A next-generation liquid xenon observatory for dark matter and neutrino physics
Reviewartikel, 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
Författare
J. Aalbers
Stanford University
S. S. Abdussalam
Shahid Beheshti University
K. Abe
University of Tokyo
V. Aerne
Universität Zürich
F. Agostini
Universita di Bologna
S. Ahmed Maouloud
Université Pierre et Marie Curie (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
Universität Münster
C. S. Amarasinghe
University of Michigan
F. D. Amaro
Universidade de Coimbra
A. Ames
Stanford University
T. J. Anderson
Stanford University
B. Andrieu
Université Pierre et Marie Curie (UPMC)
N. Angelides
Imperial College London
E. Angelino
Universita degli Studi di Torino
J. Angevaare
Universiteit Van 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
Karlsruher Institut für Technologie (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
Universität Zürich
D. Bauer
Imperial College London
D. Baur
Albert-Ludwigs-Universität Freiburg
A. Baxter
University of Liverpool
A. L. Baxter
Purdue University
M. Bazyk
Université de Nantes
K. Beattie
Lawrence Berkeley National Laboratory
J. Behrens
Karlsruher Institut für Technologie (KIT)
N. F. Bell
School of Physics
L. Bellagamba
Universita di 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
Universiteit Van 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
Universität Zürich
H. J. Birch
University of Michigan
F. Bishara
Deutsches Elektronen-Synchrotron (DESY)
A. Bismark
Universität 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
Istituto Nazionale di Fisica Nucleare
Scuola Normale Superiore di Pisa
C. Bourgeois
Laboratoire de l'Accélérateur Linéaire
B. Boxer
University of California
P. Brás
Universidade de Coimbra
A. Breskin
Weizmann Institute of Science
P. A. Breur
Universiteit Van Amsterdam
C. A.J. Brew
STFC Rutherford Appleton Laboratory
J. Brod
University of Cincinnati
E. Brookes
Universiteit Van Amsterdam
A. Brown
Albert-Ludwigs-Universität Freiburg
E. Brown
Rensselaer Polytechnic Institute
S. Bruenner
Universiteit Van Amsterdam
G. Bruno
Université de Nantes
R. Budnik
Weizmann Institute of Science
T. K. Bui
University of Tokyo
S. Burdin
University of Liverpool
S. Buse
Universität Zürich
J. K. Busenitz
University of Alabama
D. Buttazzo
Istituto Nazionale di Fisica Nucleare
M. Buuck
Stanford University
A. Buzulutskov
Novosibirsk State University
Russian Academy of Sciences
R. Cabrita
Universidade de Coimbra
C. Cai
Tsinghua University
D. Cai
Université de Nantes
C. Capelli
Universität Zürich
J. M.R. Cardoso
Universidade de Coimbra
M. C. Carmona-Benitez
Eberly College of Science
M. Cascella
University College London (UCL)
Riccardo Catena
Chalmers, Fysik, Subatomär, högenergi- och plasmafysik
Journal of Physics G: Nuclear and Particle Physics
0954-3899 (ISSN) 13616471 (eISSN)
Vol. 50 1 013001Empirisk bestämning av mörka materians spinn
Vetenskapsrådet (VR) (2018-05029), 2019-01-01 -- 2022-12-31.
Ämneskategorier
Acceleratorfysik och instrumentering
Subatomär fysik
Annan fysik
DOI
10.1088/1361-6471/ac841a