Jiajie Ling

Sun Yat-Sen University

H-index: 62

Asia-China

About Jiajie Ling

Jiajie Ling, With an exceptional h-index of 62 and a recent h-index of 44 (since 2020), a distinguished researcher at Sun Yat-Sen University, specializes in the field of particle physics, neutrino physics.

His recent articles reflect a diverse array of research interests and contributions to the field:

Charged-current non-standard neutrino interactions at Daya Bay

Performance of a modular ton-scale pixel-readout liquid argon time projection chamber

First measurement of the yield of He isotopes produced in liquid scintillator by cosmic-ray muons at Daya Bay

Doping liquid argon with xenon in ProtoDUNE Single-Phase: effects on scintillation light

Real-time monitoring for the next core-collapse supernova in JUNO

Search for a sub-eV sterile neutrino using Daya Bay's full dataset

The DUNE Far Detector Vertical Drift Technology, Technical Design Report

arXiv: Performance of a modular ton-scale pixel-readout liquid argon time projection chamber

Jiajie Ling Information

University	Sun Yat-Sen University
Position	Professor of Physics
Citations(all)	20911
Citations(since 2020)	7725
Cited By	16204
hIndex(all)	62
hIndex(since 2020)	44
i10Index(all)	119
i10Index(since 2020)	106
Email	Access Email
University Profile Page	Sun Yat-Sen University

Jiajie Ling Skills & Research Interests

particle physics

neutrino physics

Search for a sub-eV sterile neutrino using Daya Bay's full dataset

Authors

Journal

arXiv preprint arXiv:2404.01687

Published Date

2024/4/2

This Letter presents results of a search for the mixing of a sub-eV sterile neutrino based on the full data sample of the Daya Bay Reactor Neutrino Experiment, collected during 3158 days of detector operation, which contains reactor \anue candidates identified as inverse beta-decay interactions followed by neutron-capture on gadolinium. The result was obtained in the minimally extended 3+1 neutrino mixing model. The analysis benefits from a doubling of the statistics of our previous result and from improvements of several important systematic uncertainties. The results are consistent with the standard three-neutrino mixing model and no significant signal of a sub-eV sterile neutrino was found. Exclusion limits are set by both Feldman-Cousins and CLs methods. Light sterile neutrino mixing with can be excluded at 95\% confidence level in the region of eV eV. This result represents the world-leading constraints in the region of eV eV.

The DUNE Far Detector Vertical Drift Technology, Technical Design Report

Authors

A Abed Abud,B Abi,R Acciarri,MA Acero,MR Adames,G Adamov,M Adamowski,D Adams,M Adinolfi,C Adriano,A Aduszkiewicz,J Aguilar,B Aimard,F Akbar,K Allison,S Alonso Monsalve,M Alrashed,A Alton,R Alvarez,H Amar,P Amedo,J Anderson,DA Andrade,C Andreopoulos,M Andreotti,MP Andrews,F Andrianala,S Andringa,N Anfimov,A Ankowski,M Antoniassi,M Antonova,A Antoshkin,A Aranda-Fernandez,L Arellano,E Arrieta Diaz,MA Arroyave,J Asaadi,A Ashkenazi,L Asquith,E Atkin,D Auguste,A Aurisano,V Aushev,D Autiero,F Azfar,A Back,H Back,JJ Back,I Bagaturia,L Bagby,N Balashov,S Balasubramanian,P Baldi,W Baldini,B Baller,B Bambah,R Banerjee,F Barao,G Barenboim,P Barham Alzás,GJ Barker,W Barkhouse,G Barr,J Barranco Monarca,A Barros,N Barros,D Barrow,JL Barrow,A Basharina-Freshville,A Bashyal,V Basque,C Batchelor,L Bathe-Peters,JBR Battat,F Battisti,F Bay,MCQ Bazetto,JLL Alba,JF Beacom,E Bechetoille,B Behera,E Belchior,G Bell,L Bellantoni,G Bellettini,V Bellini,O Beltramello,N Benekos,C Benitez Montiel,D Benjamin,F Bento Neves,J Berger,S Berkman,P Bernardini,A Bersani,S Bertolucci,M Betancourt,A Betancur Rodríguez,A Bevan,Y Bezawada,AT Bezerra,TJ Bezerra,A Bhat,V Bhatnagar,J Bhatt,M Bhattacharjee,M Bhattacharya,S Bhuller,B Bhuyan,S Biagi,J Bian,K Biery,B Bilki,M Bishai,A Bitadze,A Blake,FD Blaszczyk,GC Blazey,E Blucher,J Boissevain,S Bolognesi,T Bolton,L Bomben,M Bonesini,C Bonilla-Diaz,F Bonini,A Booth,F Boran,S Bordoni,R Borges Merlo,A Borkum,N Bostan,J Bracinik,D Braga,B Brahma,D Brailsford,F Bramati,A Branca,A Brandt,J Bremer,C Brew,SJ Brice,V Brio,C Brizzolari,C Bromberg,J Brooke,A Bross,G Brunetti,M Brunetti

Journal

arXiv preprint arXiv:2312.03130

Published Date

2023/12/5

DUNE is an international experiment dedicated to addressing some of the questions at the forefront of particle physics and astrophysics, including the mystifying preponderance of matter over antimatter in the early universe. The dual-site experiment will employ an intense neutrino beam focused on a near and a far detector as it aims to determine the neutrino mass hierarchy and to make high-precision measurements of the PMNS matrix parameters, including the CP-violating phase. It will also stand ready to observe supernova neutrino bursts, and seeks to observe nucleon decay as a signature of a grand unified theory underlying the standard model. The DUNE far detector implements liquid argon time-projection chamber (LArTPC) technology, and combines the many tens-of-kiloton fiducial mass necessary for rare event searches with the sub-centimeter spatial resolution required to image those events with high precision. The addition of a photon detection system enhances physics capabilities for all DUNE physics drivers and opens prospects for further physics explorations. Given its size, the far detector will be implemented as a set of modules, with LArTPC designs that differ from one another as newer technologies arise. In the vertical drift LArTPC design, a horizontal cathode bisects the detector, creating two stacked drift volumes in which ionization charges drift towards anodes at either the top or bottom. The anodes are composed of perforated PCB layers with conductive strips, enabling reconstruction in 3D. Light-trap-style photon detection modules are placed both on the cryostat's side walls and on the central cathode where they are …

arXiv: Performance of a modular ton-scale pixel-readout liquid argon time projection chamber

Authors

Adam Abed Abud,Pierre Granger,Sanjay Swain,Pierre Baldi,Marcelo Antoniassi,Silvia Pascoli,Paul De Jong,Nikolozi Tsverava,Zahra Ghorbani-Moghaddam,John Learned,David Warner,Gregory Michna,Catia Petta,David Payne,Ina Sarcevic,Eric Zimmerman,Stefano Di Falco,Wayne Barkhouse,Laura Zambelli,Alexander Bitadze,Matheus Hostert,Edward Blucher,Vitaliy Popov,Simone Biagi,Daisy Kalra,Andrew Lawrence,Sandeep Miryala,Tom Lord,Keith Gollwitzer,Niccolo Gallice,Joshua Barrow,Nicola Delmonte,Nicolas Geffroy,Carmen Giugliano,Hugh Gallagher,Brian Rebel,Adrian Thompson,Jacob Goudeau,Giuseppe Cerati,Mark Adamowski,Guillermo Palacio,Atanu Nath,Sujit Sahoo,Andrea Falcone,Luis Montaño Zetina,Paul Smith,Francisco Ganacim,Alessandro Thea,Biswaranjan Behera,Carlos Senise Jr,Faiza Akbar,Kurtis Nishimura,Pablo Amedo,Luca Bomben,Matthew Kramer,Kunal Kothekar,Dmitry Fedoseev,Robert Zwaska,Sofia Andringa,Andrés Castillo,Antonio Gioiosa,Simona Giovannella,Hirohisa Tanaka,Jack Fried,Johan Bremer,Francisco Nicolas-Arnaldos,Adam Lister,Piera Sapienza,Nicola McConkey,Jaroslaw Pasternak,Veljko Radeka,Niccolo Moggi,Douglas Benjamin,Nadine Kurita,Matthew Wetstein,Yasaman Farzan,Wei Mu,Anibal Bezerra,Julio Ureña González,Laura Molina Bueno,Elena Gramellini,Olivia Dalager,Dario Autiero,Edgar Rincón,A Rappoldi,Alejandro Diaz,Eric Guerard,Fabio Happacher,Emilija Pantic,Burak Bilki,Tim Young,Alfonso Madera,Ian Kotler,Ruben Saakyan,Steven Dytman,Niki Saoulidou,Elisabetta Pennacchio,Jose Valle,Daniele Montanino,Jeremy Wolcott,Andrew Mastbaum,Paul Keener,Grzegorz Deptuch,Quynh Vuong,Arseniy Rybnikov,Wei Shi,Giacomo Scanavini,Yi Wang,Sabrina Sacerdoti,Shirley W Li,Carlos Benitez Montiel,Esteban Cristaldo,Liudmila Kolupaeva,Pierre Lasorak,Gavin Davies,Fatma Boran,Mitch Soderberg,Haiwang Yu,Linhui Gu,Marcelo Ismerio Oliveira,Avinay Bhat,EL Snider,Furkan Dolek,Antonis Papanestis,Konstantinos Manolopoulos,Diana Méndez,Raul Stein,Mitchell Mote,Ornella Palamara,Letizia Di Giulio,Yuying Guo,Supraja Balasubramanian,Valerio Giusti,Steven Doran,Jovana Nikolov,Oleg Samoylov,AM Gago,Haifa Rejeb Sfar,Aretha Mercuri,Olga Gogota,Fernando Gardim,Michael Wang,James Matthews,David Martinez Caicedo,Giorgio Riccobene,Yanou Cui,James Stewart,Javier Bernal,Joseph Walsh,Terri Shaw

Published Date

2024/3/5

Precision measurement of reactor antineutrino oscillation at kilometer-scale baselines by Daya Bay

Authors

FP An,WD Bai,AB Balantekin,M Bishai,S Blyth,GF Cao,J Cao,JF Chang,Y Chang,HS Chen,HY Chen,SM Chen,Y Chen,YX Chen,ZY Chen,J Cheng,ZK Cheng,JJ Cherwinka,MC Chu,JP Cummings,O Dalager,FS Deng,YY Ding,XY Ding,MV Diwan,T Dohnal,D Dolzhikov,J Dove,HY Duyang,DA Dwyer,JP Gallo,M Gonchar,GH Gong,H Gong,WQ Gu,JY Guo,L Guo,XH Guo,YH Guo,Z Guo,RW Hackenburg,Y Han,S Hans,M He,KM Heeger,YK Heng,YK Hor,YB Hsiung,BZ Hu,JR Hu,T Hu,ZJ Hu,HX Huang,JH Huang,XT Huang,YB Huang,P Huber,DE Jaffe,KL Jen,XL Ji,XP Ji,RA Johnson,D Jones,L Kang,SH Kettell,S Kohn,M Kramer,TJ Langford,J Lee,JHC Lee,RT Lei,R Leitner,JKC Leung,F Li,HL Li,JJ Li,QJ Li,RH Li,S Li,SC Li,WD Li,XN Li,XQ Li,YF Li,ZB Li,H Liang,CJ Lin,GL Lin,S Lin,JJ Ling,JM Link,L Littenberg,BR Littlejohn,JC Liu,JL Liu,JX Liu,C Lu,HQ Lu,KB Luk,BZ Ma,XB Ma,XY Ma,YQ Ma,RC Mandujano,C Marshall,KT McDonald,RD McKeown,Y Meng,J Napolitano,D Naumov,E Naumova,TMT Nguyen,JP Ochoa-Ricoux,A Olshevskiy,H-R Pan,J Park,S Patton,JC Peng,CSJ Pun,FZ Qi,M Qi,X Qian,N Raper,J Ren,C Morales Reveco,R Rosero,B Roskovec,XC Ruan,B Russell,H Steiner,JL Sun,T Tmej,K Treskov,W-H Tse,CE Tull,B Viren,V Vorobel,CH Wang,J Wang,M Wang,NY Wang,RG Wang,W Wang,X Wang,Y Wang,YF Wang,Z Wang,ZM Wang,HY Wei,LH Wei

