Ultrapure SiPMs and Associated Readout Electronics group activity
The main focus of group 4 led by Dr Masayuki Wada is the development of light detectors based on Silicon Photo Multipliers (SiPMs) for experimental searches for new physics beyond the Standard Model, such as dark matter direction and neutrino-less double beta decay. The same technology will be applied to develop medical devices based on SiPMs.
One key physics goal is to use dedicated systems of SiPMs to look for the elusive dark matter in the Universe. In order to achieve extreme sensitivity of detectors, its components themselves must not generate any background that could potentially obscure the signal from dark matter. Another important physics goal is the search for so-called Majorana neutrinos. A similar detection technology enables us to look for this potential feature of neutrinos, which could shed lights on the reasons for why our Universe is mostly made up of matter and not antimatter.
The group works is in collaboration with local groups in Poland and international partners to develop radio-pure light detectors with high performance required for those exciting searches.
We are proud to announce that Astrocent (NCAC PAS) has signed a Memorandum of Understanding (MoU) with CERN to become a participating institution in the Detector Research and Development 1 (DRD1) Collaboration, which focuses on advancing gaseous detector technologies.
The MoU was signed on 29 July 2025 by Prof. Rafał Moderski, Director of NCAC PAS, formalizing Astrocent’s involvement in this cutting-edge R&D initiative hosted by CERN. While the scientific proposal for DRD1 was reviewed and approved by CERN’s Research Board in late 2023, the signing of this MoU marks the official establishment of the collaboration.
Celebrating a New Era of Scientific Excellence: Astrocent Plus Takes Stage
On 19 February 2025... Read more
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