Future Experiments in Particle and Nuclear Physics
Astrophysical Instrumentation for ICTS, ESFRI Projects in Astronomy, and Space Missions
Gravitational Wave Experiments and Multi-Messenger Astronomy
Large Astronomical Surveys
Direct Searches for Dark Matter
Neutrino Physics
Space Exploration with Small Satellites
Computing, Big Data, and Artificial Intelligence
Summary of program lines of action in terms of objectives, participants, actions to be carried out, and expected results.
Line of Action 5
The objective of this line is to carry out a series of experimental, technological development, and phenomenological actions for the direct detection of Dark Matter over a wide range of masses, from the μeV axion to the 100 GeV WIMP. Much of the experimental activity in this LIA is carried out at the Underground Laboratory of Canfranc (LSC), a reference ICTS in the field of particle astrophysics.
The scientific communities that participate in this line of action are: