycling the target gas.
Keywords	Physics - Instrumentation and Detectors
Subject code	660
Publishing date	2023-12-12
Publishing country	us
Document type	Book ; Online
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Book ; Online: Test of low radioactive molecular sieves for radon filtration in SF6 gas-based rare-event physics experiments

Gregorio, R. R. Marcelo / Spooner, N. J. C. / Berry, J. / Ezeribe, A. C. / Miuchi, K. / Ogawa, H. / Scarff, A.

2020

Abstract: Type 5A molecular sieves (MS) have been demonstrated to remove radon from SF$_6$ gas. This is important for ultra-sensitive SF$_6$ gas-based directional dark matter and related rare-event physics experiments, as radon can provide a source of unwanted ... ...

Abstract	Type 5A molecular sieves (MS) have been demonstrated to remove radon from SF$_6$ gas. This is important for ultra-sensitive SF$_6$ gas-based directional dark matter and related rare-event physics experiments, as radon can provide a source of unwanted background events. Unfortunately, commercially available sieves intrinsically emanate radon at levels not suitable for ultra-sensitive physics experiments. A method to produce a low radioactive MS has been developed in Nihon University (NU). In this work, we explore the feasibility of the NU-developed 5A type MS for use in such experiments. A comparison with a commercially available Sigma-Aldrich 5A type MS was made. The comparison was done by calculating a parameter indicating the amount of radon intrinsically emanated by the MS per unit radon captured from SF$_6$ gas. The measurements were made using a specially adapted DURRIDGE RAD7 radon detector. The NU-developed 5A MS emanated radon up to 61$\pm$9$\%$ less per radon captured (2.1$\pm$0.1)$\times 10^{-3}$, compared to the commercial Sigma-Aldrich MS (5.4$\pm$0.4)$\times 10^{-3}$, making it a better candidate for use in a radon filtration setup for future ultra-sensitive SF$_6$ gas based experiments.
Keywords	Physics - Instrumentation and Detectors ; High Energy Physics - Experiment ; Physics - Chemical Physics
Subject code	621
Publishing date	2020-11-13
Publishing country	us
Document type	Book ; Online
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Article ; Online: Search for Boosted Dark Matter in COSINE-100.

Adhikari, G / Carlin, N / Choi, J J / Choi, S / Ezeribe, A C / França, L E / Ha, C / Hahn, I S / Hollick, S J / Jeon, E J / Jo, J H / Joo, H W / Kang, W G / Kauer, M / Kim, B H / Kim, H J / Kim, J / Kim, K W / Kim, S H /

Kim, S K / Kim, W K / Kim, Y D / Kim, Y H / Ko, Y J / Lee, D H / Lee, E K / Lee, H / Lee, H S / Lee, H Y / Lee, I S / Lee, J / Lee, J Y / Lee, M H / Lee, S H / Lee, S M / Lee, Y J / Leonard, D S / Luan, N T / Manzato, B B / Maruyama, R H / Neal, R J / Nikkel, J A / Olsen, S L / Park, B J / Park, H K / Park, H S / Park, K S / Park, S D / Pitta, R L C / Prihtiadi, H / Ra, S J / Rott, C / Shin, K A / Cavalcante, D F F S / Scarff, A / Spooner, N J C / Thompson, W G / Yang, L / Yu, G H

Physical review letters

2023 Volume 131, Issue 20, Page(s) 201802

Abstract: We search for energetic electron recoil signals induced by boosted dark matter (BDM) from the galactic center using the COSINE-100 array of NaI(Tl) crystal detectors at the Yangyang Underground Laboratory. The signal would be an excess of events with ... ...

