Xiaofeng Wang

Xiaofeng Wang

Tsinghua University

H-index: 283

Asia-China

Professor Information

University

Tsinghua University

Position

Physics Department

Citations(all)

341203

Citations(since 2020)

177411

Cited By

113087

hIndex(all)

283

hIndex(since 2020)

185

i10Index(all)

1261

i10Index(since 2020)

1139

Email

University Profile Page

Tsinghua University

Research & Interests List

supernova

time-domain astronomy

AGN

Top articles of Xiaofeng Wang

New constraints on ultraheavy dark matter from the LZ experiment

Searches for dark matter with liquid xenon time projection chamber experiments have traditionally focused on the region of the parameter space that is characteristic of weakly interacting massive particles, ranging from a few GeV/ to a few TeV/. Models of dark matter with a mass much heavier than this are well motivated by early production mechanisms different from the standard thermal freeze-out, but they have generally been less explored experimentally. In this work, we present a re-analysis of the first science run (SR1) of the LZ experiment, with an exposure of tonneyear, to search for ultraheavy particle dark matter. The signal topology consists of multiple energy deposits in the active region of the detector forming a straight line, from which the velocity of the incoming particle can be reconstructed on an event-by-event basis. Zero events with this topology were observed after applying the data selection calibrated on a simulated sample of signal-like events. New experimental constraints are derived, which rule out previously unexplored regions of the dark matter parameter space of spin-independent interactions beyond a mass of 10 GeV/.

Authors

J Aalbers,DS Akerib,AK Al Musalhi,CS Amarasinghe,A Ames,TJ Anderson,N Angelides,HM Araújo,JE Armstrong,M Arthurs,A Baker,S Balashov,J Bang,JW Bargemann,A Baxter,K Beattie,T Benson,A Bhatti,A Biekert,TP Biesiadzinski,HJ Birch,E Bishop,GM Blockinger,B Boxer,CAJ Brew,P Brás,S Burdin,M Buuck,MC Carmona-Benitez,M Carter,A Chawla,H Chen,JJ Cherwinka,NI Chott,MV Converse,A Cottle,G Cox,D Curran,CE Dahl,A David,J Delgaudio,S Dey,L de Viveiros,C Ding,JEY Dobson,E Druszkiewicz,SR Eriksen,A Fan,NM Fearon,S Fiorucci,H Flaecher,ED Fraser,TMA Fruth,RJ Gaitskell,A Geffre,J Genovesi,C Ghag,R Gibbons,S Gokhale,J Green,MGD van der Grinten,CR Hall,S Han,E Hartigan-O'Connor,SJ Haselschwardt,SA Hertel,G Heuermann,GJ Homenides,M Horn,DQ Huang,D Hunt,CM Ignarra,E Jacquet,RS James,J Johnson,AC Kaboth,AC Kamaha,D Khaitan,A Khazov,I Khurana,J Kim,J Kingston,R Kirk,D Kodroff,L Korley,EV Korolkova,H Kraus,S Kravitz,L Kreczko,B Krikler,VA Kudryavtsev,J Lee,DS Leonard,KT Lesko,C Levy,J Lin,A Lindote,R Linehan,WH Lippincott,MI Lopes,E Lopez Asamar,W Lorenzon,C Lu,S Luitz,PA Majewski,A Manalaysay,RL Mannino,C Maupin,ME McCarthy,G McDowell,DN McKinsey,J McLaughlin,R McMonigle,EH Miller,E Mizrachi,A Monte,ME Monzani,JD Mendoza,E Morrison,BJ Mount,M Murdy,A St J Murphy,A Naylor,C Nedlik,HN Nelson,F Neves,A Nguyen,JA Nikoleyczik,I Olcina,KC Oliver-Mallory,J Orpwood,KJ Palladino,J Palmer,NJ Pannifer,N Parveen,SJ Patton,B Penning,G Pereira,E Perry,T Pershing,A Piepke,Y Qie,J Reichenbacher,CA Rhyne,Q Riffard,GRC Rischbieter,HS Riyat,R Rosero,T Rushton,D Rynders