Journal

Physical review letters

Published Date

2023/4/21

We present a new determination of the smallest neutrino mixing angle θ 13 and the mass-squared difference Δ m 32 2 using a final sample of 5.55× 10 6 inverse beta-decay (IBD) candidates with the final-state neutron captured on gadolinium. This sample is selected from the complete dataset obtained by the Daya Bay reactor neutrino experiment in 3158 days of operation. Compared to the previous Daya Bay results, selection of IBD candidates has been optimized, energy calibration refined, and treatment of backgrounds further improved. The resulting oscillation parameters are sin 2 2 θ 13= 0.0851±0.0024, Δ m 32 2=(2.466±0.060)× 10− 3 eV 2 for the normal mass ordering or Δ m 32 2=−(2.571±0.060)× 10− 3 eV 2 for the inverted mass ordering.

Impact of cross-section uncertainties on supernova neutrino spectral parameter fitting in the Deep Underground Neutrino Experiment

Authors

A Abed Abud,Babak Abi,Roberto Acciarri,MA Acero,MR Adames,George Adamov,Mark Adamowski,David Adams,Marco Adinolfi,Cris Adriano,Antoni Aduszkiewicz,Jessica Aguilar,Zubayer Ahmad,Jhanzeb Ahmed,Benjamin Aimard,Faiza Akbar,Kyle Allison,S Alonso Monsalve,Munera Alrashed,Andrew Alton,Rodrigo Alvarez,Pablo Amedo,John Anderson,DA Andrade,Costas Andreopoulos,Mirco Andreotti,Michael P Andrews,Fenompanirina Andrianala,Sofia Andringa,Nikolay Anfimov,WL Anicézio Campanelli,Artur Ankowski,Marcelo Antoniassi,Maria Antonova,Alexander Antoshkin,Alfredo Aranda-Fernandez,Luciano Arellano,LO Arnold,MA Arroyave,Jonathan Asaadi,Adi Ashkenazi,Lily Asquith,Edward Atkin,Didier Auguste,Adam Aurisano,Vladimir Aushev,Dario Autiero,M Ayala-Torres,Farrukh Azfar,Ashley Back,Henning Back,JJ Back,Iuri Bagaturia,Linda Bagby,Nikita Balashov,Supraja Balasubramanian,Pierre Baldi,Wander Baldini,Bruce Baller,Bindu Bambah,Rituparna Banerjee,Fernando Barao,Gabriela Barenboim,P Barham Alzás,GJ Barker,Wayne Barkhouse,Christopher Barnes,Giles Barr,J Barranco Monarca,Adilson Barros,Nuno Barros,JL Barrow,Anastasia Basharina-Freshville,Amit Bashyal,Vincent Basque,Charlie Batchelor,JBR Battat,Federico Battisti,Fatih Bay,MCQ Bazetto,JLL Bazo Alba,JF Beacom,Edouard Bechetoille,Biswaranjan Behera,Ewerton Belchior,Gerard Bell,Leo Bellantoni,Giorgio Bellettini,Vincenzo Bellini,Olga Beltramello,Nektarios Benekos,C Benitez Montiel,Douglas Benjamin,F Bento Neves,Joshua Berger,Sophie Berkman,Paolo Bernardini,RM Berner,Andrea Bersani,Sergio Bertolucci,Minerba Betancourt,A Betancur Rodríguez,Adrian Bevan,Yashwanth Bezawada,AT Bezerra,TJ Bezerra,Jay Bhambure,Akhil Bhardwaj,Vipin Bhatnagar,Maharnab Bhattacharjee,Meghna Bhattacharya,Devesh Bhattarai,Shyam Bhuller,Bipul Bhuyan,Simone Biagi,Jianming Bian,Kurt Biery,Burak Bilki,Mary Bishai,Alexander Bitadze,Andrew Blake,FD Blaszczyk,GC Blazey,Dylan Blend,Edward Blucher,Jan Boissevain,Sara Bolognesi,Timothy Bolton,Luca Bomben,Maurizio Bonesini,Cesar Bonilla-Diaz,Filiberto Bonini,Alexander Booth,Fatma Boran,Stefania Bordoni,Aran Borkum,Nilay Bostan,Petr Bour,Juraj Bracinik,Davide Braga,Dominic Brailsford,Antonio Branca,Andrew Brandt,Marina Bravo-Moreno,Johan Bremer,Christopher Brew,SJ Brice,Vanessa Brio,Claudia Brizzolari,Carl Bromberg

Journal

Physical Review D

Published Date

2023/6/29

JUNO sensitivity on proton decay p→ ν K+ searches

Authors

Angel Abusleme,Thomas Adam,Shakeel Ahmad,Rizwan Ahmed,Sebastiano Aiello,Muhammad Akram,Fengpeng An,Qi An,Giuseppe Andronico,Nikolay Anfimov,Vito Antonelli,Tatiana Antoshkina,Burin Asavapibhop,João Pedro Athayde Marcondes de André,Didier Auguste,Nikita Balashov,Wander Baldini,Andrea Barresi,Davide Basilico,Eric Baussan,Marco Bellato,Antonio Bergnoli,Thilo Birkenfeld,Sylvie Blin,David Blum,Simon Blyth,Anastasia Bolshakova,Mathieu Bongrand,Clément Bordereau,Dominique Breton,Augusto Brigatti,Riccardo Brugnera,Riccardo Bruno,Antonio Budano,Mario Buscemi,Jose Busto,Ilya Butorov,Anatael Cabrera,Barbara Caccianiga,Hao Cai,Xiao Cai,Yanke Cai,Zhiyan Cai,Riccardo Callegari,Antonio Cammi,Agustin Campeny,Chuanya Cao,Guofu Cao,Jun Cao,Rossella Caruso,Cédric Cerna,Jinfan Chang,Yun Chang,Pingping Chen,Po-An Chen,Shaomin Chen,Xurong Chen,Yi-Wen Chen,Yixue Chen,Yu Chen,Zhang Chen,Jie Cheng,Yaping Cheng,Alexey Chetverikov,Davide Chiesa,Pietro Chimenti,Artem Chukanov,Gérard Claverie,Catia Clementi,Barbara Clerbaux,Selma Conforti Di Lorenzo,Daniele Corti,Flavio Dal Corso,Olivia Dalager,Christophe De La Taille,Zhi Deng,Ziyan Deng,Wilfried Depnering,Marco Diaz,Xuefeng Ding,Yayun Ding,Bayu Dirgantara,Sergey Dmitrievsky,Tadeas Dohnal,Dmitry Dolzhikov,Georgy Donchenko,Jianmeng Dong,Evgeny Doroshkevich,Marcos Dracos,Frédéric Druillole,Ran Du,Shuxian Du,Stefano Dusini,Martin Dvorak,Timo Enqvist,Heike Enzmann,Andrea Fabbri,Ulrike Fahrendholz,Donghua Fan,Lei Fan,Jian Fang,Wenxing Fang,Marco Fargetta,Dmitry Fedoseev,Li-Cheng Feng,Qichun Feng,Richard Ford,Amélie Fournier,Haonan Gan,Feng Gao,Alberto Garfagnini,Arsenii Gavrikov,Marco Giammarchi,Agnese Giaz,Nunzio Giudice,Maxim Gonchar,Guanghua Gong,Hui Gong,Yuri Gornushkin,Alexandre Göttel,Marco Grassi,Christian Grewing,Vasily Gromov,Minghao Gu,Xiaofei Gu,Yu Gu,Mengyun Guan,Nunzio Guardone,Maria Gul,Cong Guo,Jingyuan Guo,Wanlei Guo,Xinheng Guo,Yuhang Guo,Paul Hackspacher,Caren Hagner,Ran Han,Yang Han,Muhammad Sohaib Hassan,Miao He,Wei He,Tobias Heinz,Patrick Hellmuth,Yuekun Heng,Rafael Herrera,YuenKeung Hor,Shaojing Hou,Yee Hsiung,Bei-Zhen Hu,Hang Hu

Journal

Chinese Physics C

Published Date

2023/11/1

The Jiangmen Underground Neutrino Observatory (JUNO) is a large liquid scintillator detector designed to explore many topics in fundamental physics. In this study, the potential of searching for proton decay in the

The Design and Technology Development of the JUNO Central Detector

Authors

Angel Abusleme,Thomas Adam,Shakeel Ahmad,Rizwan Ahmed,Sebastiano Aiello,Muhammad Akram,Abid Aleem,Tsagkarakis Alexandros,Fengpeng An,Qi An,Giuseppe Andronico,Nikolay Anfimov,Vito Antonelli,Tatiana Antoshkina,Burin Asavapibhop,João Pedro Athayde Marcondes de André,Didier Auguste,Weidong Bai,Nikita Balashov,Wander Baldini,Andrea Barresi,Davide Basilico,Eric Baussan,Marco Bellato,Marco Beretta,Antonio Bergnoli,Daniel Bick,Thilo Birkenfeld,David Blum,Simon Blyth,Anastasia Bolshakova,Mathieu Bongrand,Clément Bordereau,Dominique Breton,Augusto Brigatti,Riccardo Brugnera,Riccardo Bruno,Antonio Budano,Jose Busto,Anatael Cabrera,Barbara Caccianiga,Hao Cai,Xiao Cai,Yanke Cai,Zhiyan Cai,Stéphane Callier,Antonio Cammi,Agustin Campeny,Chuanya Cao,Guofu Cao,Jun Cao,Rossella Caruso,Cédric Cerna,Vanessa Cerrone,Chi Chan,Jinfan Chang,Yun Chang,Guoming Chen,Pingping Chen,Shaomin Chen,Yixue Chen,Yu Chen,Zhiyuan Chen,Zikang Chen,Jie Cheng,Yaping Cheng,Yu Chin Cheng,Alexander Chepurnov,Alexey Chetverikov,Davide Chiesa,Pietro Chimenti,Ziliang Chu,Artem Chukanov,Gérard Claverie,Catia Clementi,Barbara Clerbaux,Marta Colomer Molla,Selma Conforti Di Lorenzo,Alberto Coppi,Daniele Corti,Flavio Dal Corso,Olivia Dalager,Christophe de la Taille,Zhi Deng,Ziyan Deng,Wilfried Depnering,Marco Diaz,Xuefeng Ding,Yayun Ding,Bayu Dirgantara,Sergey Dmitrievsky,Tadeas Dohnal,Dmitry Dolzhikov,Georgy Donchenko,Jianmeng Dong,Evgeny Doroshkevich,Wei Dou,Marcos Dracos,Frédéric Druillole,Ran Du,Shuxian Du,Stefano Dusini,Hongyue Duyang,Timo Enqvist,Andrea Fabbri,Ulrike Fahrendholz,Lei Fan,Jian Fang,Wenxing Fang,Marco Fargetta,Dmitry Fedoseev,Zhengyong Fei,Li-Cheng Feng,Qichun Feng,Federico Ferraro,Amélie Fournier,Haonan Gan,Feng Gao,Alberto Garfagnini,Arsenii Gavrikov,Marco Giammarchi,Nunzio Giudice,Maxim Gonchar,Guanghua Gong,Hui Gong,Yuri Gornushkin,Alexandre Göttel,Marco Grassi,Maxim Gromov,Vasily Gromov,Minghao Gu,Xiaofei Gu,Yu Gu,Mengyun Guan,Yuduo Guan,Nunzio Guardone,Cong Guo,Wanlei Guo,Xinheng Guo,Yuhang Guo,Caren Hagner,Ran Han,Yang Han,Jiajun Hao,Miao He,Wei He,Tobias Heinz,Patrick Hellmuth,Yuekun Heng,Rafael Herrera

