A next-generation liquid xenon observatory for dark matter and neutrino physics
Review article, 2023
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.
neutrinoless double-beta decay
supernova
astroparticle physics
neutrinos
direct detection
dark matter
xenon
Author
J. Aalbers
Stanford University
S. S. Abdussalam
Shahid Beheshti University
K. Abe
University of Tokyo
V. Aerne
University of Zürich
F. Agostini
University of Bologna
S. Ahmed Maouloud
Pierre and Marie Curie University (UPMC)
D. S. Akerib
Stanford University
D. Y. Akimov
National Research Nuclear University
J. Akshat
Purdue University
A. K. Al Musalhi
University of Oxford
F. Alder
University College London (UCL)
S. K. Alsum
University of Wisconsin Madison
L. Althueser
University of Münster
C. S. Amarasinghe
University of Michigan
F. D. Amaro
University of Coimbra
A. Ames
Stanford University
T. J. Anderson
Stanford University
B. Andrieu
Pierre and Marie Curie University (UPMC)
N. Angelides
Imperial College London
E. Angelino
University of Turin
J. Angevaare
University of Amsterdam
V. C. Antochi
Oskar Klein Centre
D. Antón Martin
University of Chicago
B. Antunovic
University of Banja Luka
Institut za nuklearne nauke Vinca
E. Aprile
Columbia University
H. M. Araújo
Imperial College London
J. E. Armstrong
University of Maryland
F. Arneodo
New York University Abu Dhabi
M. Arthurs
University of Michigan
P. Asadi
Center for Theoretical Physics
S. Baek
Korea University
X. Bai
South Dakota School of Mines & Technology
D. Bajpai
University of Alabama
A. Baker
Imperial College London
J. Balajthy
University of California
S. Balashov
STFC Rutherford Appleton Laboratory
M. Balzer
Karlsruhe Institute of Technology (KIT)
A. Bandyopadhyay
Ramakrishna Mission Vivekananda Educational and Research Institute
J. Bang
Brown University
E. Barberio
School of Physics
J. W. Bargemann
University of California
L. Baudis
University of Zürich
D. Bauer
Imperial College London
D. Baur
University of Freiburg
A. Baxter
University of Liverpool
A. L. Baxter
Purdue University
M. Bazyk
Nantes University
K. Beattie
Lawrence Berkeley National Laboratory
J. Behrens
Karlsruhe Institute of Technology (KIT)
N. F. Bell
School of Physics
L. Bellagamba
University of Bologna
P. Beltrame
Vatican Observatory
M. Benabderrahmane
New York University Abu Dhabi
E. P. Bernard
University of California
Lawrence Berkeley National Laboratory
G. F. Bertone
University of Amsterdam
P. Bhattacharjee
Saha Institute of Nuclear Physics
A. Bhatti
University of Maryland
A. Biekert
Lawrence Berkeley National Laboratory
University of California
T. P. Biesiadzinski
Stanford University
A. R. Binau
Purdue University
R. Biondi
Laboratori Nazionali del Gran Sasso
Y. Biondi
University of Zürich
H. J. Birch
University of Michigan
F. Bishara
Deutsches Elektronen-Synchrotron (DESY)
A. Bismark
University of Zürich
C. Blanco
Princeton University
Oskar Klein Centre
G. M. Blockinger
SUNY Albany
E. Bodnia
University of California
C. Boehm
The University of Sydney
A. I. Bolozdynya
National Research Nuclear University
P. D. Bolton
University College London (UCL)
S. Bottaro
National Institute for Nuclear Physics
Scuola Normale Superiore di Pisa
C. Bourgeois
Laboratoire de l'Accélérateur Linéaire
B. Boxer
University of California
P. Brás
University of Coimbra
A. Breskin
Weizmann Institute of Science
P. A. Breur
University of Amsterdam
C. A.J. Brew
STFC Rutherford Appleton Laboratory
J. Brod
University of Cincinnati
E. Brookes
University of Amsterdam
A. Brown
University of Freiburg
E. Brown
Rensselaer Polytechnic Institute
S. Bruenner
University of Amsterdam
G. Bruno
Nantes University
R. Budnik
Weizmann Institute of Science
T. K. Bui
University of Tokyo
S. Burdin
University of Liverpool
S. Buse
University of Zürich
J. K. Busenitz
University of Alabama
D. Buttazzo
National Institute for Nuclear Physics
M. Buuck
Stanford University
A. Buzulutskov
Novosibirsk State University
Russian Academy of Sciences
R. Cabrita
University of Coimbra
C. Cai
Tsinghua University
D. Cai
Nantes University
C. Capelli
University of Zürich
J. M.R. Cardoso
University of Coimbra
M. C. Carmona-Benitez
Eberly College of Science
M. Cascella
University College London (UCL)
Riccardo Catena
Chalmers, Physics, Subatomic, High Energy and Plasma Physics
Journal of Physics G: Nuclear and Particle Physics
0954-3899 (ISSN) 13616471 (eISSN)
Vol. 50 1 013001Empirical Determination of the Dark Matter Particle Spin
Swedish Research Council (VR) (2018-05029), 2019-01-01 -- 2022-12-31.
Subject Categories
Accelerator Physics and Instrumentation
Subatomic Physics
Other Physics Topics
DOI
10.1088/1361-6471/ac841a