11–13 May 2026
Roma
Europe/Rome timezone

Session

TES Based Neutrino and Dark Matter

11 May 2026, 17:00
Roma

Roma

Centro Congressi d'Ateneo, Via Salaria 113, 00198 Roma

Conveners

TES Based Neutrino and Dark Matter

  • Claudia Tomei (Istituto Nazionale di Fisica Nucleare)

Presentation materials

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  1. Paolo Gorla (Istituto Nazionale di Fisica Nucleare)
    11/05/2026, 17:00

    The Cryogenic Rare Event Search with Superconducting Thermometers (CRESST), located at the Laboratori Nazionali del Gran Sasso (INFN, Italy), targets the direct detection of sub-GeV dark matter (DM) via nuclear recoils in cryogenic CaWO$_4$ detectors instrumented with tungsten Transition Edge Sensors (W-TES). Operating at millikelvin temperatures, these detectors combine phonon and light...

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  2. Raimund Strauss (TUM)
    11/05/2026, 17:20
  3. Matteo Borghesi (Istituto Nazionale di Fisica Nucleare)
    11/05/2026, 17:40

    The absolute value of the neutrino mass 𝑚𝜈remains one of the key missing pieces in the Standard Model. Its value plays a fundamental role in shaping the formation of large-scale structures in the Universe. The only model-independent method to determine 𝑚𝜈relies on direct kinematic measurements of the electrons emitted in beta decay processes. Current experimental approaches fall into two...

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  4. Yury Kolomensky
    11/05/2026, 18:05

    CUPID — CUORE Upgrade with Particle Identification — is the ton-scale neutrinoless double beta decay (NLDBD) experiment at LNGS. CUPID will be mounted in the CUORE cryostat, leveraging the existing cryogenic infrastructure and a decade of experience operating the largest bolometer array in existence. CUPID will deploy 1600 Li2MoO4 scintillating bolometers with the dual heat-light readout to...

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