Abstract	We search for energetic electron recoil signals induced by boosted dark matter (BDM) from the galactic center using the COSINE-100 array of NaI(Tl) crystal detectors at the Yangyang Underground Laboratory. The signal would be an excess of events with energies above 4 MeV over the well-understood background. Because no excess of events are observed in a 97.7 kg·yr exposure, we set limits on BDM interactions under a variety of hypotheses. Notably, we explored the dark photon parameter space, leading to competitive limits compared to direct dark photon search experiments, particularly for dark photon masses below 4 MeV and considering the invisible decay mode. Furthermore, by comparing our results with a previous BDM search conducted by the Super-Kamionkande experiment, we found that the COSINE-100 detector has advantages in searching for low-mass dark matter. This analysis demonstrates the potential of the COSINE-100 detector to search for MeV electron recoil signals produced by the dark sector particle interactions.
Language	English
Publishing date	2023-11-30
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.131.201802
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Article ; Online: First Direct Search for Inelastic Boosted Dark Matter with COSINE-100.

Ha, C / Adhikari, G / Adhikari, P / Barbosa de Souza, E / Carlin, N / Choi, S / Djamal, M / Ezeribe, A C / Hahn, I S / Jeon, E J / Jo, J H / Joo, H W / Kang, W G / Kang, W / Kauer, M / Kim, G S / Kim, H / Kim, H J / Kim, K W /

Kim, N Y / Kim, S K / Kim, Y D / Kim, Y H / Ko, Y J / Kudryavtsev, V A / Lee, H S / Lee, J / Lee, J Y / Lee, M H / Leonard, D S / Lynch, W A / Maruyama, R H / Mouton, F / Olsen, S L / Park, B J / Park, H K / Park, H S / Park, K S / Pitta, R L C / Prihtiadi, H / Ra, S J / Rott, C / Shin, K A / Scarff, A / Spooner, N J C / Thompson, W G / Yang, L / Yu, G H

Physical review letters

2019 Volume 122, Issue 13, Page(s) 131802

Abstract: A search for inelastic boosted dark matter (IBDM) using the COSINE-100 detector with 59.5 days of data is presented. This relativistic dark matter is theorized to interact with the target material through inelastic scattering with electrons, creating a ... ...

Abstract	A search for inelastic boosted dark matter (IBDM) using the COSINE-100 detector with 59.5 days of data is presented. This relativistic dark matter is theorized to interact with the target material through inelastic scattering with electrons, creating a heavier state that subsequently produces standard model particles, such as an electron-positron pair. In this study, we search for this electron-positron pair in coincidence with the initially scattered electron as a signature for an IBDM interaction. No excess over the predicted background event rate is observed. Therefore, we present limits on IBDM interactions under various hypotheses, one of which allows us to explore an area of the dark photon parameter space that has not yet been covered by other experiments. This is the first experimental search for IBDM using a terrestrial detector.
Language	English
Publishing date	2019-04-23
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.122.131802
Database	MEDical Literature Analysis and Retrieval System OnLINE

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Article: Background model for the NaI(Tl) crystals in COSINE-100.

Adhikari, P / Adhikari, G / Souza, E Barbosa de / Carlin, N / Choi, S / Choi, W Q / Djamal, M / Ezeribe, A C / Ha, C / Hahn, I S / Hubbard, A J F / Jeon, E J / Jo, J H / Joo, H W / Kang, W G / Kauer, M / Kang, W S / Kim, B H / Kim, H /

Kim, H J / Kim, K W / Kim, M C / Kim, N Y / Kim, S K / Kim, Y D / Kim, Y H / Kudryavtsev, V A / Lee, H S / Lee, J / Lee, J Y / Lee, M H / Leonard, D S / Lynch, W A / Maruyama, R H / Mouton, F / Olsen, S L / Park, H K / Park, H S / Park, J S / Park, K S / Pettus, W / Prihtiadi, H / Ra, S / Rott, C / Scarff, A / Spooner, N J C / Thompson, W G / Yang, L / Yong, S H

The European physical journal. C, Particles and fields

2018 Volume 78, Issue 6, Page(s) 490

Abstract: The COSINE-100 dark matter search experiment is an array of NaI(Tl) crystal detectors located in the Yangyang Underground Laboratory (Y2L). To understand measured backgrounds in the NaI(Tl) crystals we have performed Monte Carlo simulations using the ... ...