Journal

arXiv preprint arXiv:2402.08865

Published Date

2024/2/14

Search for a CP-odd Higgs boson decaying into a heavy CP-even Higgs boson and a Z boson in the and final states using 140 fb−1 of data collected …

A search for a heavy CP-odd Higgs boson, A, decaying into a Z boson and a heavy CP-even Higgs boson, H, is presented. It uses the full LHC Run 2 dataset of pp collisions at s= 13 TeV collected with the ATLAS detector, corresponding to an integrated luminosity of 140 fb− 1. The search for A→ ZH is performed in the ℓ+ ℓ− tt and ννbb final states and surpasses the reach of previous searches in different final states in the region with mH> 350 GeV and mA> 800 GeV. No significant deviation from the Standard Model expectation is found. Upper limits are placed on the production cross-section times the decay branching ratios. Limits with less model dependence are also presented as functions of the reconstructed m (tt) and m (bb) distributions in the ℓ+ ℓ− tt and ννbb channels, respectively. In addition, the results are interpreted in the context of two-Higgs-doublet models.

Authors

G Aad,B Abbott,K Abeling,NJ Abicht,SH Abidi,A Aboulhorma,H Abramowicz,H Abreu,Y Abulaiti,BS Acharya,C Adam Bourdarios,L Adamczyk,SV Addepalli,MJ Addison,J Adelman,A Adiguzel,T Adye,AA Affolder,Y Afik,MN Agaras,J Agarwala,A Aggarwal,C Agheorghiesei,A Ahmad,F Ahmadov,WS Ahmed,S Ahuja,X Ai,G Aielli,A Aikot,M Ait Tamlihat,B Aitbenchikh,I Aizenberg,M Akbiyik,TPA Åkesson,AV Akimov,D Akiyama,NN Akolkar,S Aktas,K Al Khoury,GL Alberghi,J Albert,P Albicocco,GL Albouy,S Alderweireldt,M Aleksa,IN Aleksandrov,C Alexa,T Alexopoulos,F Alfonsi,M Algren,M Alhroob,B Ali,HMJ Ali,S Ali,SW Alibocus,M Aliev,G Alimonti,W Alkakhi,C Allaire,BMM Allbrooke,JF Allen,CA Allendes Flores,PP Allport,A Aloisio,F Alonso,C Alpigiani,M Alvarez Estevez,A Alvarez Fernandez,M Alves Cardoso,MG Alviggi,M Aly,Y Amaral Coutinho,A Ambler,C Amelung,M Amerl,CG Ames,D Amidei,SP Amor Dos Santos,KR Amos,V Ananiev,C Anastopoulos,T Andeen,JK Anders,SY Andrean,A Andreazza,S Angelidakis,A Angerami,AV Anisenkov,A Annovi,C Antel,MT Anthony,E Antipov,M Antonelli,F Anulli,M Aoki,T Aoki,JA Aparisi Pozo,MA Aparo,L Aperio Bella,C Appelt,A Apyan,N Aranzabal,SJ Arbiol Val,C Arcangeletti,ATH Arce,E Arena,JF Arguin,S Argyropoulos,J-H Arling,O Arnaez,H Arnold,G Artoni,H Asada,K Asai,S Asai,NA Asbah,K Assamagan,R Astalos,S Atashi,RJ Atkin,M Atkinson,H Atmani,PA Atmasiddha,K Augsten,S Auricchio,AD Auriol,VA Austrup,G Avolio,K Axiotis,G Azuelos,D Babal,H Bachacou,K Bachas,A Bachiu,F Backman,A Badea,TM Baer,P Bagnaia,M Bahmani,AJ Bailey,VR Bailey,JT Baines,L Baines,OK Baker,E Bakos,D Bakshi Gupta,V Balakrishnan,R Balasubramanian,EM Baldin

Published Date

2024/2/26

GWTC-2.1: Deep extended catalog of compact binary coalescences observed by LIGO and Virgo during the first half of the third observing run

