CERN Accelerating science

Article
Report number arXiv:2104.07634
Title Direct detection of dark matter—APPEC committee report
Related titleDirect detection of dark matter—APPEC committee report
Author(s) Billard, Julien (IP2I, Lyon) ; Boulay, Mark (Carleton U.) ; Cebrián, Susana (Zaragoza U.) ; Covi, Laura (Gottingen U.) ; Fiorillo, Giuliana (Insubria U., Como ; Naples U. ; INFN, Naples) ; Green, Anne (Nottingham U.) ; Kopp, Joachim (CERN ; Mainz U.) ; Majorovits, Béla (Munich, Max Planck Inst.) ; Palladino, Kimberly (Wisconsin U., Madison ; Oxford U.) ; Petricca, Federica (Munich, Max Planck Inst.) ; Roszkowski, Leszek (Warsaw, Inst. Phys. ; Cracow, Copernicus Astron. Ctr. ; NCBJ, Warsaw) ; Schumann, Marc (Freiburg U.)
Publication 2022-04-29
Imprint 2021-04-15
Number of pages 68
Note 106 pages
In: Rep. Prog. Phys.
DOI 10.1088/1361-6633/ac5754
10.1088/1361-6633/ac5754 (publication)
Subject category hep-ph ; Particle Physics - Phenomenology ; astro-ph.HE ; Astrophysics and Astronomy ; hep-ex ; Particle Physics - Experiment
Abstract This Report provides an extensive review of the experimental programme of direct detection searches of particle dark matter. It focuses mostly on European efforts, both current and planned, but does it within a broader context of a worldwide activity in the field. It aims at identifying the virtues, opportunities and challenges associated with the different experimental approaches and search techniques. It presents scientific and technological synergies, both existing and emerging, with some other areas of particle physics, notably collider and neutrino programmes, and beyond. It addresses the issue of infrastructure in light of the growing needs and challenges of the different experimental searches. Finally, the Report makes a number of recommendations from the perspective of a long-term future of the field. They are introduced, along with some justification, in the opening Overview and Recommendations section and are next summarised at the end of the Report. Overall, we recommend that the direct search for dark matter particle interactions with a detector target should be given top priority in astroparticle physics, and in all particle physics, and beyond, as a positive measurement will provide the most unambiguous confirmation of the particle nature of dark matter in the Universe.
Copyright/License publication: © 2022 IOP Publishing Ltd
preprint: (License: CC-BY-NC-ND 4.0)

\sigma_d$ at $\ge$3\,sigma. It is computed using the assumptions and the methodology described in~\cite{Billard:2011zj,Billard:2013qya}, however, it has been extended to very low DM mass range by assuming an unrealistic $1\milieV$ threshold below $0.8\GeV/c^2$. Shown are results from CDEX~\cite{Liu:2019kzq}, CDMSLite~\cite{Agnese:2018gze}, COSINE-100~\cite{cosinenature}, CRESST~\cite{Angloher:2017sxg,Abdelhameed:2019hmk}, DAMA/LIBRA~\cite{Bernabei:2008yi} (contours from~\cite{Savage:2008er}), DAMIC~\cite{damic3}, DarkSide-50~\cite{Agnes:2018ep,Agnes:2018fg}, DEAP-3600~\cite{Ajaj:2019jk}, EDELWEISS~\cite{Armengaud:2019kfj,Hehn:2016nll}, LUX~\cite{Akerib:2016vxi,Akerib:2018hck}, NEWS-G~\cite{newsg1}, PandaX-II~\cite{Cui:2017nnn}, SuperCDMS~\cite{Agnese:2014aze}, XENON100~\cite{Aprile:2016swn} and XENON1T~\cite{Aprile:2018dbl,Aprile:2019xxb,Aprile:2019jmx,Aprile:2020thb}." width="200px"/> Show more plots


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