Abstract	The COSINE-100 dark matter search experiment is an array of NaI(Tl) crystal detectors located in the Yangyang Underground Laboratory (Y2L). To understand measured backgrounds in the NaI(Tl) crystals we have performed Monte Carlo simulations using the Geant4 toolkit and developed background models for each crystal that consider contributions from both internal and external sources, including cosmogenic nuclides. The background models are based on comparisons of measurement data with Monte Carlo simulations that are guided by a campaign of material assays and are used to evaluate backgrounds and identify their sources. The average background level for the six crystals (70 kg total mass) that are studied is 3.5 counts/day/keV/kg in the (2-6) keV energy interval. The dominant contributors in this energy region are found to be
Language	English
Publishing date	2018-06-12
Publishing country	France
Document type	Journal Article
ZDB-ID	1459069-4
ISSN	1434-6052 ; 1434-6044
ISSN (online)	1434-6052
ISSN	1434-6044
DOI	10.1140/epjc/s10052-018-5970-2
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Book ; Online: Study of cosmogenic radionuclides in the COSINE-100 NaI(Tl) detectors

de Souza, E. Barbosa / Park, B. J. / Adhikari, G. / Adhikari, P. / Carlin, N. / Choi, J. J. / Choi, S. / Djamal, M. / Ezeribe, A. C. / Ha, C. / Hahn, I. S. / Jeon, E. J. / Jo, J. H. / Kang, W. G. / Kauer, M. / Kim, G. S. / Kim, H. / Kim, H. J. / Kim, K. W. /

Kim, N. Y. / Kim, S. K. / Kim, Y. D. / Kim, Y. H. / Ko, Y. J. / Kudryavtsev, V. A. / Lee, E. K. / Lee, H. S. / Lee, J. / Lee, J. Y. / Lee, M. H. / Lee, S. H. / Leonard, D. S. / Lynch, W. A. / Manzato, B. B. / Maruyama, R. H. / Neal, R. J. / Olsen, S. L. / Park, H. K. / Park, H. S. / Park, K. S. / Pitta, R. L. C. / Prihtiadi, H. / Ra, S. J. / Rott, C. / Shin, K. A. / Scarff, A. / Spooner, N. J. C. / Thompson, W. G. / Yang, L. / Yu, G. H. / Collaboration, COSINE-100

2019

Abstract: COSINE-100 is a direct detection dark matter search experiment that uses a 106 kg array of eight NaI(Tl) crystals that are kept underground at the Yangyang Underground Laboratory to avoid cosmogenic activation of radioisotopes by cosmic rays. Even though ...

Abstract	COSINE-100 is a direct detection dark matter search experiment that uses a 106 kg array of eight NaI(Tl) crystals that are kept underground at the Yangyang Underground Laboratory to avoid cosmogenic activation of radioisotopes by cosmic rays. Even though the cosmogenic activity is declining with time, there are still significant background rates from the remnant nuclides. In this paper, we report measurements of cosmogenic isotope contaminations with less than one year half-lives that are based on extrapolations of the time dependent activities of their characteristic energy peaks to activity rates at the time the crystals were deployed underground. For longer-lived $^{109}$Cd ($T_{1/2}=1.6$ y) and $^{22}$Na ($T_{1/2}=2.6$ y), we investigate time correlations of characteristic $\gamma$/X-ray peaks. The inferred sea-level production rates are compared with caluclations based on the ACTIVIA and MENDL-2 model calculations and experimental data. For $^{3}$H, which has a long, 12.3 year half-life, we evaluated the activity levels from the exposure times and determined a cosmogenic activation rate that is consistent with other measurements.
Keywords	Astrophysics - Instrumentation and Methods for Astrophysics
Subject code	333
Publishing date	2019-05-30
Publishing country	us
Document type	Book ; Online
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Article ; Online: Cosmic Ray Background Removal With Deep Neural Networks in SBND.

