First Constraints from DAMIC-M on Sub-GeV Dark-Matter Particles Interacting with Electrons.


Journal

Physical review letters
ISSN: 1079-7114
Titre abrégé: Phys Rev Lett
Pays: United States
ID NLM: 0401141

Informations de publication

Date de publication:
28 Apr 2023
Historique:
received: 09 02 2023
accepted: 21 03 2023
medline: 12 5 2023
pubmed: 12 5 2023
entrez: 12 5 2023
Statut: ppublish

Résumé

We report constraints on sub-GeV dark matter particles interacting with electrons from the first underground operation of DAMIC-M detectors. The search is performed with an integrated exposure of 85.23 g days, and exploits the subelectron charge resolution and low level of dark current of DAMIC-M charge-coupled devices (CCDs). Dark-matter-induced ionization signals above the detector dark current are searched for in CCD pixels with charge up to 7e^{-}. With this dataset we place limits on dark matter particles of mass between 0.53 and 1000  MeV/c^{2}, excluding unexplored regions of parameter space in the mass ranges [1.6,1000]  MeV/c^{2} and [1.5,15.1]  MeV/c^{2} for ultralight and heavy mediator interactions, respectively.

Identifiants

pubmed: 37172255
doi: 10.1103/PhysRevLett.130.171003
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

171003

Auteurs

I Arnquist (I)

Pacific Northwest National Laboratory (PNNL), Richland, Washington, USA.

N Avalos (N)

Centro Atómico Bariloche and Instituto Balseiro, Comisión Nacional de Energía Atómica (CNEA), Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Universidad Nacional de Cuyo (UNCUYO), San Carlos de Bariloche 8400, Argentina.

D Baxter (D)

Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.

X Bertou (X)

Centro Atómico Bariloche and Instituto Balseiro, Comisión Nacional de Energía Atómica (CNEA), Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Universidad Nacional de Cuyo (UNCUYO), San Carlos de Bariloche 8400, Argentina.

N Castelló-Mor (N)

Instituto de Física de Cantabria (IFCA), CSIC-Universidad de Cantabria, Santander 39005, Spain.

A E Chavarria (AE)

Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA.

J Cuevas-Zepeda (J)

Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.

J Cortabitarte Gutiérrez (JC)

Instituto de Física de Cantabria (IFCA), CSIC-Universidad de Cantabria, Santander 39005, Spain.

J Duarte-Campderros (J)

Instituto de Física de Cantabria (IFCA), CSIC-Universidad de Cantabria, Santander 39005, Spain.

A Dastgheibi-Fard (A)

LPSC LSM, CNRS/IN2P3, Université Grenoble-Alpes, Grenoble 38026, France.

O Deligny (O)

CNRS/IN2P3, IJCLab, Université Paris-Saclay, Orsay 91405, France.

C De Dominicis (C)

Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.
SUBATECH, Nantes Université, IMT Atlantique, CNRS-IN2P3, Nantes 44300, France.

E Estrada (E)

Centro Atómico Bariloche and Instituto Balseiro, Comisión Nacional de Energía Atómica (CNEA), Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Universidad Nacional de Cuyo (UNCUYO), San Carlos de Bariloche 8400, Argentina.

N Gadola (N)

Universität Zürich Physik Institut, Zürich 8057, Switzerland.

R Gaïor (R)

Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.

T Hossbach (T)

Pacific Northwest National Laboratory (PNNL), Richland, Washington, USA.

L Iddir (L)

Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.

L Khalil (L)

Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.

B Kilminster (B)

Universität Zürich Physik Institut, Zürich 8057, Switzerland.

A Lantero-Barreda (A)

Instituto de Física de Cantabria (IFCA), CSIC-Universidad de Cantabria, Santander 39005, Spain.

I Lawson (I)

SNOLAB, Lively, Ontario P341N2, Canada.

S Lee (S)

Universität Zürich Physik Institut, Zürich 8057, Switzerland.

A Letessier-Selvon (A)

Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.

P Loaiza (P)

CNRS/IN2P3, IJCLab, Université Paris-Saclay, Orsay 91405, France.

A Lopez-Virto (A)

Instituto de Física de Cantabria (IFCA), CSIC-Universidad de Cantabria, Santander 39005, Spain.

A Matalon (A)

Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.

S Munagavalasa (S)

Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.

K J McGuire (KJ)

Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA.

P Mitra (P)

Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA.

D Norcini (D)

Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.

G Papadopoulos (G)

Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.

S Paul (S)

Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.

A Piers (A)

Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA.

P Privitera (P)

Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.

K Ramanathan (K)

Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.

P Robmann (P)

Universität Zürich Physik Institut, Zürich 8057, Switzerland.

M Settimo (M)

SUBATECH, Nantes Université, IMT Atlantique, CNRS-IN2P3, Nantes 44300, France.

R Smida (R)

Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.

R Thomas (R)

Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.

M Traina (M)

Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA.
Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.

I Vila (I)

Instituto de Física de Cantabria (IFCA), CSIC-Universidad de Cantabria, Santander 39005, Spain.

R Vilar (R)

Instituto de Física de Cantabria (IFCA), CSIC-Universidad de Cantabria, Santander 39005, Spain.

G Warot (G)

LPSC LSM, CNRS/IN2P3, Université Grenoble-Alpes, Grenoble 38026, France.

R Yajur (R)

Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.

J-P Zopounidis (JP)

Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.

Classifications MeSH