Published Date

2023/12/12

Authors

Adam Abed Abud,Pierre Granger,Henrique Vieira de Souza,Peter Cooke,Pierre Baldi,Marcelo Antoniassi,Silvia Pascoli,Bryan Ramson,Nikolozi Tsverava,Zahra Ghorbani-Moghaddam,John Learned,David Warner,Gregory Michna,Catia Petta,David Payne,Eric Zimmerman,Stefano Di Falco,Wayne Barkhouse,Laura Zambelli,Alexander Bitadze,Matheus Hostert,Edward Blucher,Simone Biagi,Daisy Kalra,Andrew Lawrence,Sandeep Miryala,Tom Lord,Keith Gollwitzer,Joshua Barrow,Nicola Delmonte,Nicolas Geffroy,Carmen Giugliano,Hugh Gallagher,Brian Rebel,Adrian Thompson,Federico Ferraro,Giuseppe Cerati,Mark Adamowski,Guillermo Palacio,Atanu Nath,Andrea Falcone,Luis Montaño Zetina,Paul Smith,Stephen Gent,Alessandro Thea,Biswaranjan Behera,Carlos Senise Jr,Faiza Akbar,Kurtis Nishimura,Pablo Amedo,Luca Bomben,Matthew Kramer,Kunal Kothekar,Dmitry Fedoseev,Robert Zwaska,Sofia Andringa,Andrés Castillo,Antonio Gioiosa,Simona Giovannella,Hirohisa Tanaka,Jack Fried,Johan Bremer,Francisco Nicolas-Arnaldos,Adam Lister,Piera Sapienza,Nicola McConkey,Jaroslaw Pasternak,Veljko Radeka,Niccolo Moggi,Douglas Benjamin,Nadine Kurita,Matthew Wetstein,Yasaman Farzan,Wei Mu,Anibal Bezerra,Ka Vang Tsang,Elena Gramellini,Olivia Dalager,Dario Autiero,Wenlong Yuan,A Rappoldi,Anthony Wood,Eric Guerard,Fabio Happacher,Emilija Pantic,Burak Bilki,Andrzej Szelc,Alfonso Madera,Ian Kotler,Steven Dytman,Niki Saoulidou,Elisabetta Pennacchio,Jose Valle,Daniele Montanino,Jeremy Wolcott,Andrew Mastbaum,Paul Keener,Jose Luis Rocabado Rocha,Grzegorz Deptuch,Quynh Vuong,Arseniy Rybnikov,Fabian Castaño Usuga,Matthew Worcester,Giacomo Scanavini,Yi Wang,Sabrina Sacerdoti,Shirley W Li,Morgan Wascko,Esteban Cristaldo,Liudmila Kolupaeva,Pierre Lasorak,Gavin Davies,Fatma Boran,Haiwang Yu,Marcelo Ismerio Oliveira,Avinay Bhat,EL Snider,Furkan Dolek,Antonis Papanestis,Konstantinos Manolopoulos,Diana Méndez,Mark Ross-Lonergan,Ornella Palamara,Letizia Di Giulio,Yuying Guo,Supraja Balasubramanian,Valerio Giusti,Steven Doran,Jovana Nikolov,Oleg Samoylov,AM Gago,Ryan Rivera,Edgar Rincón,Olga Gogota,Fernando Gardim,Michael Wang,James Matthews,David Martinez Caicedo,Giorgio Riccobene,Yanou Cui,James Stewart,Karolina Wresilo,Joseph Walsh,Terri Shaw,Vladimir Savinov,Guanqun Ge,Evgueni Goudzovski,Ina Sarcevic,Kevin Kelly,Diana Leon Silverio

Published Date

2023/12/5

Authors

A Abed Abud,B Abi,R Acciarri,MA Acero,MR Adames,G Adamov,M Adamowski,D Adams,M Adinolfi,C Adriano,A Aduszkiewicz,J Aguilar,Z Ahmad,J Ahmed,B Aimard,F Akbar,B Ali-Mohammadzadeh,K Allison,S Alonso Monsalve,M AlRashed,C Alt,A Alton,R Alvarez,P Amedo,J Anderson,C Andreopoulos,M Andreotti,M Andrews,F Andrianala,S Andringa,N Anfimov,A Ankowski,M Antoniassi,M Antonova,A Antoshkin,S Antusch,A Aranda-Fernandez,L Arellano,LO Arnold,MA Arroyave,J Asaadi,L Asquith,A Aurisano,V Aushev,D Autiero,V Ayala Lara,M Ayala-Torres,F Azfar,A Back,H Back,JJ Back,C Backhouse,I Bagaturia,L Bagby,N Balashov,S Balasubramanian,P Baldi,B Baller,B Bambah,F Barao,G Barenboim,G Barker,W Barkhouse,C Barnes,G Barr,J Barranco Monarca,A Barros,N Barros,JL Barrow,A Basharina-Freshville,A Bashyal,V Basque,C Batchelor,J Battat,F Battisti,F Bay,MCQ Bazetto,JL Bazo Alba,JF Beacom,E Bechetoille,B Behera,E das Chagas,L Bellantoni,G Bellettini,V Bellini,O Beltramello,N Benekos,C Benitez Montiel,F Bento Neves,J Berger,S Berkman,P Bernardini,RM Berner,A Bersani,S Bertolucci,M Betancourt,A Betancur Rodríguez,A Bevan,Y Bezawada,AT Bezerra,TJ Bezerra,A Bhardwaj,V Bhatnagar,M Bhattacharjee,D Bhattarai,S Bhuller,B Bhuyan,S Biagi,J Bian,M Biassoni,K Biery,B Bilki,M Bishai,A Bitadze,A Blake,FDM Blaszczyk,GC Blazey,E Blucher,J Boissevain,S Bolognesi,T Bolton,L Bomben,M Bonesini,C Bonilla-Diaz,F Bonini,A Booth,F Boran,S Bordoni,A Borkum,N Bostan,P Bour,D Boyden,J Bracinik,D Braga,D Brailsford,A Branca,A Brandt,J Bremer,C Brew,SJ Brice,C Brizzolari,C Bromberg,J Brooke,A Bross,G Brunetti,M Brunetti,N Buchanan,H Budd,I Butorov,I Cagnoli

Journal

European Physical Journal C

Published Date

2023/7

Sub-percent precision measurement of neutrino oscillation parameters with JUNO

Authors

Angel Abusleme,Thomas Adam,Shakeel Ahmad,Rizwan Ahmed,Sebastiano Aiello,Muhammad Akram,Abid Aleem,Fengpeng An,Qi An,Giuseppe Andronico,Nikolay Anfimov,Vito Antonelli,Tatiana Antoshkina,Burin Asavapibhop,João Pedro Athayde Marcondes de André,Didier Auguste,Weidong Bai,Nikita Balashov,Wander Baldini,Andrea Barresi,Davide Basilico,Eric Baussan,Marco Bellato,Antonio Bergnoli,Thilo Birkenfeld,Sylvie Blin,David Blum,Simon Blyth,Anastasia Bolshakova,Mathieu Bongrand,Clément Bordereau,Dominique Breton,Augusto Brigatti,Riccardo Brugnera,Riccardo Bruno,Antonio Budano,Jose Busto,Ilya Butorov,Anatael Cabrera,Barbara Caccianiga,Hao Cai,Xiao Cai,Yanke Cai,Zhiyan Cai,Riccardo Callegari,Antonio Cammi,Agustin Campeny,Chuanya Cao,Guofu Cao,Jun Cao,Rossella Caruso,Cédric Cerna,Chi Chan,Jinfan Chang,Yun Chang,Guoming Chen,Pingping Chen,Po-An Chen,Shaomin Chen,Xurong Chen,Yixue Chen,Yu Chen,Zhiyuan Chen,Zikang Chen,Jie Cheng,Yaping Cheng,Yu Chin Cheng,Alexey Chetverikov,Davide Chiesa,Pietro Chimenti,Artem Chukanov,Gérard Claverie,Catia Clementi,Barbara Clerbaux,Selma Conforti Di Lorenzo,Daniele Corti,Flavio Dal Corso,Olivia Dalager,Christophe De La Taille,Zhi Deng,Ziyan Deng,Wilfried Depnering,Marco Diaz,Xuefeng Ding,Yayun Ding,Bayu Dirgantara,Sergey Dmitrievsky,Tadeas Dohnal,Dmitry Dolzhikov,Georgy Donchenko,Jianmeng Dong,Evgeny Doroshkevich,Marcos Dracos,Frédéric Druillole,Ran Du,Shuxian Du,Stefano Dusini,Martin Dvorak,Timo Enqvist,Heike Enzmann,Andrea Fabbri,Donghua Fan,Lei Fan,Jian Fang,Wenxing Fang,Marco Fargetta,Dmitry Fedoseev,Zhengyong Fei,Li-Cheng Feng,Qichun Feng,Richard Ford,Amélie Fournier,Haonan Gan,Feng Gao,Alberto Garfagnini,Arsenii Gavrikov,Marco Giammarchi,Nunzio Giudice,Maxim Gonchar,Guanghua Gong,Hui Gong,Yuri Gornushkin,Alexandre Göttel,Marco Grassi,Vasily Gromov,Minghao Gu,Xiaofei Gu,Yu Gu,Mengyun Guan,Yuduo Guan,Nunzio Guardone,Cong Guo,Jingyuan Guo,Wanlei Guo,Xinheng Guo,Yuhang Guo,Paul Hackspacher,Caren Hagner,Ran Han,Yang Han,Miao He,Wei He,Tobias Heinz,Patrick Hellmuth,Yuekun Heng,Rafael Herrera,YuenKeung Hor,Shaojing Hou,Yee Hsiung,Bei-Zhen Hu

Journal

Chinese Physics C

Published Date

2022/12/1

JUNO is a multi-purpose neutrino observatory under construction in the south of China. This publication presents new sensitivity estimates for the measurement of the

Joint Determination of Reactor Antineutrino Spectra from and Fission by Daya Bay and PROSPECT