Acciarri, R / Adams, C / Andreopoulos, C / Asaadi, J / Babicz, M / Backhouse, C / Badgett, W / Bagby, L / Barker, D / Basque, V / Bazetto, M C Q / Betancourt, M / Bhanderi, A / Bhat, A / Bonifazi, C / Brailsford, D / Brandt, A G / Brooks, T / Carneiro, M F /

Chen, Y / Chen, H / Chisnall, G / Crespo-Anadón, J I / Cristaldo, E / Cuesta, C / de Icaza Astiz, I L / De Roeck, A / de Sá Pereira, G / Del Tutto, M / Di Benedetto, V / Ereditato, A / Evans, J J / Ezeribe, A C / Fitzpatrick, R S / Fleming, B T / Foreman, W / Franco, D / Furic, I / Furmanski, A P / Gao, S / Garcia-Gamez, D / Frandini, H / Ge, G / Gil-Botella, I / Gollapinni, S / Goodwin, O / Green, P / Griffith, W C / Guenette, R / Guzowski, P / Ham, T / Henzerling, J / Holin, A / Howard, B / Jones, R S / Kalra, D / Karagiorgi, G / Kashur, L / Ketchum, W / Kim, M J / Kudryavtsev, V A / Larkin, J / Lay, H / Lepetic, I / Littlejohn, B R / Louis, W C / Machado, A A / Malek, M / Mardsen, D / Mariani, C / Marinho, F / Mastbaum, A / Mavrokoridis, K / McConkey, N / Meddage, V / Méndez, D P / Mettler, T / Mistry, K / Mogan, A / Molina, J / Mooney, M / Mora, L / Moura, C A / Mousseau, J / Navrer-Agasson, A / Nicolas-Arnaldos, F J / Nowak, J A / Palamara, O / Pandey, V / Pater, J / Paulucci, L / Pimentel, V L / Psihas, F / Putnam, G / Qian, X / Raguzin, E / Ray, H / Reggiani-Guzzo, M / Rivera, D / Roda, M / Ross-Lonergan, M / Scanavini, G / Scarff, A / Schmitz, D W / Schukraft, A / Segreto, E / Soares Nunes, M / Soderberg, M / Söldner-Rembold, S / Spitz, J / Spooner, N J C / Stancari, M / Stenico, G V / Szelc, A / Tang, W / Tena Vidal, J / Torretta, D / Toups, M / Touramanis, C / Tripathi, M / Tufanli, S / Tyley, E / Valdiviesso, G A / Worcester, E / Worcester, M / Yarbrough, G / Yu, J / Zamorano, B / Zennamo, J / Zglam, A

Frontiers in artificial intelligence

2021 Volume 4, Page(s) 649917

Abstract: In liquid argon time projection chambers exposed to neutrino beams and running on or near surface levels, cosmic muons, and other cosmic particles are incident on the detectors while a single neutrino-induced event is being recorded. In practice, this ... ...

Abstract	In liquid argon time projection chambers exposed to neutrino beams and running on or near surface levels, cosmic muons, and other cosmic particles are incident on the detectors while a single neutrino-induced event is being recorded. In practice, this means that data from surface liquid argon time projection chambers will be dominated by cosmic particles, both as a source of event triggers and as the majority of the particle count in true neutrino-triggered events. In this work, we demonstrate a novel application of deep learning techniques to remove these background particles by applying deep learning on full detector images from the SBND detector, the near detector in the Fermilab Short-Baseline Neutrino Program. We use this technique to identify, on a pixel-by-pixel level, whether recorded activity originated from cosmic particles or neutrino interactions.
Language	English
Publishing date	2021-08-24
Publishing country	Switzerland
Document type	Journal Article
ISSN	2624-8212
ISSN (online)	2624-8212
DOI	10.3389/frai.2021.649917
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Article ; Online: Search for a Dark Matter-Induced Annual Modulation Signal in NaI(Tl) with the COSINE-100 Experiment.

