A next-generation liquid xenon observatory for dark matter and neutrino physics
- Authors
- J Aalbers
- SS AbdusSalam
- K Abe
- V Aerne
- F Agostini
- S Ahmed Maouloud
- DS Akerib
- DY Akimov
- J Akshat
- AK Al Musalhi
- F Alder
- SK Alsum
- L Althueser
- CS Amarasinghe
- FD Amaro
- A Ames
- TJ Anderson
- B Andrieu
- N Angelides
- E Angelino
- J Angevaare
- VC Antochi
- B Antunovic
- D Antón Martin
- E Aprile
- HM Araújo
- JE Armstrong
- F Arneodo
- M Arthurs
- P Asadi
- S Baek
- X Bai
- D Bajpai
- A Baker
- J Balajthy
- S Balashov
- M Balzer
- A Bandyopadhyay
- J Bang
- E Barberio
- JW Bargemann
- L Baudis
- D Bauer
- D Baur
- A Baxter
- AL Baxter
- M Bazyk
- K Beattie
- J Behrens
- NF Bell
- L Bellagamba
- P Beltrame
- M Benabderrahmane
- EP Bernard
- GF Bertone
- P Bhattacharjee
- A Bhatti
- A Biekert
- TP Biesiadzinski
- AR Binau
- R Biondi
- Y Biondi
- HJ Birch
- F Bishara
- A Bismark
- C Blanco
- GM Blockinger
- E Bodnia
- C Boehm
- AI Bolozdynya
- PD Bolton
- S Bottaro
- C Bourgeois
- B Boxer
- A Breskin
- PA Breur
- CAJ Brew
- J Brod
- E Brookes
- A Brown
- E Brown
- S Bruenner
- G Bruno
- P Brás
- R Budnik
- TK Bui
- S Burdin
- S Buse
- JK Busenitz
- D Buttazzo
- M Buuck
- A Buzulutskov
- R Cabrita
- C Cai
- D Cai
- C Capelli
- JMR Cardoso
- MC Carmona-Benitez
- M Cascella
- R Catena
- S Chakraborty
- C Chan
- S Chang
- A Chauvin
- A Chawla
- H Chen
- V Chepel
- NI Chott
- D Cichon
- A Cimental Chavez
- B Cimmino
- M Clark
- RT Co
- AP Colijn
- J Conrad
- MV Converse
- M Costa
- A Cottle
- G Cox
- O Creaner
- JJ Cuenca Garcia
- JP Cussonneau
- JE Cutter
- CE Dahl
- A David
- A de Gouvêa
- L de Viveiros
- MP Decowski
- JB Dent
- FF Deppisch
- P Di Gangi
- A Di Giovanni
- S Di Pede
- J Dierle
- S Diglio
- JEY Dobson
- M Doerenkamp
- JMF dos Santos
- D Douillet
- G Drexlin
- E Druszkiewicz
- D Dunsky
- V D’Andrea
- K Eitel
- A Elykov
- T Emken
- R Engel
- SR Eriksen
- M Fairbairn
- A Fan
- JJ Fan
- SJ Farrell
- S Fayer
- NM Fearon
- A Ferella
- C Ferrari
- A Fieguth
- A Fieguth
- S Fiorucci
- H Fischer
- H Flaecher
- M Flierman
- T Florek
- R Foot
- PJ Fox
- R Franceschini
- ED Fraser
- CS Frenk
- S Frohlich
- T Fruth
- W Fulgione
- C Fuselli
- P Gaemers
- R Gaior
- RJ Gaitskell
- M Galloway
- F Gao
- I Garcia Garcia
- J Genovesi
- C Ghag
- S Ghosh
- E Gibson
- W Gil
- D Giovagnoli
- F Girard
- R Glade-Beucke
- F Glück
- S Gokhale
- L Grandi
- J Grigat
- B Grinstein
- L Gráf
- R Grössle
- H Guan
- M Guida
- R Gumbsheimer
- CB Gwilliam
- CR Hall
- LJ Hall
- R Hammann
- K Han
- V Hannen
- S Hansmann-Menzemer
- R Harata
- SP Hardin
- CA Hardy
- E Hardy
- K Harigaya
- R Harnik
- SJ Haselschwardt
- M Hernandez
- SA Hertel
- A Higuera
- C Hils
