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Christophe Royon, William d?Assignies D., Florian Gautier, Tommaso Isidori, Nicola Minafra and Alexander Novikov
We use fast silicon detectors and the fast sampling method originally developed for high energy physics for two applications: cosmic ray measurements in collaboration with NASA and dose measurements during flash beam cancer treatment. The cosmic ray meas...
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Elisa Maria Gandolfo, José Roberto Brandao Oliveira, Luigi Campajola, Dimitra Pierroutsakou, Alfonso Boiano, Clementina Agodi, Francesco Cappuzzello, Diana Carbone, Manuela Cavallaro, Irene Ciraldo, Daniela Calvo, Franck Delaunay, Canel Eke, Fabio Longhitano, Nilberto Medina, Mauricio Moralles, Diego Sartirana, Vijay Raj Sharma, Alessandro Spatafora, Dennis Toufen and Paolo FinocchiaroaddShow full author listremoveHide full author list
The G-NUMEN array is the future gamma spectrometer of the NUMEN experiment (nuclear matrix element for neutrinoless double beta decay), to be installed around the object point of the MAGNEX magnetic spectrometer at the INFN-LNS laboratory. This project a...
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Thomas Anderson, Thomas Barbera, Bradley Cox, Paul Debbins, Maxwell Dubnowski, Kiva Ford, Maxwell Herrmann, Chen Hu, Colin Jessop, Ohannes Kamer-Koseyan, Alexander Ledovskoy, Yasar Onel, Carlos Perez-Lara, Randal Ruchti, Daniel Ruggiero, Daniel Smith, Mark Vigneault, Yuyi Wan, Mitchell Wayne, James Wetzel, Liyuan Zhang and Ren-Yuan ZhuaddShow full author listremoveHide full author list
To address the challenges of providing high-performance calorimetry in future hadron collider experiments under conditions of high luminosity and high radiation (FCC-hh environments), we conducted R&D on advanced calorimetry techniques suitable for s...
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Christopher Betancourt, Dario De Simone, Gregor Kramberger, Maria Manna, Giulio Pellegrini and Nicola Serra
We report on the measurements of time resolution for double-sided 3D pixel sensors with a single cell of 50 μ" role="presentation">µµ
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m ×" role="presentation">××
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50 μ" role="presentation">µµ
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m and thickness of 285 &...
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Lucía Castillo García, Evangelos Leonidas Gkougkousis, Chiara Grieco and Sebastian Grinstein
Low Gain Avalanche Detectors (LGADs) are n-on-p silicon sensors with an extra doped p-layer below the n-p junction which provides signal amplification. The moderate gain of these sensors, together with the relatively thin active region, provides excellen...
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Sergio Ceravolo, Francesco Colao, Camilla Curatolo, Elisa Di Meco, Eleonora Diociaiuti, Donatella Lucchesi, Daniele Paesani, Nadia Pastrone, Gianantonio Pezzullo, Alessandro Saputi, Ivano Sarra, Lorenzo Sestini and Diego Tagnani
Calorimeters, as other detectors, have to face the increasing performance demands of the new energy frontier experiments. For a future Muon Collider the main challenge is given by the Beam Induced Background that may pose limitations to the physics perfo...
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Stefano Perazzini, Fabio Ferrari, Vincenzo Maria Vagnoni and on behalf of the LHCb ECAL Upgrade-2 R&D Group
The increase in instantaneous luminosity during the high-luminosity phase of the LHC represents a significant challenge for future detectors. A strategy to cope with high-pileup conditions is to add a fourth dimension to the measurements of the hits, by ...
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Daniele Paesani, Alessandro Saputi and Ivano Sarra
Measurement of physics processes at new energy frontier experiments requires excellent spatial, time, and energy resolutions to resolve the structure of collimated high-energy jets. In a future Muon Collider, beam-induced backgrounds (BIB) represent the ...
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Simone Michele Mazza
PIONEER is a next-generation experiment to measure the charged pion branching ratios to electrons vs. muons Re/μ=Γπ+→e+ν(γ)Γπ+→μ+ν(γ...
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Lucio Anderlini, Marco Bellini, Chiara Corsi, Stefano Lagomarsino, Chiara Lucarelli, Giovanni Passaleva, Silvio Sciortino and Michele Veltri
Tracking detectors at future high luminosity hadron colliders are expected to be able to stand unprecedented levels of radiation as well as to efficiently reconstruct a huge number of tracks and primary vertices. To face the challenges posed by the radia...
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