Adhikari, G / Adhikari, P / de Souza, E Barbosa / Carlin, N / Choi, S / Djamal, M / Ezeribe, A C / Ha, C / Hahn, I S / Jeon, E J / Jo, J H / Joo, H W / Kang, W G / Kang, W / Kauer, M / Kim, G S / Kim, H / Kim, H J / Kim, K W /

Physical review letters

2015 Volume 123, Issue 3, Page(s) 31302

Abstract: We present new constraints on the dark matter-induced annual modulation signal using 1.7 years of COSINE-100 data with a total exposure of 97.7 kg yr. The COSINE-100 experiment, consisting of 106 kg of NaI(Tl) target material, is designed to carry out a ... ...

Abstract	We present new constraints on the dark matter-induced annual modulation signal using 1.7 years of COSINE-100 data with a total exposure of 97.7 kg yr. The COSINE-100 experiment, consisting of 106 kg of NaI(Tl) target material, is designed to carry out a model-independent test of DAMA/LIBRA's claim of WIMP discovery by searching for the same annual modulation signal using the same NaI(Tl) target. The crystal data show a 2.7 cpd/kg/keV background rate on average in the 2-6 keV energy region of interest. Using a χ-squared minimization method we observe best fit values for modulation amplitude and phase of 0.0092±0.0067 cpd/kg/keV and 127.2±45.9 d, respectively.
Language	English
Publishing date	2015-09-30
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.123.031302
Database	MEDical Literature Analysis and Retrieval System OnLINE

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Article: Scintillation light detection in the 6-m drift-length ProtoDUNE Dual Phase liquid argon TPC.

Abud, A Abed / Abi, B / Acciarri, R / Acero, M A / Adames, M R / Adamov, G / Adamowski, M / Adams, D / Adinolfi, M / Aduszkiewicz, A / Aguilar, J / Ahmad, Z / Ahmed, J / Aimard, B / Ali-Mohammadzadeh, B / Alion, T / Allison, K / Monsalve, S Alonso / AlRashed, M /

