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1.
High latitude observation of the Forbush decrease during the May 2024 solar storms with muon and neutron detectors on Svalbard / Riggi, F (Unlisted, IT ; INFN, Catania ; U. Catania (main)) ; Hertle, L (Unlisted, DE) ; Abbrescia, M (Bari U. ; INFN, Bari) ; Avanzini, C (U. Pisa (main) ; INFN, Pisa) ; Baldini, L (U. Pisa (main) ; INFN, Pisa) ; Baldini Ferroli, R (Frascati) ; Batignani, G (U. Pisa (main) ; INFN, Pisa ; Unlisted, IT) ; Battaglieri, M (INFN, Genoa) ; Boi, S (U. Cagliari (main) ; INFN, Cagliari) ; Boike, J (Unlisted, DE ; Humboldt U., Berlin (main)) et al.
During the series of intense solar flares and coronal mass ejections, that occurred in May 2024, a remarkable Forbush decrease in the cosmic ray flux was observed on the Earth. While this event was observed by particle detectors around the world, the archipelago of Svalbard was heavily exposed to it due to the weak geomagnetic shielding in the polar region. [...]
2025 - 15 p. - Published in : Adv. Space Res. 76 (2025) 1225-1239
2.
Measurement of the muon flux in the tunnels of Doss Trento hill / Abbrescia, M (Bari U. ; INFN, Bari) ; Avanzini, C (INFN, Pisa ; Pisa U.) ; Baldini, L (Pisa U. ; INFN, Pisa) ; Ferroli, R Baldini (Frascati) ; Batignani, G (Pisa U. ; INFN, Pisa ; Enrico Fermi Ctr., Rome) ; Battaglieri, M (INFN, Genoa) ; Battiston, R (Trento U. ; TIFPA-INFN, Trento) ; Bimbi, S (Rome U.) ; Boi, S (INFN, Cagliari) ; Bossini, E (INFN, Pisa) et al.
In the context of astroparticle physics, nuclear astrophysics and quantum computing projects, it is important identifying underground laboratories where the cosmogenic background is suppressed. Located about 500 m far from the center of Trento (Italy) the Piedicastello tunnels are covered by 100 m limestone rock of the Doss Trento hill. [...]
2024 - 9 p. - Published in : Nucl. Instrum. Methods Phys. Res., A 1072 (2025) 170163 Fulltext: PDF;
3.
Quality Assurance and Quality Control of the $26~\text{m}^2$ SiPM production for the DarkSide-20k dark matter experiment / DarkSide-20k Collaboration
DarkSide-20k is a novel liquid argon dark matter detector currently under construction at the Laboratori Nazionali del Gran Sasso (LNGS) of the Istituto Nazionale di Fisica Nucleare (INFN) that will push the sensitivity for Weakly Interacting Massive Particle (WIMP) detection into the neutrino fog. [...]
arXiv:2412.18867.
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Fulltext
4.
First results on new helium based eco-gas mixtures for the Extreme Energy Events Project / EEE Collaboration
The Extreme Energy Events (EEE) Project, a joint project of the Centro Fermi (Museo Storico della Fisica e Centro Studi e Ricerche "E.Fermi") and INFN, has a dual purpose: a scientific research program on cosmic rays at ground level and an intense outreach and educational program. The project consists in a network of about 60 tracking detectors, called telescopes, mostly hosted in Italian High Schools. [...]
arXiv:2408.01802.- 2024-11-11 - 12 p. - Published in : JINST 19 (2024) P11003 Fulltext: 2408.01802 - PDF; document - PDF;
5.
Ecological transition for the gas mixtures of the MRPC cosmic ray telescopes of the EEE Project / EEE Collaboration
The Extreme Energy Events (EEE) Collaboration is fully involved in an ecological transition. The use of the standard gas mixture, \ce{C_2H_2F_4}+ \ce{SF_6}, has stopped in favor of an alternative green mixture based on \ce{C_3H_2F_4} with the addition of He or \ce{CO_2}. [...]
arXiv:2309.17375.- 2024-03-27 - 5 p. - Published in : JINST 19 (2024) C03060 Fulltext: document - PDF; 2309.17375 - PDF;
6.
