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20042026
most citedFirst Results on 12Lambda-C production at DAPHNE

88 citations · 446 across the 42 of their papers we have counts for

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physics.ins-det2026

Detector Performance and Dark Matter Sensitivity of CYGNO with HFO-1234ze Gas Admixtures

F. D. Amaro, R. Antonietti, E. Baracchini +42

The CYGNO project develops optical time projection chambers for directional dark matter searches, using a He:CF4 (60:40) gas mixture at atmospheric pressure and a triple-GEM amplif…

physics.ins-det2026

He-CF4-CH4 ternary mixtures as target gas for the CYGNO directional dark matter experiment

F. D. Amaro, R. Antonietti, E. Baracchini +41

The CYGNO collaboration is advancing a high-resolution optical Time Projection Chamber (TPC) for directional dark matter searches and solar neutrino spectroscopy at LNGS. The detec…

physics.ins-det2026

Simulation of the CYGNO Gaseous TPC Optical Readout

F. D. Amaro, R. Antonietti, E. Baracchini +41

Gaseous Time Projection Chambers with Optical Readout are sensitive detectors suitable for 3D measurement of low-energy O(1 keV) particles and are proposed for detecting rare event…

physics.ins-det2024★ 3 cited

Enhancing the light yield of He:CF based gaseous detector

F. D. Amaro, R. Antonietti, E. Baracchini +51

The CYGNO experiment aims to build a large ( m) directional detector for rare event searches, such as nuclear recoils (NRs) induced by dark matter (DM), such a…

physics.ins-det2024

Charge Amplification in Low Pressure CF4:SF6:He Mixtures with a Multi-Mesh ThGEM for Directional Dark Matter Searches

F. D. Amaro, E. Baracchini, L. Benussi +46

The CYGNO collaboration is developing next generation directional Dark Matter (DM) detection experiments, using gaseous Time Projection Chambers (TPCs), as a robust method for iden…

physics.ins-det2024

Status of the production of GEM chambers for the CMS experiment at Large Hadron Collider

L. Benussi, S. Bianco, R. Campagnola +10

The High Luminosity LHC phase includes an upgrade to the muon stations for the CMS Experiment. CMS trigger and muon identification performance will be crucial, and it is, therefore…