Alt, C / Alton, A / Alvarez, R / Amedo, P / Anderson, J / Andreopoulos, C / Andreotti, M / Andrews, M / Andrianala, F / Andringa, S / Anfimov, N / Ankowski, A / Antoniassi, M / Antonova, M / Antoshkin, A / Antusch, S / Aranda-Fernandez, A / Arellano, L / Arnold, L O / Arroyave, M A / Asaadi, J / Asquith, L / Aurisano, A / Aushev, V / Autiero, D / Lara, V Ayala / Ayala-Torres, M / Azfar, F / Back, A / Back, H / Back, J J / Backhouse, C / Bagaturia, I / Bagby, L / Balashov, N / Balasubramanian, S / Baldi, P / Baller, B / Bambah, B / Barao, F / Barenboim, G / Alzas, P Barham / Barker, G / Barkhouse, W / Barnes, C / Barr, G / Monarca, J Barranco / Barros, A / Barros, N / Barrow, J L / Basharina-Freshville, A / Bashyal, A / Basque, V / Batchelor, C / Chagas, E Batista das / Battat, J B R / Battisti, F / Bay, F / Bazetto, M C Q / Alba, J L L Bazo / Beacom, J F / Bechetoille, E / Behera, B / Beigbeder, C / Bellantoni, L / Bellettini, G / Bellini, V / Beltramello, O / Benekos, N / Montiel, C Benitez / Neves, F Bento / Berger, J / Berkman, S / Bernardini, P / Berner, R M / Bersani, A / Bertolucci, S / Betancourt, M / Rodríguez, A Betancur / Bevan, A / Bezawada, Y / Bezerra, T J C / Bhardwaj, A / Bhatnagar, V / Bhattacharjee, M / Bhattarai, D / Bhuller, S / Bhuyan, B / Biagi, S / Bian, J / Biassoni, M / Biery, K / Bilki, B / Bishai, M / Bitadze, A / Blake, A / Blaszczyk, F / Blazey, G C / Blucher, E / Boissevain, J / Bolognesi, S / Bolton, T / Bomben, L / Bonesini, M / Bongrand, M / Bonilla-Diaz, C / Bonini, F / Booth, A / Boran, F / Bordoni, S / Borkum, A / Bostan, N / Bour, P / Bourgeois, C / Boyden, D / Bracinik, J / Braga, D / Brailsford, D / Branca, A / Brandt, A / Bremer, J / Breton, D / Brew, C / Brice, S J / Brizzolari, C / Bromberg, C / Brooke, J / Bross, A / Brunetti, G / Brunetti, M / Buchanan, N / Budd, H / Butorov, I / Cagnoli, I / Cai, T / Caiulo, D / Calabrese, R / Calafiura, P / Calcutt, J / Calin, M / Calvez, S / Calvo, E / Caminata, A / Campanelli, M / Caratelli, D / Carber, D / Carceller, J C / Carini, G / Carlus, B / Carneiro, M F / Carniti, P / Terrazas, I Caro / Carranza, H / Carroll, T / Forero, J F Castaño / Castillo, A / Castromonte, C / Catano-Mur, E / Cattadori, C / Cavalier, F / Cavallaro, G / Cavanna, F / Centro, S / Cerati, G / Cervelli, A / Villanueva, A Cervera / Chalifour, M / Chappell, A / Chardonnet, E / Charitonidis, N / Chatterjee, A / Chattopadhyay, S / Neyra, M S S Chavarry / Chen, H / Chen, M / Chen, Y / Chen, Z / Chen-Wishart, Z / Cheon, Y / Cherdack, D / Chi, C / Childress, S / Chirco, R / Chiriacescu, A / Chisnall, G / Cho, K / Choate, S / Chokheli, D / Chong, P S / Christensen, A / Christian, D / Christodoulou, G / Chukanov, A / Chung, M / Church, E / Cicero, V / Clarke, P / Cline, G / Coan, T E / Cocco, A G / Coelho, J A B / Colton, N / Conley, E / Conley, R / Conrad, J / Convery, M / Copello, S / Cova, P / Cremaldi, L / Cremonesi, L / Crespo-Anadón, J I / Crisler, M / Cristaldo, E / Crnkovic, J / Cross, R / Cudd, A / Cuesta, C / Cui, Y / Cussans, D / Dalager, O / da Motta, H / Da Silva Peres, L / David, C / David, Q / Davies, G S / Davini, S / Dawson, J / De, K / De, S / Debbins, P / De Bonis, I / Decowski, M P / De Gouvêa, A / De Holanda, P C / De Icaza Astiz, I L / Deisting, A / De Jong, P / Delbart, A / Delepine, D / Delgado, M / Dell'Acqua, A / Delmonte, N / De Lurgio, P / de Mello Neto, J R T / DeMuth, D M / Dennis, S / Densham, C / Deptuch, G W / De Roeck, A / De Romeri, V / De Souza, G / Devi, R / Dharmapalan, R / Dias, M / Diaz, F / Díaz, J S / Domizio, S Di / Giulio, L Di / Ding, P / Noto, L Di / Dirkx, G / Distefano, C / Diurba, R / Diwan, M / Djurcic, Z / Doering, D / Dolan, S / Dolek, F / Dolinski, M / Domine, L / Donon, Y / Douglas, D / Douillet, D / Dragone, A / Drake, G / Drielsma, F / Duarte, L / Duchesneau, D / Duffy, K / Dunne, P / Dutta, B / Duyang, H / Dvornikov, O / Dwyer, D / Dyshkant, A / Eads, M / Earle, A / Edmunds, D / Eisch, J / Emberger, L / Emery, S / Englezos, P / Ereditato, A / Erjavec, T / Escobar, C / Eurin, G / Evans, J J / Ewart, E / Ezeribe, A C / Fahey, K / Falcone, A / Fani', M / Farnese, C / Farzan, Y / Fedoseev, D / Felix, J / Feng, Y / Fernandez-Martinez, E / Menendez, P Fernandez / Morales, M Fernandez / Ferraro, F / Fields, L / Filip, P / Filthaut, F / Fiorini, M / Fischer, V / Fitzpatrick, R S / Flanagan, W / Fleming, B / Flight, R / Fogarty, S / Foreman, W / Fowler, J / Fox, W / Franc, J / Francis, K / Franco, D / Freeman, J / Freestone, J / Fried, J / Friedland, A / Robayo, F Fuentes / Fuess, S / Furic, I K / Furman, K / Furmanski, A P / Gabrielli, A / Gago, A / Gallagher, H / Gallas, A / Gallego-Ros, A / Gallice, N / Galymov, V / Gamberini, E / Gamble, T / Ganacim, F / Gandhi, R / Gandrajula, R / Gao, F / Gao, S / Garcia-Gamez, D / García-Peris, M Á / Gardiner, S / Gastler, D / Gauvreau, J / Ge, G / Geffroy, N / Gelli, B / Gendotti, A / Gent, S / Ghorbani-Moghaddam, Z / Giammaria, P / Giammaria, T / Giangiacomi, N 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Muramatsu, H / Murphy, S / Musser, J / Nachtman, J / Nagu, S / Nalbandyan, M / Nandakumar, R / Naples, D / Narita, S / Nath, A / Navrer-Agasson, A / Nayak, N / Nebot-Guinot, M / Negishi, K / Nelson, J K / Nesbit, J / Nessi, M / Newbold, D / Newcomer, M / Newton, H / Nichol, R / Nicolas-Arnaldos, F / Nikolica, A / Niner, E / Nishimura, K / Norman, A / Norrick, A / Northrop, R / Novella, P / Nowak, J A / Oberling, M / Ochoa-Ricoux, J / Olivier, A / Olshevskiy, A / Onel, Y / Onishchuk, Y / Ott, J / Pagani, L / Palacio, G / Palamara, O / Palestini, S / Paley, J M / Pallavicini, M / Palomares, C / Vazquez, W Panduro / Pantic, E / Paolone, V / Papadimitriou, V / Papaleo, R / Papanestis, A / Paramesvaran, S / Parke, S / Parozzi, E / Parsa, Z / Parvu, M / Pascoli, S / Pasqualini, L / Pasternak, J / Pater, J / Patrick, C / Patrizii, L / Patterson, R B / Patton, S J / Patzak, T / Paudel, A / Paulos, B / Paulucci, L / Pavlovic, Z / Pawloski, G / Payne, D / Pec, V / Peeters, S J M / Perez, A Pena / Pennacchio, E / Penzo, A / Peres, O L G / Perry, J / Pershey, D / Pessina, G / Petrillo, G / Petta, C / Petti, R / Pia, V / Piastra, F / Pickering, L / Pietropaolo, F / Pimentel, V L / Pinaroli, G / Plows, K / Plunkett, R / Poling, R / Pompa, F / Pons, X / Poonthottathil, N / Poppi, F / Pordes, S / Porter, J / Potekhin, M / Potenza, R / Potukuchi, B V K S / Pozimski, J / Pozzato, M / Prakash, S / Prakash, T / Prest, M / Prince, S / Psihas, F / Pugnere, D / Qian, X / Raaf, J L / Radeka, V / Rademacker, J / Radics, B / Rafique, A / Raguzin, E / Rai, M / Rajaoalisoa, M / Rakhno, I / Rakotonandrasana, A / Rakotondravohitra, L / Rameika, R / Delgado, M A Ramirez / Ramson, B / Rappoldi, A / Raselli, G / Ratoff, P / Raut, S / Razakamiandra, R F / Rea, E M / Real, J S / Rebel, B / Rechenmacher, R / Reggiani-Guzzo, M / Reichenbacher, J / Reitzner, S D / Sfar, H Rejeb / Renshaw, A / Rescia, S / Resnati, F / Ribas, M / Riboldi, S / Riccio, C / Riccobene, G / Rice, L C J / Ricol, J S / Rigamonti, A / Rigaut, Y / Rincón, E V / Ritchie-Yates, H / Rivera, D / Robert, A / Rochester, L / Roda, M / Rodrigues, P / Alonso, M J Rodriguez / Bonilla, E Rodriguez / Rondon, J Rodriguez / Rosauro-Alcaraz, S / Rosenberg, M / Rosier, P / Roskovec, B / Rossella, M / Rossi, M / Rout, J / Roy, P / Rubbia, A / Rubbia, C / Russell, B / Ruterbories, D / Rybnikov, A / Saa-Hernandez, A / Saakyan, R / Sacerdoti, S / Safford, T / Sahu, N / Sakashita, K / Sala, P / Samios, N / Samoylov, O / Sanchez, M C / Sandberg, V / Sanders, D A / Sankey, D / Santana, S / Santos-Maldonado, M / Saoulidou, N / Sapienza, P / Sarasty, C / Sarcevic, I / Savage, G / Savinov, V / Scaramelli, A / Scarff, A / Scarpelli, A / Schefke, T / Schellman, H / Schifano, S / Schlabach, P / Schmitz, D / Schneider, A W / Scholberg, K / Schukraft, A / Segreto, E / Selyunin, A / Senise, C R / Sensenig, J / Sergi, A / Sgalaberna, D / Shaevitz, M H / Shafaq, S / Shaker, F / Shamma, M / Sharankova, R / Sharma, H R / Sharma, R / 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Zennamo, J / Zeug, K / Zhang, C / Zhang, S / Zhang, Y / Zhao, M / Zhivun, E / Zhu, G / Zimmerman, E D / Zucchelli, S / Zuklin, J / Zutshi, V / Zwaska, R