The second Gravitational-Wave Transient Catalog, GWTC-2, reported on 39 compact binary coalescences observed by the Advanced LIGO and Advanced Virgo detectors between 1 April 2019 15∶ 00 UTC and 1 October 2019 15∶ 00 UTC. Here, we present GWTC-2.1, which reports on a deeper list of candidate events observed over the same period. We analyze the final version of the strain data over this period with improved calibration and better subtraction of excess noise, which has been publicly released. We employ three matched-filter search pipelines for candidate identification, and estimate the probability of astrophysical origin for each candidate event. While GWTC-2 used a false alarm rate threshold of 2 per year, we include in GWTC-2.1, 1201 candidates that pass a false alarm rate threshold of 2 per day. We calculate the source properties of a subset of 44 high-significance candidates that have a …

Authors

R Abbott,TD Abbott,F Acernese,K Ackley,C Adams,N Adhikari,RX Adhikari,VB Adya,C Affeldt,D Agarwal,M Agathos,K Agatsuma,N Aggarwal,OD Aguiar,L Aiello,A Ain,P Ajith,S Albanesi,A Allocca,PA Altin,A Amato,C Anand,S Anand,A Ananyeva,SB Anderson,WG Anderson,T Andrade,N Andres,T Andrić,SV Angelova,S Ansoldi,JM Antelis,S Antier,S Appert,K Arai,MC Araya,JS Areeda,M Arène,N Arnaud,SM Aronson,KG Arun,Y Asali,G Ashton,M Assiduo,SM Aston,P Astone,F Aubin,C Austin,S Babak,F Badaracco,MKM Bader,C Badger,S Bae,AM Baer,S Bagnasco,Y Bai,J Baird,M Ball,G Ballardin,SW Ballmer,A Balsamo,G Baltus,S Banagiri,D Bankar,JC Barayoga,C Barbieri,BC Barish,D Barker,P Barneo,F Barone,B Barr,L Barsotti,M Barsuglia,D Barta,J Bartlett,MA Barton,I Bartos,R Bassiri,A Basti,M Bawaj,JC Bayley,AC Baylor,M Bazzan,B Bécsy,VM Bedakihale,M Bejger,I Belahcene,V Benedetto,D Beniwal,TF Bennett,JD Bentley,M Benyaala,F Bergamin,BK Berger,S Bernuzzi,CPL Berry,D Bersanetti,A Bertolini,J Betzwieser,D Beveridge,R Bhandare,U Bhardwaj,D Bhattacharjee,S Bhaumik,IA Bilenko,G Billingsley,S Bini,R Birney,O Birnholtz,S Biscans,M Bischi,S Biscoveanu,A Bisht,B Biswas,M Bitossi,M-A Bizouard,JK Blackburn,CD Blair,DG Blair,RM Blair,F Bobba,N Bode,M Boer,G Bogaert,M Boldrini,LD Bonavena,F Bondu,E Bonilla,R Bonnand,P Booker,BA Boom,R Bork,V Boschi,N Bose,S Bose,V Bossilkov,V Boudart,Y Bouffanais,A Bozzi,C Bradaschia,PR Brady,A Bramley,A Branch,M Branchesi,JE Brau,M Breschi,T Briant,JH Briggs,A Brillet,M Brinkmann

Journal

Physical Review D

Published Date

2024/1/5

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

Daya Bay presents the first measurement of cosmogenic He isotope production in liquid scintillator, using an innovative method for identifying cascade decays of He and its child isotope, Li. We also measure the production yield of Li isotopes using well-established methodology. The results, in units of 10gcm, are 0.3070.042, 0.3410.040, and 0.5460.076 for He, and 6.730.73, 6.750.70, and 13.740.82 for Li at average muon energies of 63.9~GeV, 64.7~GeV, and 143.0~GeV, respectively. The measured production rate of He isotopes is more than an order of magnitude lower than any other measurement of cosmogenic isotope production. It replaces the results of previous attempts to determine the ratio of He to Li production that yielded a wide range of limits from 0 to 30\%. The results provide future liquid-scintillator-based experiments with improved ability to predict cosmogenic backgrounds.