- S Hochrein
- L Hoetzsch
- M Hoferichter
- N Hood
- D Hooper
- M Horn
- J Howlett
- DQ Huang
- Y Huang
- D Hunt
- M Iacovacci
- G Iaquaniello
- R Ide
- CM Ignarra
- G Iloglu
- Y Itow
- E Jacquet
- O Jahangir
- J Jakob
- RS James
- A Jansen
- W Ji
- X Ji
- F Joerg
- J Johnson
- A Joy
- AC Kaboth
- L Kalhor
- AC Kamaha
- K Kanezaki
- K Kar
- M Kara
- N Kato
- P Kavrigin
- S Kazama
- AW Keaveney
- J Kellerer
- D Khaitan
- A Khazov
- G Khundzakishvili
- I Khurana
- B Kilminster
- M Kleifges
- P Ko
- M Kobayashi
- D Kodroff
- G Koltmann
- A Kopec
- A Kopmann
- J Kopp
- L Korley
- VN Kornoukhov
- EV Korolkova
- H Kraus
- LM Krauss
- S Kravitz
- L Kreczko
- VA Kudryavtsev
- F Kuger
- J Kumar
- L LaCascio
- R Laha
- Q Laine
- H Landsman
- RF Lang
- EA Leason
- J Lee
- DS Leonard
- KT Lesko
- L Levinson
- C Levy
- I Li
- SC Li
- T Li
- S Liang
- CS Liebenthal
- J Lin
- Q Lin
- S Lindemann
- M Lindner
- A Lindote
- R Linehan
- WH Lippincott
- J Liu
- K Liu
- X Liu
- J Loizeau
- F Lombardi
- J Long
- MI Lopes
- E Lopez Asamar
- W Lorenzon
- C Lu
- S Luitz
- B López Paredes
- Y Ma
- PAN Machado
- C Macolino
- T Maeda
- J Mahlstedt
- PA Majewski
- A Manalaysay
- A Mancuso
- L Manenti
- A Manfredini
- RL Mannino
- N Marangou
- J March-Russell
- F Marignetti
- T Marrodán Undagoitia
- K Martens
- R Martin
- I Martinez-Soler
- J Masbou
- D Masson
- E Masson
- S Mastroianni
- M Mastronardi
- JA Matias-Lopes
- ME McCarthy
- N McFadden
- E McGinness
- DN McKinsey
- J McLaughlin
- K McMichael
- P Meinhardt
- Y Meng
- J Menéndez
- M Messina
- R Midha
- D Milisavljevic
- EH Miller
- B Milosevic
- S Milutinovic
- SA Mitra
- K Miuchi
- E Mizrachi
- K Mizukoshi
- A Molinario
- A Monte
- CMB Monteiro
- ME Monzani
- JS Moore
- JA Morad
- JD Morales Mendoza
- S Moriyama
- E Morrison
- E Morteau
- K Morå
- Y Mosbacher
- BJ Mount
- J Mueller
- A St J Murphy
- M Murra
- D Naim
- S Nakamura
- E Nash
- N Navaieelavasani
- A Naylor
- C Nedlik
- HN Nelson
- F Neves
- JL Newstead
- K Ni
- JA Nikoleyczik
- V Niro
- UG Oberlack
- M Obradovic
- K Odgers
- P Oikonomou
- I Olcina
- K Oliver-Mallory
- A Oranday
- J Orpwood
- I Ostrovskiy
- K Ozaki
- CAJ O’Hare
- B Paetsch
- S Pal
- J Palacio
- KJ Palladino
- J Palmer
- P Panci
- M Pandurovic
- A Parlati
- N Parveen
- SJ Patton
- Q Pellegrini
- B Penning
- G Pereira
- R Peres
- Y Perez-Gonzalez
- E Perry
- T Pershing
- R Petrossian-Byrne
- J Pienaar
- A Piepke
- G Pieramico
- M Pierre
- M Piotter
- V Pizzella
- G Plante
- T Pollmann
- D Porzio
- V Pěč
- J Qi
- Y Qie
- J Qin
- F Quevedo
- N Raj
- M Rajado Silva
- K Ramanathan
- D Ramírez García
- J Ravanis
- L Redard-Jacot
- D Redigolo
- S Reichard
- J Reichenbacher
- CA Rhyne
- A Richards