Authors

FP An,M Andriamirado,AB Balantekin,HR Band,CD Bass,DE Bergeron,D Berish,M Bishai,S Blyth,NS Bowden,CD Bryan,GF Cao,J Cao,JF Chang,Y Chang,HS Chen,SM Chen,Y Chen,YX Chen,J Cheng,ZK Cheng,JJ Cherwinka,MC Chu,T Classen,AJ Conant,JP Cummings,O Dalager,G Deichert,A Delgado,FS Deng,YY Ding,MV Diwan,T Dohnal,MJ Dolinski,D Dolzhikov,J Dove,M Dvořák,DA Dwyer,A Erickson,BT Foust,JK Gaison,A Galindo-Uribarri,JP Gallo,CE Gilbert,M Gonchar,GH Gong,H Gong,M Grassi,WQ Gu,JY Guo,L Guo,XH Guo,YH Guo,Z Guo,RW Hackenburg,S Hans,AB Hansell,M He,KM Heeger,B Heffron,YK Heng,YK Hor,YB Hsiung,BZ Hu,JR Hu,T Hu,ZJ Hu,HX Huang,JH Huang,XT Huang,YB Huang,P Huber,J Koblanski,DE Jaffe,S Jayakumar,KL Jen,XL Ji,XP Ji,RA Johnson,DC Jones,L Kang,SH Kettell,S Kohn,M Kramer,O Kyzylova,CE Lane,TJ Langford,J LaRosa,J Lee,JHC Lee,RT Lei,R Leitner,JKC Leung,F Li,HL Li,JJ Li,QJ Li,RH Li,S Li,SC Li,WD Li,XN Li,XQ Li,YF Li,ZB Li,H Liang,CJ Lin,GL Lin,S Lin,JJ Ling,JM Link,L Littenberg,BR Littlejohn,JC Liu,JL Liu,JX Liu,C Lu,HQ Lu,X Lu,KB Luk,BZ Ma,XB Ma,XY Ma,YQ Ma,RC Mandujano,J Maricic,C Marshall,KT McDonald,RD McKeown,MP Mendenhall,Y Meng,AM Meyer,R Milincic,PE Mueller,HP Mumm,J Napolitano,D Naumov,E Naumova,R Neilson,TMT Nguyen,JA Nikkel,S Nour,JP Ochoa-Ricoux,A Olshevskiy,JL Palomino,H-R Pan,J Park,S Patton,JC Peng,CSJ Pun

Journal

Physical review letters

Published Date

2022/2/22

Authors

A Abed Abud,A Friedland,M Smy,P Hamacher-Baumann,Z Djurcic,E Goudzovski,D Totani,I Katsioulas,C Densham,B Russell,E Calvo,P Green,A Penzo,D Shooltz,D Blend,L Singh,J Crnkovic,P Vahle,CS Mishra,MA Acero,H Meyer,DH Koh,D Moretti,G Cerati,M Adamowski,J Zennamo,AS Dyshkant,R Gran,J Stewart,D Marfatia,J Tamara,T Patzak,C Pernas,A Thompson,K Yonehara,JBR Battat,D Kwak,P Dunne,C Brizzolari,K Cho,R Rivera,G Lehmann Miotto,H Newton,C Mariani,S Vallecorsa,S Prakash,IK Furic,A Gabrielli,A Ankowski,PC De Holanda,A Barros,C Benitez Montiel,S Sacerdoti,E Smith,P Keener,X Wang,V Pec,O Palamara,JC Carceller,J Brooke,P Lasorak,CA Moura,A De la Torre,MA Delgado,E Guerard,W Ketchum,C Petta,G Miller,Z Hulcher,DA Dwyer,LW Koerner,J Maalmi,B Szczerbinska,V Tishchenko,A Thea,JRT de Mello Neto,T Gamble,J Matthews,K Moffat,F Muheim,M Chen,L Di Giulio,I Kotler,K Dugas,R Cross,T Cai,GC Blazey,P Novella,B Howard,L Jiang,N Talukdar,A Laundrie,L Suter,MHLS Wang,A Robert,J Soto-Oton,J Kvasnicka,X Ji,Y Onel,N Carrara,H Duyang,A De Roeck,J Franc,A Gago,D Last,J Bhambure,JWF Valle,P De Almeida,V Papadimitriou,Y Suvorov,C Thorn,S Uzunyan,S Manly,F Matichard,D Carber,L Paulucci,T Junk,S Copello,F Di Capua,R Mohanta,G Barr,P Gauzzi,JLL Bazo Alba,S Dolan,SD Reitzner,LS Fajardo,F Psihas,J Heise,S Antusch,K Duffy,S Miryala,D Whittington,L Rochester,C Mossey,L Kolupaeva,N Samios,N Gallice,E Pennacchio,X Qian,E Parozzi,D Torbunov,S Rosauro-Alcaraz,C Wret,O Goodwin,M Worcester,N McConkey,S Gent,A Gallego-Ros,P Laycock,MP Decowski

Published Date

2022/11/2

Measurements of electrons from νe interactions are crucial for the Deep Underground Neutrino Experiment (DUNE) neutrino oscillation program, as well as searches for physics beyond the standard model, supernova neutrino detection, and solar neutrino measurements. This article describes the selection and reconstruction of low-energy (Michel) electrons in the ProtoDUNE-SP detector. ProtoDUNE-SP is one of the prototypes for the DUNE far detector, built and operated at CERN as a charged particle test beam experiment. A sample of lowenergy electrons produced by the decay of cosmic muons is selected with a purity of 95%. This sample is used to calibrate the low-energy electron energy scale with two techniques. An electron energy calibration based on a cosmic ray muon sample uses calibration constants derived from measured and simulated cosmic ray muon events. Another calibration technique makes use of the theoretically well-understood Michel electron energy spectrum to convert reconstructed charge to electron energy. In addition, the effects of detector response to lowenergy electron energy scale and its resolution including readout electronics threshold effects are quantified. Finally, the relation between the theoretical and reconstructed low-energy electron energy spectrum is derived and the energy resolution is characterized. The low-energy electron selection presented here accounts for about 75% of the total electron deposited energy. After the addition of missing energy using a Monte Carlo simulation, the energy resolution improves from about 40% to 25% at 50 MeV. These results are used to validate the expected …

Feasibility of detecting B8 solar neutrinos at JUNO

Authors

João Pedro Athayde Marcondes de André,Angel Abusleme,Thomas Adam,Shakeel Ahmad,Rizwan Ahmed,Sebastiano Aiello,Muhammad Akram,An Fengpeng,An Qi,Giuseppe Andronico,Nikolay Anfimov,Vito Antonelli,Tatiana Antoshkina,Burin Asavapibhop,Didier Auguste,Andrej Babic,Nikita Balashov,Wander Baldini,Andrea Barresi,Davide Basilico,Eric Baussan,Marco Bellato,Antonio Bergnoli,Thilo Birkenfeld,Sylvie Blin,David Blum,Simon Blyth,Anastasia Bolshakova,Mathieu Bongrand,Clément Bordereau,Dominique Breton,Augusto Brigatti,Riccardo Brugnera,Riccardo Bruno,Antonio Budano,Mario Buscemi,Jose Busto,Ilya Butorov,Anatael Cabrera,Hao Cai,Xiao Cai,Yanke Cai,Zhiyan Cai,Riccardo Callegari,Antonio Cammi,Agustin Campeny,Chuanya Cao,Guofu Cao,Jun Cao,Rossella Caruso,Cédric Cerna,Jinfan Chang,Yun Chang,Pingping Chen,Po-An Chen,Shaomin Chen,Xurong Chen,Yi-Wen Chen,Yixue Chen,Yu Chen,Zhang Chen,Jie Cheng,Yaping Cheng,Alexey Chetverikov,Davide Chiesa,Pietro Chimenti,Artem Chukanov,Gérard Claverie,Catia Clementi,Barbara Clerbaux,Selma CONFORTI DI LORENZO,Daniele Corti,Flavio Dal Corso,Olivia Dalager,Christophe De La Taille,Jiawei Deng,Zhi Deng,Ziyan Deng,Wilfried Depnering,Marco Diaz,Xuefeng Ding,Yayun Ding,Bayu Dirgantara,Sergey Dmitrievsky,Tadeas Dohnal,Dmitry Dolzhikov,Georgy Donchenko,Jianmeng Dong,Evgeny Doroshkevich,Marcos Dracos,Frédéric Druillole,Du Ran,Du Shuxian,Stefano Dusini,Martin Dvorak,Timo Enqvist,Heike Enzmann,Andrea Fabbri,Lukas Fajt,Donghua Fan,Lei Fan,Jian Fang,Wenxing Fang,Marco Fargetta,Dmitry Fedoseev,Vladko Fekete,Li-Cheng Feng,Qichun Feng,Richard Ford,Amélie Fournier,Haonan Gan,Feng Gao,Alberto Garfagnini,Arsenii Gavrikov,Marco Giammarchi,Agnese Giaz,Nunzio Giudice,Maxim Gonchar,Guanghua Gong,Hui Gong,Yuri Gornushkin,Alexandre Sébastien Göttel,Marco Grassi,Christian Grewing,Vasily Gromov,Gu Minghao,Gu Xiaofei,Gu Yu,Mengyun Guan,Nunzio Guardone,Maria Gul,Cong Guo,Jingyuan Guo,Wanlei Guo,Xinheng Guo,Yuhang Guo,Paul Hackspacher,Caren Hagner,Ran Han,Yang Han,Muhammad Sohaib Hassan,He Miao,He Wei,Tobias Heinz,Patrick Hellmuth,Yuekun Heng,Rafael Herrera,Yuenkeung Hor,Shaojing Hou,Yee Bob Hsiung

Journal

POS PROCEEDINGS OF SCIENCE

Published Date

2022

The Jiangmen Underground Neutrino Observatory (JUNO) features a 20 kt multi-purpose underground liquid scintillator sphere as its main detector. In this talk we describe in detail a comprehensive assessment of JUNO's potential for detecting 8B solar neutrinos via the neutrino-electron elastic scattering process. A reduced 2 MeV threshold for the recoil electron energy is achievable with optimized background reduction strategies. With ten years of data taking, about 60,000 signal and 30,000 background events are expected. This leads to a simultaneous measurement of sin2θ12 and Δm221 using reactor antineutrinos and solar neutrinos in the JUNO detector. This large sample will enable an examination of the distortion of the recoil electron spectrum that is dominated by the neutrino flavor transformation in the dense solar matter. If Δm221= 4.8× 10− 5 (7.5× 10− 5eV2), JUNO can provide evidence of neutrino oscillation in the Earth at approximately the 3σ (2σ) level by measuring the non-zero signal rate variation with respect to the solar zenith angle. Moreover, JUNO can simultaneously measure Δm221 using 8B solar neutrinos to a precision of 20% or better, depending on the central value, and to sub-percent precision using reactor antineutrinos. A comparison of these two measurements from the same detector will help understand the current mild inconsistency between the value of reported by solar neutrino experiments and the KamLAND experiment.

arXiv: A Gaseous Argon-Based Near Detector to Enhance the Physics Capabilities of DUNE