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,YC Cheng,ZK Cheng,JJ Cherwinka,MC Chu,JP Cummings,O Dalager,FS Deng,XY Ding,YY Ding,MV Diwan,T Dohnal,D Dolzhikov,J Dove,KV Dugas,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,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,W-H Tse,CE Tull,YC Tung,B Viren,V Vorobel,CH Wang,J Wang,M Wang,NY Wang,RG Wang,W Wang,X Wang,YF Wang,Z Wang,ZM Wang,HY Wei,LH Wei

Journal

arXiv preprint arXiv:2402.05383

Published Date

2024/2/8

Study of decays at  = 8 TeV with the ATLAS detector

This paper presents a study of Z→ llγ decays with the ATLAS detector at the Large Hadron Collider. The analysis uses a proton–proton data sample corresponding to an integrated luminosity of 20.2 fb− 1 collected at a centre-of mass energy√ s= 8 TeV. Integrated fiducial cross-sections together with normalised differential fiducial cross-sections, sensitive to the kinematics of final-state QED radiation, are obtained. The results are found to be in agreement with state of-the-art predictions for final-state QED radiation. First measurements of Z→ llγ γ decays are also reported

Authors

N Null,G Aad,B Abbott,Dc Abbott,K Abeling,Sh Abidi,A Aboulhorma,H Abramowicz,H Abreu,Y Abulaiti,Aca Hoffman,Bs Acharya,B Achkar,Ca Bourdarios,L Adamczyk,L Adamek,Sv Addepalli,J Adelman,A Adiguzel,S Adorni,T Adye,Aa Affolder,Y Afik,Mn Agaras,J Agarwala,A Aggarwal,C Agheorghiesei,Ja Aguilar-Saavedra,A Ahmad,F Ahmadov,Ws Ahmed,S Ahuja,X Ai,G Aielli,I Aizenberg,M Akbiyik,Tpa Åkesson,Av Akimov,Ka Khoury,Gl Alberghi,J Albert,P Albicocco,S Alderweireldt,M Aleksa,In Aleksandrov,C Alexa,T Alexopoulos,A Alfonsi,F Alfonsi,M Alhroob,B Ali,S Ali,M Aliev,G Alimonti,W Alkakhi,C Allaire,Bmm Allbrooke,Pp Allport,A Aloisio,F Alonso,C Alpigiani,Ea Camelia,Ma Estevez,Mg Alviggi,M Aly,Ya Coutinho,A Ambler,C Amelung,M Amerl,Cg Ames,D Amidei,Spad Santos,S Amoroso,Kr Amos,V Ananiev,C Anastopoulos,T Andeen,Jk Anders,Sy Andrean,A Andreazza,S Angelidakis,A Angerami,Av Anisenkov,A Annovi,C Antel,Mt Anthony,E Antipov,M Antonelli,Dja Antrim,F Anulli,M Aoki,T Aoki,Jaa Pozo,Ma Aparo,La Bella,C Appelt,N Aranzabal,Va Ferraz,C Arcangeletti,Ath Arce,E Arena,J Arguin,S Argyropoulos,Jh Arling,Aj Armbruster,O Arnaez,H Arnold,Zpa Tame,G Artoni,H Asada,K Asai,S Asai,Na Asbah,K Assamagan,R Astalos,Rj Atkin,M Atkinson,Nb Atlay,H Atmani,Pa Atmasiddha,K Augsten,S Auricchio,Ad Auriol,Va Austrup,G Avner,G Avolio,K Axiotis,Mk Ayoub,G Azuelos,D Babal,H Bachacou,K Bachas,A Bachiu,F Backman,A Badea,P Bagnaia,M Bahmani,Aj Bailey,Vr Bailey,Jt Baines,C Bakalis,Ok Baker,Pj Bakker,E Bakos,Db Gupta,S Balaji,R Balasubramanian,Em Baldin,P Balek,E Ballabene

Journal

EUROPEAN PHYSICAL JOURNAL. C, PARTICLES AND FIELDS

Published Date

2024

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

The core-collapse supernova (CCSN) is considered one of the most energetic astrophysical events, accompanying the death of a massive star. A burst of neutrinos of tens of MeV energies plays important roles during its explosion and carries away most of the released gravitational binding energy of around 1053 erg. This overall picture is essentially supported by the detection of sparse neutrinos from SN 1987A in the Large Magellanic Cloud [1–3]. For the next Galactic or nearby extra-galactic CCSN, more detailed time and energy spectra information of neutrinos from the CCSN are highly desired to describe and model the complex physical processes of the explosion. Such more detailed picture will be achieved by different types of modern neutrino detectors with lower energy threshold, larger target masses and complementary designs. Moreover, the first detection of neutrinos emitted prior to the core collapse (pre …

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,Marco Beretta,Antonio Bergnoli,Daniel Bick,Lukas Bieger,Svetlana Biktemerova,Thilo Birkenfeld,Iwan Morton-Blake,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,Auttakit Chatrabhuti,Chao Chen,Guoming Chen,Pingping Chen,Shaomin Chen,Yixue Chen,Yu Chen,Zhangming Chen,Zhiyuan Chen,Zikang Chen,Jie Cheng,Yaping Cheng,Yu Chin Cheng,Alexander Chepurnov,Alexey Chetverikov,Davide Chiesa,Pietro Chimenti,Yen-Ting Chin,Ziliang Chu,Artem Chukanov,Gérard Claverie,Catia Clementi,Barbara Clerbaux,Marta Colomer Molla,Selma Conforti Di Lorenzo,Alberto Coppi,Daniele Corti,Simon Csakli,Flavio Dal Corso,Olivia Dalager,Jaydeep Datta,Christophe De La Taille,Zhi Deng,Ziyan Deng,Xiaoyu Ding,Xuefeng Ding,Yayun Ding,Bayu Dirgantara,Carsten Dittrich,Sergey Dmitrievsky,Tadeas Dohnal,Dmitry Dolzhikov,Georgy Donchenko,Jianmeng Dong,Evgeny Doroshkevich,Wei Dou,Marcos Dracos,Frédéric Druillole,Ran Du,Shuxian Du,Katherine Dugas,Stefano Dusini,Hongyue Duyang,Jessica Eck,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,Caren Hagner

Journal

Journal of Cosmology and Astroparticle Physics

Published Date

2024/1/25

Search for non-resonant Higgs boson pair production in the 2b+ 2ℓ+ Emiss T fnal state in pp collisions at√ s= 13 TeV with the ATLAS detector

A search for non-resonant Higgs boson pair production, as predicted by the Standard Model, is presented, where one of the Higgs bosons decays via the H→ b b channel and the other via one of the H→ W W⁎/Z Z⁎/τ τ channels. The analysis selection requires events to have at least two b-tagged jets and exactly two leptons (electrons or muons) with opposite electric charge in the final state. Candidate events consistent with Higgs boson pair production are selected using a multi-class neural network discriminant. The analysis uses 139 fb− 1 of pp collision data recorded at a centre-of-mass energy of 13 TeV by the ATLAS detector at the Large Hadron Collider. An observed (expected) upper limit of 1.2 (0.9− 0.3+ 0.4) pb is set on the non-resonant Higgs boson pair production cross-section at 95% confidence level, which is equivalent to 40 (29− 9+ 14) times the value predicted in the Standard Model.

Authors

Georges Aad,Brad Abbott,Dale Charles Abbott,A Abed Abud,Kira Abeling,Deshan Kavishka Abhayasinghe,Syed Haider Abidi,OS AbouZeid,Nadine L Abraham,Halina Abramowicz,Henso Abreu,Yiming Abulaiti,Bobby Samir Acharya,Baida Achkar,Shunsuke Adachi,Lennart Adam,C Adam Bourdarios,Leszek Adamczyk,Lukas Adamek,Jahred Adelman,Michael Adersberger,Aytul Adiguzel,Sofia Adorni,Tim Adye,AA Affolder,Yoav Afik,Christina Agapopoulou,Merve Nazlim Agaras,Anamika Aggarwal,Catalin Agheorghiesei,JA Aguilar-Saavedra,Faig Ahmadov,Waleed Syed Ahmed,Xiaocong Ai,Giulio Aielli,Shunichi Akatsuka,TPA Åkesson,Ece Akilli,AV Akimov,Konie Al Khoury,Gian Luigi Alberghi,Justin Albert,MJ Alconada Verzini,S Alderweireldt,Martin Aleksa,IN Aleksandrov,Calin Alexa,Didier Alexandre,Theodoros Alexopoulos,Alice Alfonsi,Fabrizio Alfonsi,Muhammad Alhroob,Babar Ali,Gianluca Alimonti,John Alison,Steven Patrick Alkire,Corentin Allaire,BMM Allbrooke,Benjamin William Allen,PP Allport,Alberto Aloisio,Alejandro Alonso,Francisco Alonso,Cristiano Alpigiani,Azzah Aziz Alshehri,M Alvarez Estevez,D Álvarez Piqueras,MG Alviggi,Y Amaral Coutinho,Alessandro Ambler,Luca Ambroz,Christoph Amelung,D Amidei,SP Amor Dos Santos,Simone Amoroso,Cherifa Sabrina Amrouche,Fenfen An,Christos Anastopoulos,Nansi Andari,Timothy Andeen,Christoph Falk Anders,John Kenneth Anders,Attilio Andreazza,V Andrei,Christopher Ryan Anelli,Stylianos Angelidakis,Aaron Angerami,AV Anisenkov,Alberto Annovi,Claire Antel,Matthew Thomas Anthony,Mario Antonelli,DJA Antrim,Fabio Anulli,Masato Aoki,JA Aparisi Pozo,L Aperio Bella,Giorgi Arabidze,JP Araque,V Araujo Ferraz,R Araujo Pereira,Chiara Arcangeletti,ATH Arce,Francisco Anuar Arduh,Jean-Francois Arguin,Spyridon Argyropoulos,J-H Arling,Aaron James Armbruster,Alexander Armstrong,Olivier Arnaez,Hannah Arnold,ZP Arrubarrena Tame,Andrei Artamonov,Giacomo Artoni,Sebastian Artz,Shoji Asai,Nedaa Asbah,Eleni Myrto Asimakopoulou,Lily Asquith,Jihad Assahsah,Ketevi Assamagan,Robert Astalos,Ryan Justin Atkin,Markus Atkinson,Naim Bora Atlay,Hicham Atmani,Kamil Augsten,Giuseppe Avolio,R Avramidou,Mohamad Kassem Ayoub,Adam Maxwell Azoulay,Georges Azuelos,Henri Bachacou,Konstantinos Bachas,Moritz Backes,Filip Backman,Paolo Bagnaia,Marzieh Bahmani,H Bahrasemani,AJ Bailey,Virginia Ruth Bailey,JT Baines,Milena Bajic,Christos Bakalis,OK Baker,Pepijn Johannes Bakker,D Bakshi Gupta,Shyam Balaji,EM Baldin,Petr Balek

Journal

Physics Letters B

Published Date

2020/2/10

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

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.

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,YC Cheng,ZK Cheng,JJ Cherwinka,MC Chu,JP Cummings,O Dalager,FS Deng,XY Ding,YY Ding,MV Diwan,T Dohnal,D Dolzhikov,J Dove,KV Dugas,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,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,W-H Tse,CE Tull,YC Tung,B Viren,V Vorobel,CH Wang,J Wang,M Wang,NY Wang,RG Wang,W Wang,X Wang,YF Wang,Z Wang,ZM Wang,HY Wei,LH Wei

Journal

arXiv preprint arXiv:2404.01687

Published Date

2024/4/2

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