The European physical journal. C, Particles and fields

2022 Volume 82, Issue 7, Page(s) 618

Abstract: DUNE is a dual-site experiment for long-baseline neutrino oscillation studies, neutrino astrophysics and nucleon decay searches. ProtoDUNE Dual Phase (DP) is a ... ...

Abstract	DUNE is a dual-site experiment for long-baseline neutrino oscillation studies, neutrino astrophysics and nucleon decay searches. ProtoDUNE Dual Phase (DP) is a 6
Language	English
Publishing date	2022-07-16
Publishing country	France
Document type	Journal Article
ZDB-ID	1459069-4
ISSN	1434-6052 ; 1434-6044
ISSN (online)	1434-6052
ISSN	1434-6044
DOI	10.1140/epjc/s10052-022-10549-w
Database	MEDical Literature Analysis and Retrieval System OnLINE

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Article: Prospects for beyond the Standard Model physics searches at the Deep Underground Neutrino Experiment: DUNE Collaboration.

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The European physical journal. C, Particles and fields

2021 Volume 81, Issue 4, Page(s) 322

Abstract: The Deep Underground Neutrino Experiment (DUNE) will be a powerful tool for a variety of physics topics. The high-intensity proton beams provide a large neutrino flux, sampled by a near detector system consisting of a combination of capable precision ... ...

Abstract	The Deep Underground Neutrino Experiment (DUNE) will be a powerful tool for a variety of physics topics. The high-intensity proton beams provide a large neutrino flux, sampled by a near detector system consisting of a combination of capable precision detectors, and by the massive far detector system located deep underground. This configuration sets up DUNE as a machine for discovery, as it enables opportunities not only to perform precision neutrino measurements that may uncover deviations from the present three-flavor mixing paradigm, but also to discover new particles and unveil new interactions and symmetries beyond those predicted in the Standard Model (SM). Of the many potential beyond the Standard Model (BSM) topics DUNE will probe, this paper presents a selection of studies quantifying DUNE's sensitivities to sterile neutrino mixing, heavy neutral leptons, non-standard interactions, CPT symmetry violation, Lorentz invariance violation, neutrino trident production, dark matter from both beam induced and cosmogenic sources, baryon number violation, and other new physics topics that complement those at high-energy colliders and significantly extend the present reach.
Language	English
Publishing date	2021-04-16
Publishing country	France
Document type	Journal Article
ZDB-ID	1459069-4
ISSN	1434-6052 ; 1434-6044
ISSN (online)	1434-6052
ISSN	1434-6044
DOI	10.1140/epjc/s10052-021-09007-w
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