Authors

A Abed Abud,A Friedland,M Smy,P Hamacher-Baumann,Z Djurcic,E Goudzovski,D Totani,E Mazzucato,C Densham,B Russell,E Calvo,P Green,A Penzo,D Shooltz,L Singh,J Crnkovic,P Vahle,CS Mishra,J Smolik,MA Acero,H Meyer,DH Koh,D Moretti,G Cerati,M Adamowski,J Zennamo,AS Dyshkant,R Gran,J Stewart,D Marfatia,T Patzak,K Yonehara,JBR Battat,D Kwak,P Dunne,C Brizzolari,K Cho,G Lehmann Miotto,H Newton,C Mariani,S Vallecorsa,S Prakash,IK Furic,A Gabrielli,A Ankowski,PC De Holanda,A Barros,C Benitez Montiel,S Sacerdoti,E Smith,P Keener,X Wang,V Pec,O Palamara,L Strigari,J Brooke,P Rosier,P Lasorak,CA Moura,MA Delgado,E Guerard,W Ketchum,C Petta,G Miller,Z Hulcher,DA Dwyer,LW Koerner,J Maalmi,B Szczerbinska,V Tishchenko,A Thea,JRT de Mello Neto,T Gamble,J Matthews,K Moffat,F Muheim,M Chen,L Di Giulio,F Battisti,R Cross,T Cai,GC Blazey,P Novella,B Howard,S Prince,V Ayala Lara,N Talukdar,A Laundrie,L Suter,MHLS Wang,A Robert,FDM Blaszczyk,J Kvasnicka,X Ji,Y Onel,J Nesbit,H Duyang,A De Roeck,J Franc,A Gago,D Last,K Nishimura,JWF Valle,V Papadimitriou,Y Suvorov,C Thorn,S Uzunyan,S Manly,F Matichard,D Carber,L Paulucci,T Junk,S Copello,F Di Capua,R Mohanta,G Barr,P Gauzzi,B Lunday,S Dolan,SD Reitzner,LS Fajardo,F Psihas,J Heise,S Antusch,P Clarke,S Miryala,H Mendez,L Rochester,K Fahey,C Mossey,L Kolupaeva,N Samios,N Gallice,E Pennacchio,X Qian,E Parozzi,D Torbunov,S Rosauro-Alcaraz,C Wret,M Fernandez Morales,O Goodwin,M Worcester,N McConkey,S Gent,A Gallego-Ros,MP Decowski,M Kirby,ED Zimmerman,A Surdo,L Da Silva Peres

Published Date

2022/3/11

The Deep Underground Neutrino Experiment (DUNE) is a next-generation international particle physics experiment seeking to answer fundamental questions about the neutrino. It will use a new high-intensity neutrino beam that will be generated at the US Department of Energy’s Fermi National Accelerator Laboratory (Fermilab). The experiment will consist of a far detector (FD) located approximately 1.5 km underground at the Sanford Underground Research Facility (SURF) in Lead, South Dakota, at a distance of 1285 km from Fermilab, and a near detector (ND) that will be located on the Fermilab site in Illinois. The FD will consist of a large, modular liquid-argon time projection chamber (LArTPC) with a fiducial mass of roughly 40 kt (total mass of 68 kton).The reference ND will be located approximately 574 m from DUNE’s neutrino target, which is the starting point for the Long-Baseline Neutrino Facility (LBNF) beam. The conceptual design for the DUNE ND is described in detail in Ref.[2]. The reference ND design consists of several different components shown in Fig. 1: an upstream modular non-magnetized LArTPC (ND-LAr), a magnetized tracker containing a pressurized gaseous-argon time projection chamber (ND-GAr), and a large, magnetized tracking spectrometer (SAND). SAND will remain fixed on the beam axis, while ND-LAr and ND-GAr will move transverse to the beam to collect data at various off-axis positions, providing different neutrino energy spectra by the PRISM concept [3]. In a conventional neutrino beam, the peak energy of the neutrino spectrum decreases and the size of the high energy tail is reduced when the detection …

Low exposure long-baseline neutrino oscillation sensitivity of the DUNE experiment

Authors

A Abed Abud,B Abi,R Acciarri,MA Acero,MR Adames,G Adamov,D Adams,M Adinolfi,A Aduszkiewicz,J Aguilar,Z Ahmad,J Ahmed,B Aimard,B Ali-Mohammadzadeh,T Alion,K Allison,S Alonso Monsalve,M AlRashed,C Alt,A Alton,P Amedo,J Anderson,C Andreopoulos,M Andreotti,MP Andrews,F Andrianala,S Andringa,N Anfimov,A Ankowski,M Antoniassi,M Antonova,A Antoshkin,S Antusch,A Aranda-Fernandez,LO Arnold,MA Arroyave,J Asaadi,L Asquith,A Aurisano,V Aushev,D Autiero,M Ayala-Torres,F Azfar,A Back,H Back,JJ Back,C Backhouse,I Bagaturia,L Bagby,N Balashov,S Balasubramanian,P Baldi,B Baller,B Bambah,F Barao,G Barenboim,GJ Barker,W Barkhouse,C Barnes,G Barr,J Barranco Monarca,A Barros,N Barros,JL Barrow,A Basharina-Freshville,A Bashyal,V Basque,E Belchior,JBR Battat,F Battisti,F Bay,JL Bazo Alba,JF Beacom,E Bechetoille,B Behera,L Bellantoni,G Bellettini,V Bellini,O Beltramello,N Benekos,C Benitez Montiel,F Bento Neves,J Berger,S Berkman,P Bernardini,RM Berner,S Bertolucci,M Betancourt,A Betancur Rodríguez,A Bevan,Y Bezawada,TJC Bezerra,A Bhardwaj,V Bhatnagar,M Bhattacharjee,S Bhuller,B Bhuyan,S Biagi,J Bian,M Biassoni,K Biery,B Bilki,M Bishai,A Bitadze,A Blake,FDM Blaszczyk,GC Blazey,E Blucher,J Boissevain,S Bolognesi,T Bolton,L Bomben,M Bonesini,M Bongrand,C Bonilla-Diaz,F Bonini,A Booth,F Boran,S Bordoni,A Borkum,N Bostan,P Bour,C Bourgeois,D Boyden,J Bracinik,D Braga,D Brailsford,A Branca,A Brandt,J Bremer,C Brew,SJ Brice,C Brizzolari,C Bromberg,J Brooke,A Bross,G Brunetti,M Brunetti,N Buchanan,H Budd,I Butorov,I Cagnoli,D Caiulo,R Calabrese,P Calafiura,J Calcutt,M Calin,S Calvez,E Calvo,A Caminata

Journal

Physical Review D

Published Date

2022/4/25

The Deep Underground Neutrino Experiment (DUNE) will produce world-leading neutrino oscillation measurements over the lifetime of the experiment. In this work, we explore DUNE’s sensitivity to observe charge-parity violation (CPV) in the neutrino sector, and to resolve the mass ordering, for exposures of up to 100 kiloton-megawatt-calendar years (kt-MW-CY), where calendar years include an assumption of 57% accelerator uptime based on past accelerator performance at Fermilab. The analysis includes detailed uncertainties on the flux prediction, the neutrino interaction model, and detector effects. We demonstrate that DUNE will be able to unambiguously resolve the neutrino mass ordering at a 4 σ (5 σ) level with a 66 (100) kt-MW-CY far detector exposure, and has the ability to make strong statements at significantly shorter exposures depending on the true value of other oscillation parameters, with a …

arXiv: Highly-parallelized simulation of a pixelated LArTPC on a GPU

Authors

Adam Abed Abud,Roman Berner,Veronica De Leo,Sanjay Swain,Pierre Baldi,Marcelo Antoniassi,Silvia Pascoli,Bryan Ramson,Nikolozi Tsverava,Zahra Ghorbani-Moghaddam,John Learned,David Warner,Gregory Michna,Catia Petta,David Payne,Asma Hadef,Eric Zimmerman,Stefano Di Falco,Wayne Barkhouse,Laura Zambelli,Alexander Bitadze,Matheus Hostert,Edward Blucher,Simone Biagi,Edgar Valencia,Daisy Kalra,Andrew Lawrence,Sandeep Miryala,Tom Lord,Keith Gollwitzer,Joshua Barrow,Nicola Delmonte,Nicolas Geffroy,Hugh Gallagher,Francesco Tortorici,Brian Rebel,Tristan Schefke,Carlo Rubbia,Federico Ferraro,Giuseppe Cerati,Mark Adamowski,Guillermo Palacio,Guang Yang,Andrea Falcone,Luis Montaño Zetina,Stephen Gent,Alessandro Thea,Biswaranjan Behera,Carlos Senise Jr,Faiza Akbar,Kurtis Nishimura,Pablo Amedo,Luca Bomben,Vladyslav Legin,Giorgio Riccobene,Kunal Kothekar,Dmitry Fedoseev,Robert Zwaska,Sofia Andringa,Andrés Castillo,Antonio Gioiosa,Simona Giovannella,Anicézio Campanelli,Wallison Luiz,Jack Fried,Johan Bremer,Francisco Nicolas-Arnaldos,Panagiotis Englezos,Piera Sapienza,Nicola McConkey,Jaroslaw Pasternak,Niccolo Moggi,Douglas Benjamin,Nadine Kurita,Matthew Wetstein,Yasaman Farzan,Wei Mu,Anibal Bezerra,Laura Molina Bueno,Felipe Kamiya,Olivia Dalager,Dario Autiero,Wenlong Yuan,A Rappoldi,Anthony Wood,Eric Guerard,Fabio Happacher,Emilija Pantic,Burak Bilki,Pierce Weatherly,Alfonso Madera,Ian Kotler,Alessandra Tonazzo,Niki Saoulidou,S Reitzner,Evgueni Goudzovski,Daniele Montanino,Andrew Mastbaum,Paul Keener,Grzegorz Deptuch,Quynh Vuong,Arseniy Rybnikov,Michael Shamma,Giacomo Scanavini,Giuseppe Cavallaro,Carlos Benitez Montiel,Esteban Cristaldo,Liudmila Kolupaeva,Pierre Lasorak,Gavin Davies,Fatma Boran,Haiwang Yu,Marcelo Ismerio Oliveira,EL Snider,Furkan Dolek,Tony Hill,Antonis Papanestis,Konstantinos Manolopoulos,Diana Méndez,Mitchell Mote,Ornella Palamara,Kyle Zeug,Letizia Di Giulio,Jeremy Wolcott,Supraja Balasubramanian,Young Soo Yoon,Tomasz Wachala,Steven Doran,Jovana Nikolov,Oleg Samoylov,AM Gago,Haifa Rejeb Sfar,Edgar Rincón,Olga Gogota,James Whilhelmi,Michael Wang,James Matthews,David Martinez Caicedo,Daniel Boyden,Yanou Cui,James Stewart,Karolina Wresilo,Terri Shaw,Vladimir Savinov,Guanqun Ge,Cristovao Vilela,Will Flanagan,Manuel Alejandro Ramirez Delgado,Kevin Kelly,Simon Peeters

Published Date

2022/12/19

arXiv: Improved Measurement of the Evolution of the Reactor Antineutrino Flux and Spectrum at Daya Bay