- Q Riffard
- GRC Rischbieter
- A Rocchetti
- SL Rosenfeld
- R Rosero
- N Rupp
- T Rushton
- S Saha
- P Salucci
- L Sanchez
- P Sanchez-Lucas
- D Santone
- I Sarnoff
- G Sartorelli
- ABMR Sazzad
- M Scheibelhut
- RW Schnee
- M Schrank
- J Schreiner
- D Schulte
- P Schulte
- H Schulze Eissing
- M Schumann
- T Schwemberger
- A Schwenk
- T Schwetz
- L Scotto Lavina
- PR Scovell
- H Sekiya
- M Selvi
- E Semenov
- F Semeria
- P Shagin
- S Shaw
- S Shi
- E Shockley
- TA Shutt
- R Si-Ahmed
- JJ Silk
- C Silva
- MC Silva
- H Simgen
- G Sinev
- R Singh
- W Skulski
- J Smirnov
- R Smith
- M Solmaz
- VN Solovov
- P Sorensen
- J Soria
- TJ Sparmann
- I Stancu
- M Steidl
- A Stevens
- K Stifter
- LE Strigari
- D Subotic
- B Suerfu
- AM Suliga
- TJ Sumner
- P Szabo
- M Szydagis
- A Takeda
- Y Takeuchi
- P-L Tan
- C Taricco
- WC Taylor
- DJ Temples
- A Terliuk
- PA Terman
- D Thers
- K Thieme
- T Thümmler
- DR Tiedt
- M Timalsina
- WH To
- F Toennies
- Z Tong
- F Toschi
- DR Tovey
- J Tranter
- M Trask
- GC Trinchero
- M Tripathi
- DR Tronstad
- R Trotta
- YD Tsai
- CD Tunnell
- WG Turner
- R Ueno
- P Urquijo
- U Utku
- A Vaitkus
- K Valerius
- MGD van der Grinten
- E Vassilev
- S Vecchi
- V Velan
- S Vetter
- AC Vincent
- L Vittorio
- G Volta
- B von Krosigk
- M von Piechowski
- D Vorkapic
- CEM Wagner
- AM Wang
- B Wang
- JJ Wang
- L-T Wang
- M Wang
- W Wang
- Y Wang
- Y Wang
- JR Watson
- Y Wei
- C Weinheimer
- E Weisman
- M Weiss
- D Wenz
- SM West
- TJ Whitis
- M Williams
- MJ Wilson
- D Winkler
- C Wittweg
- J Wolf
- T Wolf
- FLH Wolfs
- S Woodford
- D Woodward
- CJ Wright
- P Wu
- VHS Wu
- M Wurm
- S Wüstling
- Q Xia
- X Xiang
- Y Xing
- D Xu
- J Xu
- Z Xu
- M Yamashita
- R Yamazaki
- H Yan
- L Yang
- Y Yang
- J Ye
- M Yeh
- I Young
- HB Yu
- TT Yu
- L Yuan
- G Zavattini
- S Zerbo
- Y Zhang
- M Zhong
- N Zhou
- X Zhou
- T Zhu
- Y Zhu
- Y Zhuang
- JP Zopounidis
- K Zuber
- J Zupan
- F Šimkovic
- Publication date
- 1 January 2022
- Publisher
- Journal of Physics G: Nuclear and Particle Physics
- Doi
Abstract
Abstract The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for weakly interacting massive particles, while featuring extensive sensitivity to many alternative dark matter candidates. These detectors can also study neutrinos through neutrinoless double-beta decay and through a variety of astrophysical sources. A next-generation xenon-based detector will therefore be a true multi-purpose observatory to significantly advance particle physics, nuclear physics, astrophysics, solar physics, and cosmology. This review article presents the science cases for such a detector.</jats:pSimilar works
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