1 September 2024 to 1 April 2025
Europe/Zurich timezone

Quantum Sensing for Dark Matter and Gravitational Waves

Not scheduled
1m

Description

Searches for wave-like dark matter can benefit from efforts to develop experimental sensitivity beyond the Standard Quantum Limit. In particular, RF cavity experiments and spin magnetometers are promising technologies in this endeavour. In recent years, it has been shown that experiments of this kind can also be sensitive to high-frequency gravitational waves. As part of the community input to the European Strategy for Particle Physics 2026 update, we report on the activities and plans of some experimental and theoretical groups aiming to search for dark matter (and gravitational wave) signals beyond the Standard Quantum limit. Our report is not exhaustive in cataloging the efforts of experimental or theoretical groups in Europe, but presents the current status and plans of the CASPEr, GNOME, GravNet, MAGO, RADES and SRF Heterodyne collaborations.

Authors

Prof. Alejandro Díaz-Morcillo (Universidad Politécnica de Cartagena) Alexander Sushkov Alick Macpherson (CERN) Benito Gimeno Martinez (IFIC (University of Valencia - CSIC)) Carl Beadle (Universite de Geneve (CH)) Claudio Gatti (INFN e Laboratori Nazionali di Frascati (IT)) DMITRY BUDKER (Helmholtz Institute Mainz and UC Berkeley) Derek Jackson Kimball Diego Blas (ICREA/IFAE) Hendrik Bekker Igor Garcia Irastorza (Universidad de Zaragoza (ES)) Julian Walter Krisztian Peters (Deutsches Elektronen-Synchrotron (DE)) Mr Lee Millar (CERN) Natalia Koss (CERN) Raffaele D'Agnolo Sebastian Ellis (Universite de Geneve (CH)) Sergio Calatroni (CERN) Yuzhe Zhang

Presentation materials