Authors

FP An,XT Zhang,HK Xu,ZJ Zhang,ZP Zhang,JL Sun,CG White,BZ Hu,V Vorobel,YF Li,M Ye,S Li,L Zhou,XH Guo,SQ Zhang,Y Wang,JM Link,FY Zhang,JR Hu,JW Zhang,YY Ding,HL Zhuang,L Zhan,RA Johnson,ZM Wang,Y Zeng,J Cao,J Zhao,RH Li,JC Liu,H Gong,V Zavadskyi,Y-C Cheng,FS Deng,JL Zhang,JHC Lee,CG Yang,J Dove,W Wang,JX Liu,C Morales Reveco,YX Chen,X Wang,BL Young,HQ Lu,HS Chen,N Raper,ZJ Hu,L Kang,DA Dwyer,RC Mandujano,Z Guo,S Kohn,JP Ochoa-Ricoux,KL Jen,ZY Zhang,JH Zou,XN Li,M Bishai,ZZ Xing,J Lee,L Guo,SH Kettell,ZK Cheng,E Worcester,GL Lin,GH Gong,TMT Nguyen,J Napolitano,HY Wei,WD Li,XQ Li,Y Chang,B Russell,Q Wu,T Xue,M Qi,R Leitner,D Jones,J Park,MV Diwan,HZ Yu,HY Duyang,H Steiner,RZ Zhao,YF Wang,RT Lei,HY Chen,YQ Ma,B Viren,M Wang,X Qian,JP Cummings,J Cheng,ZY Yu,Y Meng,YM Zhang,JP Gallo,Y Han,DE Jaffe,XY Ma,XB Ma,S Blyth,S Lin,XL Ji,Y Chen,TJ Langford,R Rosero,B Roskovec,M Gonchar,K Treskov,W-H Tse,BB Yue,HH Zhang,QJ Li,GF Cao,T Tmej,DR Wu,YB Huang,BZ Ma,SC Li,P Huber,A Olshevskiy,E Naumova,KV Dugas,JJ Ling,HL Li,M Yeh,JKC Leung,S Patton,YZ Yang,YB Hsiung,AB Balantekin,ZQ Xie,MC Chu,NY Wang,LJ Wen,KT McDonald,L Littenberg,FZ Qi,SM Chen,KM Heeger,F Li,M Kramer,JF Chang,XP Ji,YH Guo,JL Liu,D Naumov,JC Peng

Published Date

2022/10/3

Reactor neutrino experiments play a crucial role in advancing our knowledge of neutrinos. A precise measurement of reactor electron antineutrino flux and spectrum evolution can be key inputs in improving the knowledge of neutrino mass and mixing as well as reactor nuclear physics and searching for physics beyond the standard model. In this work, the evolution of the flux and spectrum as a function of the reactor isotopic content is reported in terms of the inverse-beta-decay yield at Daya Bay with 1958 days of data and improved systematic uncertainties. These measurements are compared with two signature model predictions: the Huber-Mueller model based on the conversion method and the SM2018 model based on the summation method. The measured average flux and spectrum, as well as their evolution with the 239Pu fraction, are inconsistent with the predictions of the Huber-Mueller model. In contrast, the SM2018 model is shown to agree with the average flux and its evolution but fails to describe the energy spectrum. Altering the predicted IBD spectrum from 239Pu does not improve the agreement with the measurement for either model. The models can be brought into better agreement with the measurements if either the predicted spectrum due to 235U is changed or the predicted 235U, 238U, 239Pu, and 241Pu spectra are changed in equal measure

arXiv: DUNE Offline Computing Conceptual Design Report

Authors

Adam Abed Abud,Roman Berner,Veronica De Leo,Pierre Baldi,Marcelo Antoniassi,Silvia Pascoli,Bryan Ramson,Nikolozi Tsverava,Zahra Ghorbani-Moghaddam,John Learned,David Warner,Gregory Michna,Catia Petta,David Payne,Brandon White,Kate Scholberg,Wayne Barkhouse,Laura Zambelli,Alexander Bitadze,Matheus Hostert,Edward Blucher,DH Koh,Simone Biagi,Edgar Valencia,Daisy Kalra,Andrew Lawrence,Sandeep Miryala,Tom Lord,Keith Gollwitzer,Joshua Barrow,Nicola Delmonte,Nicolas Geffroy,Brian Rebel,Tristan Schefke,Carlo Rubbia,Asher Kaboth,NJ Spooner,Giuseppe Cerati,Mark Adamowski,Guillermo Palacio,Andrea Falcone,Michael Mooney,Stephen Gent,Alessandro Thea,Biswaranjan Behera,Carlos Senise Jr,Faiza Akbar,Kurtis Nishimura,Pablo Amedo,Luca Bomben,Vladyslav Legin,Giorgio Riccobene,Kunal Kothekar,Dmitry Fedoseev,Robert Zwaska,Sofia Andringa,Andrés Castillo,Antonio Gioiosa,JC Carceller,Anicézio Campanelli,Wallison Luiz,Jack Fried,Srishti Nagu,Johan Bremer,Francisco Nicolas-Arnaldos,Panagiotis Englezos,Piera Sapienza,Nicola McConkey,LW Koerner,Niccolo Moggi,Douglas Benjamin,Nadine Kurita,Matthew Wetstein,Yasaman Farzan,Wei Mu,Anibal Bezerra,Laura Molina Bueno,Felipe Kamiya,Olivia Dalager,Dario Autiero,Wenlong Yuan,A Rappoldi,Anthony Wood,Eric Guerard,Hirohisa Tanaka,Emilija Pantic,Burak Bilki,Pierce Weatherly,Alfonso Madera,Ian Kotler,Alessandra Tonazzo,Niki Saoulidou,Daniele Montanino,Andrew Mastbaum,Paul Keener,Grzegorz Deptuch,Quynh Vuong,Arseniy Rybnikov,Michael Shamma,Giacomo Scanavini,Giuseppe Cavallaro,LS Gomez Fajardo,Carlos Benitez Montiel,Esteban Cristaldo,Liudmila Kolupaeva,Pierre Lasorak,Gavin Davies,Fatma Boran,Marcelo Ismerio Oliveira,EL Snider,Furkan Dolek,Tony Hill,Antonis Papanestis,Konstantinos Manolopoulos,Diana Méndez,SD Reitzner,Mitchell Mote,Stephen White,Ornella Palamara,Letizia Di Giulio,Supraja Balasubramanian,Young Soo Yoon,Tomasz Wachala,Steven Doran,Jovana Nikolov,Oleg Samoylov,AM Gago,Haifa Rejeb Sfar,Edgar Rincón,Olga Gogota,James Whilhelmi,Michael Wang,James Matthews,David Martinez Caicedo,Daniel Boyden,Yanou Cui,James Stewart,Karolina Wresilo,Terri Shaw,Vladimir Savinov,Guanqun Ge,Cristovao Vilela,Andrey Bobyshev,Will Flanagan,Manuel Alejandro Ramirez Delgado,Kevin Kelly,Simon Peeters,Leigh Whitehead,Etienne Chardonnet,Stefania Bordoni

Published Date

2022/10/28

Potential of core-collapse supernova neutrino detection at JUNO

Authors

João Pedro Athayde Marcondes de André,Angel Abusleme,Thomas Adam,Shakeel Ahmad,Rizwan Ahmed,Sebastiano Aiello,Muhammad Akram,An Fengpeng,An Qi,Giuseppe Andronico,Nikolay Anfimov,Vito Antonelli,Tatiana Antoshkina,Burin Asavapibhop,Didier Auguste,Andrej Babic,Nikita Balashov,Wander Baldini,Andrea Barresi,Davide Basilico,Eric Baussan,Marco Bellato,Antonio Bergnoli,Thilo Birkenfeld,Sylvie Blin,David Blum,Simon Blyth,Anastasia Bolshakova,Mathieu Bongrand,Clément Bordereau,Dominique Breton,Augusto Brigatti,Riccardo Brugnera,Riccardo Bruno,Antonio Budano,Mario Buscemi,Jose Busto,Ilya Butorov,Anatael Cabrera,Hao Cai,Xiao Cai,Yanke Cai,Zhiyan Cai,Riccardo Callegari,Antonio Cammi,Agustin Campeny,Chuanya Cao,Guofu Cao,Jun Cao,Rossella Caruso,Cédric Cerna,Jinfan Chang,Yun Chang,Pingping Chen,Po-An Chen,Shaomin Chen,Xurong Chen,Yi-Wen Chen,Yixue Chen,Yu Chen,Zhang Chen,Jie Cheng,Yaping Cheng,Alexey Chetverikov,Davide Chiesa,Pietro Chimenti,Artem Chukanov,Gérard Claverie,Catia Clementi,Barbara Clerbaux,Selma CONFORTI DI LORENZO,Daniele Corti,Flavio Dal Corso,Olivia Dalager,Christophe De La Taille,Jiawei Deng,Zhi Deng,Ziyan Deng,Wilfried Depnering,Marco Diaz,Xuefeng Ding,Yayun Ding,Bayu Dirgantara,Sergey Dmitrievsky,Tadeas Dohnal,Dmitry Dolzhikov,Georgy Donchenko,Jianmeng Dong,Evgeny Doroshkevich,Marcos Dracos,Frédéric Druillole,Du Ran,Du Shuxian,Stefano Dusini,Martin Dvorak,Timo Enqvist,Heike Enzmann,Andrea Fabbri,Lukas Fajt,Donghua Fan,Lei Fan,Jian Fang,Wenxing Fang,Marco Fargetta,Dmitry Fedoseev,Vladko Fekete,Li-Cheng Feng,Qichun Feng,Richard Ford,Amélie Fournier,Haonan Gan,Feng Gao,Alberto Garfagnini,Arsenii Gavrikov,Marco Giammarchi,Agnese Giaz,Nunzio Giudice,Maxim Gonchar,Guanghua Gong,Hui Gong,Yuri Gornushkin,Alexandre Sébastien Göttel,Marco Grassi,Christian Grewing,Vasily Gromov,Gu Minghao,Gu Xiaofei,Gu Yu,Mengyun Guan,Nunzio Guardone,Maria Gul,Cong Guo,Jingyuan Guo,Wanlei Guo,Xinheng Guo,Yuhang Guo,Paul Hackspacher,Caren Hagner,Ran Han,Yang Han,Muhammad Sohaib Hassan,He Miao,He Wei,Tobias Heinz,Patrick Hellmuth,Yuekun Heng,Rafael Herrera,Yuenkeung Hor,Shaojing Hou,Yee Bob Hsiung

Journal

POS PROCEEDINGS OF SCIENCE

Published Date

Authors

C Awe,XT Zhang,N Giudice,HK Xu,IS Yeo,ZP Zhang,N Kutovskiy,BZ Hu,V Vorobel,DC Jones,JX Ye,S Li,HH Jia,B Zhuang,S Fargher,Y Yang,W Huo,J Borg,JW Zhang,F Petrucci,E Doroshkevich,SY Kim,L Sabarots,CY Yu,J Yoo,N Zaitseva,K Walkup,P Harrington,C Lombardo,M Wright,SCF Wong,A Broniatowski,ZM Wang,I Lippi,YW Chen,J Zhao,E Paolini,J Zhou,J Tang,M Pitt,D Stefanik,C Mariani,L Dumoulin,A Lubashevskiy,N Guardone,MY Pac,J Johnston,M Andriamirado,A Bonhomme,YX Chen,X Wang,J He,BL Young,P Poussot,M Giammarchi,YD Kim,T Subedi,A Babic,DW Mayer,ZY You,L Kang,DA Dwyer,J Maalmi,Z Guo,J Li,M Grassi,F Muheim,R Kaiser,ZY Zhang,V Antonelli,O Sramek,L Guo,HB Liu,HR Pan,A Haghighat,T Adam,P Hellmuth,YK Cai,X Ji,FY Zhao,RX Liu,AM Meyer,C Giunti,K Ni,A Mitra,C Metelko,K Nishimura,HN Gan,M Robens,D Corti,HM Lee,JS Lu,N Zafar,MA Tyra,YG Xie,T Lin,D Jones,G Varner,J Park,S Ahmad,S Dazeley,B Asavapibhop,SY Liu,X Chen,H Steiner,I Mitchell,YF Wang,ZY Deng,T Classen,RT Lei,YD Zeng,N Rodphai,A Watcharangkool,C Wiebusch,M Wang,X Qian,A Stahl,Y Pei,OA Akindele,A Krasnoperov,M Karagounis,S Monteil,X Lu,J Gribble,C Wysotzki,W He,YJ Mao,AB Yang,YM Zhang,K Stankevich,DE Jaffe,XB Ma,HLH Wong,C Sirignano,T Soldner,A Triossi,S Heine,XL Sun,JH Choi,TJ Langford,F Sawy,R Rosero,T Li,P Saggese,M Bergevin,K Treskov,Y Gu,A Erickson,V Kudryavtsev,A Druetzler

Published Date

2022/3/14

Nuclear reactors are uniquely powerful, abundant, and flavor-pure sources of antineutrinos that continue to play a vital role in the US neutrino physics program. The US reactor antineutrino physics community is a diverse interest group encompassing many detection technologies and many particle physics topics, including Standard Model and short-baseline oscillations, BSM physics searches, and reactor flux and spectrum modelling. The community’s aims offer strong complimentary with numerous aspects of the wider US neutrino program and have direct relevance to most of the topical sub-groups composing the Snowmass 2021 Neutrino Frontier. Reactor neutrino experiments also have a direct societal impact and have become a strong workforce and technology development pipeline for DOE National Laboratories and universities.This white paper, prepared as a submission to the Snowmass 2021 community organizing exercise, will survey the state of the reactor antineutrino physics field and summarize the ways in which current and future reactor antineutrino experiments can play a critical role in advancing the field of particle physics in the next decade. As it is directed towards the Snowmass 2021 Neutrino Frontier, Sections 4 through 9 are organized around specific Topical Groups within that Frontier, with the relevant Topical Group specified in each Section’s title. Finally, to enable quick reference to the document’s main themes, two to four ‘Key Takeaways’ are provided at the beginning of each Section.

First measurement of high-energy reactor antineutrinos at Daya Bay

Authors

FP An,WD Bai,AB Balantekin,M Bishai,S Blyth,GF Cao,J Cao,JF Chang,Y Chang,HS Chen,HY Chen,SM Chen,Y Chen,YX Chen,J Cheng,ZK Cheng,JJ Cherwinka,MC Chu,JP Cummings,O Dalager,FS Deng,YY Ding,MV Diwan,T Dohnal,D Dolzhikov,J Dove,DA Dwyer,JP Gallo,M Gonchar,GH Gong,H Gong,WQ Gu,JY Guo,L Guo,XH Guo,YH Guo,Z Guo,RW Hackenburg,S Hans,M He,KM Heeger,YK Heng,YK Hor,YB Hsiung,BZ Hu,JR Hu,T Hu,ZJ Hu,HX Huang,JH Huang,XT Huang,YB Huang,P Huber,DE Jaffe,KL Jen,XL Ji,XP Ji,RA Johnson,D Jones,L Kang,SH Kettell,S Kohn,M Kramer,TJ Langford,J Lee,JHC Lee,RT Lei,R Leitner,JKC Leung,F Li,HL Li,JJ Li,QJ Li,RH Li,S Li,SC Li,WD Li,XN Li,XQ Li,YF Li,ZB Li,H Liang,CJ Lin,GL Lin,S Lin,JJ Ling,JM Link,L Littenberg,BR Littlejohn,JC Liu,JL Liu,JX Liu,C Lu,HQ Lu,KB Luk,BZ Ma,XB Ma,XY Ma,YQ Ma,RC Mandujano,C Marshall,KT McDonald,RD McKeown,Y Meng,J Napolitano,D Naumov,E Naumova,TMT Nguyen,JP Ochoa-Ricoux,A Olshevskiy,H-R Pan,J Park,S Patton,JC Peng,CSJ Pun,FZ Qi,M Qi,X Qian,N Raper,J Ren,C Morales Reveco,R Rosero,B Roskovec,XC Ruan,H Steiner,JL Sun,T Tmej,K Treskov,W-H Tse,CE Tull,B Viren,V Vorobel,CH Wang,J Wang,M Wang,NY Wang,RG Wang,W Wang,X Wang,Y Wang,YF Wang,Z Wang,ZM Wang,HY Wei,LH Wei,LJ Wen,K Whisnant,CG White,HLH Wong,E Worcester

Journal

Physical review letters

Published Date

2022/7/18

Authors

Zhaokan Cheng,Jingbo Zhang,Wei Wang,Jiajie Ling

Published Date

2020

Five gravitational wave events labelled GW150914, GW151226, GW170104, GW170814 and GW170817 were observed by the Advanced LIGO detectors at the past two years, successively. A sensitive search for coincident neutrino in some neutrino experiments can provide an exciting opportunity of additional identification for GW sources. Without a observed signals, the sensitivity on 90% confidence level (C.L.) can be estimated by using the observed neutrino backgrounds. At Daya Bay, Double-CHOOZ, RENO, KamLand and Borexino experiment, the sensitivities on 90% C.L. are roughly located in a level of 2-3 events within a time window of 1000 s. With an assumption of a monochromatic spectrum of coincident neutrinos, the corresponding fluence upper limits on 90% C.L., ranging from ∼1014 to ∼108 cm−2, are obtained and found to mainly depend on the target mass and are inversely propotional to cross …

TAO conceptual design report: a precision measurement of the reactor antineutrino spectrum with sub-percent energy resolution

Authors

Angel Abusleme,Thomas Adam,Shakeel Ahmad,Sebastiano Aiello,Muhammad Akram,Nawab Ali,Fengpeng An,Guangpeng An,Qi An,Giuseppe Andronico,Nikolay Anfimov,Vito Antonelli,Tatiana Antoshkina,Burin Asavapibhop,João Pedro Athayde Marcondes de André,Didier Auguste,Andrej Babic,Wander Baldini,Andrea Barresi,Eric Baussan,Marco Bellato,Antonio Bergnoli,Enrico Bernieri,David Biare,Thilo Birkenfeld,Sylvie Blin,David Blum,Simon Blyth,Anastasia Bolshakova,Mathieu Bongrand,Clément Bordereau,Dominique Breton,Augusto Brigatti,Riccardo Brugnera,Antonio Budano,Mario Buscemi,Jose Busto,Ilya Butorov,Anatael Cabrera,Hao Cai,Xiao Cai,Yanke Cai,Zhiyan Cai,Antonio Cammi,Agustin Campeny,Chuanya Cao,Guofu Cao,Jun Cao,Rossella Caruso,Cédric Cerna,Irakli Chakaberia,Jinfan Chang,Yun Chang,Pingping Chen,Po-An Chen,Shaomin Chen,Shenjian Chen,Xurong Chen,Yi-Wen Chen,Yixue Chen,Yu Chen,Zhang Chen,Jie Cheng,Yaping Cheng,Alexander Chepurnov,Davide Chiesa,Pietro Chimenti,Artem Chukanov,Anna Chuvashova,Gérard Claverie,Catia Clementi,Barbara Clerbaux,Selma Conforti Di Lorenzo,Daniele Corti,Salvatore Costa,Flavio Dal Corso,Christophe De La Taille,Jiawei Deng,Zhi Deng,Ziyan Deng,Wilfried Depnering,Marco Diaz,Xuefeng Ding,Yayun Ding,Bayu Dirgantara,Sergey Dmitrievsky,Tadeas Dohnal,Georgy Donchenko,Jianmeng Dong,Damien Dornic,Evgeny Doroshkevich,Marcos Dracos,Frédéric Druillole,Shuxian Du,Stefano Dusini,Martin Dvorak,Timo Enqvist,Heike Enzmann,Andrea Fabbri,Lukas Fajt,Donghua Fan,Lei Fan,Can Fang,Jian Fang,Anna Fatkina,Dmitry Fedoseev,Vladko Fekete,Li-Cheng Feng,Qichun Feng,Richard Ford,Andrey Formozov,Amélie Fournier,Haonan Gan,Feng Gao,Alberto Garfagnini,Alexandre Göttel,Christoph Genster,Marco Giammarchi,Agnese Giaz,Nunzio Giudice,Franco Giuliani,Maxim Gonchar,Guanghua Gong,Hui Gong,Oleg Gorchakov,Yuri Gornushkin,Marco Grassi,Christian Grewing,Maxim Gromov,Vasily Gromov,Minghao Gu,Xiaofei Gu,Yu Gu,Mengyun Guan,Nunzio Guardone,Maria Gul,Cong Guo,Jingyuan Guo,Wanlei Guo,Xinheng Guo,Yuhang Guo,Michael Haacke,Paul Hackspacher,Caren Hagner,Ran Han,Yang Han,Miao He,Wei He,Tobias Heinz,Patrick Hellmuth

Journal

arXiv preprint arXiv:2005.08745

Published Date

2020/5/18

The Taishan Antineutrino Observatory (TAO, also known as JUNO-TAO) is a satellite experiment of the Jiangmen Underground Neutrino Observatory (JUNO). A ton-level liquid scintillator detector will be placed at about 30 m from a core of the Taishan Nuclear Power Plant. The reactor antineutrino spectrum will be measured with sub-percent energy resolution, to provide a reference spectrum for future reactor neutrino experiments, and to provide a benchmark measurement to test nuclear databases. A spherical acrylic vessel containing 2.8 ton gadolinium-doped liquid scintillator will be viewed by 10 m^2 Silicon Photomultipliers (SiPMs) of >50% photon detection efficiency with almost full coverage. The photoelectron yield is about 4500 per MeV, an order higher than any existing large-scale liquid scintillator detectors. The detector operates at -50 degree C to lower the dark noise of SiPMs to an acceptable level. The detector will measure about 2000 reactor antineutrinos per day, and is designed to be well shielded from cosmogenic backgrounds and ambient radioactivities to have about 10% background-to-signal ratio. The experiment is expected to start operation in 2022.

The JUNO Central Detector Filling and Overflow System for the Liquid Scintillator

Authors

Shuaijie Li,Baobiao Yue,Jiajie Ling,Zhi Wu,Xiao Tang,Yuekun Heng,JUNO Collaboration

Published Date

2020

Authors

Baobiao Yue,Jiajie Ling,Wei Li,Fanrong Xu

Published Date

2020

The standard 3-flavor neutrino oscillation has been well established. However, some experimental hints suggest the existence of new types of neutrinos at mass of eV scale. Those sterile neutrinos will change the neutrino oscillation pattern for short-baseline neutrino experiments with the 3(active)+N(sterile) neutrino mixing framework. Recent proposed medium baseline reactor neutrino experiments are sensitive to those very light sterile neutrinos at 10−4 to 0.01 eV2 mass-squared difference through electron antineutrino disappearance channel. In this paper, we will discuss the matter effect correction on those very light sterile neutrino oscillation. As shown in our study, the matter effect correction for sterile neutrino oscillation is quite small (< 4%), and at the same scale as the 3-flavor active neutrino oscillation case.

Feasibility and physics potential of detecting B solar neutrinos at JUNO

Authors

Leonidas Kalousis,Xiaonan Li,Haonan Gan,Sergey Dmitrievsky,Konstantin Stankevich,Can Fang,Jaruchit Siripak,Xi Wang,Amélie Fournier,Hongtao Liu,Li Kang,Haifeng Yao,Yixue Chen,Tobias Heinz,Benda Xu,Tobias Sterr,Patrick Hellmuth,Haiqiong Zhang,Zhijian Zhang,Dmitry Fedoseev,Tao Zhang,Dmitry V Naumov,Vladko Fekete,Cristina Martellini,Mathieu Bongrand,Yan Zhang,Dus Stefanik,Michael Wurm,Enrico Bernieri,Hongbang Liu,Ondrej Sramek,Shun Zhou,Zhonghua Qin,Xiaomei Li,Yongjiu Shi,Guanghua Gong,Alexey Krasnoperov,Zongyi Wang,Yumei Zhang,Alexander Studenikin,Arseniy Rybnikov,David Biare,Shenjian Chen,Christophe De La Taille,Antonio Budano,Shubin Liu,Guoli Wang,Sukit Limpijumnong,Bei-Zhen Hu,Muhammad Shahzad,Hiroshi Nunokawa,Yongbo Huang,Chung-Hsiang Wang,Shengxin Lin,Wilfried Depnering,Guangpeng An,Bedřich Roskovec,Zhe Wang,Jie Zhao,Jose Busto,Ran Han,Fang Liu,Henning Rebber,Feiyang Zhang,Pengwei Luo,Roberto Isocrate,Andrey Sidorenkov,Xiaoshan Jiang,Pan Zeng,Xiaomei Zhang,Alexandre Göttel,Yufei Xi,Andrea Triossi,Vladimir Lyashuk,Chuanya Cao,Tomas Tmej,Franco Giuliani,Haitao Li,Barbara Ricci,Yu Gu,Nuanwan Sanguansak,Salvatore Costa,Michael Karagounis,Haidong Liu,Utane Sawangwit,Emanuela Meroni,Jing Zhou,Livia Ludhova,Yifang Wang,Wladyslaw Trzaska,Jie Cheng,Guillaume Vanroyen,Tobias Lachenmaier,Wenhao Huang,Alexey Lokhov,Lino Miramonti,Amir Khan,Dongqin Zheng,Jin Li,Pierre-Alexandre Petitjean,Chunxu Yu,Jun Hu,Konstantin Kouzakov,Barbara Clerbaux,Xuantong Zhang,Wei Wei,Max Buesken,Chuan Lu,Ezio Previtali,Frederic Lefevre,Maxim Gonchar,Agustin Campeny,Zhang Chen,Gisele Martin-Chassard,Pablo Walker,Runxuan Liu,Christoph Genster,Yadong Wei,Vasily Gromov,Zafar Yasin,Aldo Romani,Patrick Kinz,Xichao Ruan,Juan Pedro Ochoa-Ricoux,Nina Parkalian,Maciej Slupecki,Ming Qi,Dongmei Xia,Yangfu Wang,Alberto Garfagnini,Jie Yang,Caishen Wang,Stefano Dusini,Nikolay Kutovskiy,Stefan van Waasen,Sergio Parmeggiano,Konstantin Schweizer,Andrea Serafini,Taras Rezinko,Daojin Hong,Guofu Cao,Peihuai Yi,Qingjiang Li,Alexander Tietzsch,Marco Diaz,Monica Sisti,Boonrucksar Soonthornthum,Yaping Cheng,Xianghui Yu,Lei Yang

Published Date

2020

The Jiangmen Underground Neutrino Observatory~(JUNO) features a 20~ kt multi-purpose underground liquid scintillator sphere as its main detector. Some of JUNO's features make it an excellent experiment for B solar neutrino measurements, such as its low-energy threshold, its high energy resolution compared to water Cherenkov detectors, and its much large target mass compared to previous liquid scintillator detectors. In this paper we present a comprehensive assessment of JUNO's potential for detecting B solar neutrinos via the neutrino-electron elastic scattering process. A reduced 2~ MeV threshold on the recoil electron energy is found to be achievable assuming the intrinsic radioactive background U and Th in the liquid scintillator can be controlled to 10~ g/g. With ten years of data taking, about 60,000 signal and 30,000 background events are expected. This large sample will enable an examination of the distortion of the recoil electron spectrum that is dominated by the neutrino flavor transformation in the dense solar matter, which will shed new light on the tension between the measured electron spectra and the predictions of the standard three-flavor neutrino oscillation framework. If ~ eV , JUNO can provide evidence of neutrino oscillation in the Earth at the about 3~(2) level by measuring the non-zero signal rate variation with respect to the solar zenith angle. Moveover, JUNO can simultaneously measure using B solar neutrinos to a precision of 20\% or better depending on the central value and to sub-percent precision using reactor antineutrinos. A comparison of these two measurements …

Improved Constraints on Sterile Neutrino Mixing from Disappearance Searches in the MINOS, , Daya Bay, and Bugey-3 Experiments

Authors

P Adamson,FP An,I Anghel,A Aurisano,AB Balantekin,HR Band,G Barr,M Bishai,A Blake,S Blyth,GF Cao,J Cao,SV Cao,TJ Carroll,CM Castromonte,JF Chang,Y Chang,HS Chen,R Chen,SM Chen,Y Chen,YX Chen,J Cheng,ZK Cheng,JJ Cherwinka,S Childress,MC Chu,A Chukanov,JAB Coelho,JP Cummings,N Dash,S De Rijck,FS Deng,YY Ding,MV Diwan,T Dohnal,D Dolzhikov,J Dove,M Dvořák,DA Dwyer,JJ Evans,GJ Feldman,W Flanagan,M Gabrielyan,JP Gallo,S Germani,RA Gomes,M Gonchar,GH Gong,H Gong,P Gouffon,N Graf,K Grzelak,WQ Gu,JY Guo,L Guo,XH Guo,YH Guo,Z Guo,A Habig,RW Hackenburg,SR Hahn,S Hans,J Hartnell,R Hatcher,M He,KM Heeger,YK Heng,A Higuera,A Holin,YK Hor,YB Hsiung,BZ Hu,JR Hu,T Hu,ZJ Hu,HX Huang,J Huang,XT Huang,YB Huang,P Huber,DE Jaffe,KL Jen,XL Ji,XP Ji,RA Johnson,D Jones,L Kang,SH Kettell,LW Koerner,S Kohn,M Kordosky,M Kramer,A Kreymer,K Lang,TJ Langford,J Lee,JHC Lee,RT Lei,R Leitner,JKC Leung,F Li,HL Li,JJ Li,QJ Li,S Li,SC Li,SJ Li,WD Li,XN Li,XQ Li,YF Li,ZB Li,H Liang,CJ Lin,GL Lin,S Lin,JJ Ling,JM Link,L Littenberg,BR Littlejohn,JC Liu,JL Liu,Y Liu,YH Liu,C Lu,HQ Lu,JS Lu,P Lucas,KB Luk,XB Ma,XY Ma,YQ Ma,WA Mann,ML Marshak,C Marshall,DA Martinez Caicedo,N Mayer,KT McDonald,RD McKeown,R Mehdiyev,JR Meier,Y Meng,WH Miller,G Mills,L Mora Lepin,D Naples,J Napolitano,D Naumov,E Naumova

Journal

Physical Review Letters

Published Date

2020/8/10

Searches for electron antineutrino, muon neutrino, and muon antineutrino disappearance driven by sterile neutrino mixing have been carried out by the Daya Bay and MINOS+ collaborations. This Letter presents the combined results of these searches, along with exclusion results from the Bugey-3 reactor experiment, framed in a minimally extended four-neutrino scenario. Significantly improved constraints on the θ μ e mixing angle are derived that constitute the most constraining limits to date over five orders of magnitude in the mass-squared splitting Δ m 41 2, excluding the 90% CL sterile-neutrino parameter space allowed by the LSND and MiniBooNE observations at 90% CL s for Δ m 41 2< 13 eV 2. Furthermore, the LSND and MiniBooNE 99% CL allowed regions are excluded at 99% CL s for Δ m 41 2< 1.6 eV 2.

Research on Liquid Scintillator Energy Nonlinearity

Authors

Yuzi Yang,Jiajie Ling

Published Date

2020

Liquid scintillator(LS) calorimeter is a classical technology in the particle physics, especially for the reactor neutrino experiments, which is widely used for detecting electron anti-neutrinos though the inverse beta decay interaction channel. Because of the quenching effect, the scintillator detector has nonlinear energy response. It is critical to accurately measure the scintillator energy response for both the precision measurement of reactor antineutrino energy spectrum in Daya Bay Experiment and the neutrino mass hierarchy measurement determination in JUNO experiments. There are several bench measurements of the liquid scintillator energy nonlinearity response through the gamma-ray and the electron Compton scattering process. However, it is difficult to estimate the systematic uncertainties of those measurements are difficult to assess. In this paper, we used the Geant4 simulation package to study several …

Earliest Resolution to the Neutrino Mass Ordering?

Authors

Anatael Cabrera,Yang Han,Michel Obolensky,Fabien Cavalier,João Coelho,Diana Navas-Nicolás,Hiroshi Nunokawa,Laurent Simard,Jianming Bian,Nitish Nayak,Juan Pedro Ochoa-Ricoux,Bedřich Roskovec,Pietro Chimenti,Stefano Dusini,Marco Grassi,Mathieu Bongrand,Rebin Karaparambil,Victor Lebrin,Benoit Viaud,Frederic Yermia,Lily Asquith,Thiago JC Bezerra,Jeff Hartnell,Pierre Lasorak,Jiajie Ling,Jiajun Liao,Hongzhao Yu

Journal

arXiv preprint arXiv:2008.11280

Published Date

2020/8

We hereby illustrate and numerically demonstrate via a simplified proof of concept calculation tuned to the latest average neutrino global data that the combined sensitivity of JUNO with NOvA and T2K experiments has the potential to be the first fully resolved (≥ 5σ) measurement of neutrino Mass Ordering (MO) around 2028; tightly linked to the JUNO schedule. Our predictions account for the key ambiguities and the most relevant±1σ data fluctuations. In the absence of any concrete MO theoretical prediction and given its intrinsic binary outcome, we highlight the benefits of having such a resolved measurement in the light of the remarkable MO resolution ability of the next generation of long baseline neutrino beams experiments. We motivate the opportunity of exploiting the MO experimental framework to scrutinise the standard oscillation model, thus, opening for unique discovery potential, should unexpected discrepancies manifest. Phenomenologically, the deepest insight relies on the articulation of MO resolved measurements via at least the two possible methodologies matter effects and purely vacuum oscillations. Thus, we argue that the JUNO vacuum MO measurement may feasibly yield full resolution in combination to the next generation of long baseline neutrino beams experiments.The discovery of neutrino (ν) oscillations phenomenon have completed a remarkable scientific endeavour lasting several decades that has changed forever our understanding of the phenomenology of the leptonic sector of the standard model of elementary particles (SM). A few modifications were accommodated to account for the new phenomenon [1]. This …

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