The ecological transition of the extreme energy events experiment / Abbrescia, M (Bari U. ; INFN, Bari) ; Avanzini, C (Pisa U.) ; Baldini, L (Pisa U.) ; Baldini Ferroli, R (Frascati) ; Batignani, G (Pisa U.) ; Battaglieri, M (INFN, Genoa) ; Boi, S (Cagliari U.) ; Bossini, E (Pisa U.) ; Carnesecchi, F (CERN) ; Cavazza, F (INFN, Bologna) et al.
The need for reducing the emission of gases, potentially contributing to the greenhouse effect and climate change, has impacted many fields, including scientific research. The Extreme Energy Event (EEE) collaboration started, already several years ago, a series of tests aiming at finding a more eco-friendly replacement for the gases used in the Multigap Resistive Plate Chambers (MRPCs) of its network. [...]
2023 - 4 p.

In : 16th Workshop on Resistive Plate Chambers and Related Detectors (RPC 2022), CERN, Geneva, Switzerland, 26-30 Sep 2022, pp.168431
7.
Simulation tool for MRPC telescopes of EEE experiment / Mandaglio, G (INFN, Messina ; Messina U. ; INFN, Catania) ; Abbrescia, M (Bari U. ; INFN, Bari) ; Avanzini, C (INFN, Pisa) ; Baldini, L (INFN, Pisa ; Pisa U.) ; Ferroli, R Baldini (Frascati) ; Batignani, G (INFN, Pisa ; Pisa U.) ; Battaglieri, M (INFN, Genoa ; Genoa U. ; Jefferson Lab) ; Boi, S (Cagliari U. ; INFN, Cagliari) ; Bossini, E (INFN, Pisa ; Pisa U.) ; Carnesecchi, F (INFN, Bologna ; Bologna U.) et al.
The Extreme Energy Events (EEE) experiment consists in a network of cosmic muon tracker telescopes, each made of three Multi-gap Resistive Plate Chambers (MRPC), able to precisely measure the absolute muon crossing time and the muon integrated angular flux at the ground level. To investigate the MRPC telescope response and performance, a simulation tool was developed in GEMC, software package based on GEANT4 libraries. [...]
2022 - 4 p. - Published in : J. Phys. : Conf. Ser. 2374 (2022) 012051 Fulltext: PDF;
In : International Conference on Technology and Instrumentation in Particle Physics (TIPP 2021), Online, Canada, 24 - 29 May 2021, pp.012051
8.
Reduction of Greenhouse Gases impact in the EEE Project / Ripoli, C (Salerno U. ; INFN, Salerno) ; Abbrescia, M (Bari U. ; INFN, Bari) ; Avanzini, C (INFN, Pisa) ; Baldini, L (INFN, Pisa ; Pisa U.) ; Ferroli, R Baldini (Frascati) ; Batignani, G (INFN, Pisa ; Pisa U.) ; Battaglieri, M (INFN, Genoa ; Jefferson Lab) ; Boi, S (Cagliari U. ; INFN, Cagliari) ; Bossini, E (INFN, Pisa ; Pisa U.) ; Carnesecchi, F (INFN, Bologna ; U. Bologna, DIFA) et al.
The whole Extreme Energy Events (EEE) array is composed of 61 telescopes installed in Italian High Schools, built and operated by students and teachers, constantly supervised by researchers. The muon telescope of the EEE Project is made by 3 Multigap Resistive Plate Chambers (MRPC). [...]
2022 - 4 p. - Published in : J. Phys. : Conf. Ser. 2374 (2022) 012152 Fulltext: PDF;
In : International Conference on Technology and Instrumentation in Particle Physics (TIPP 2021), Online, Canada, 24 - 29 May 2021, pp.012152
9.
Measurements of the Cherenkov effect in direct detection of charged particles with SiPMs / Carnesecchi, F. (CERN) ; Sabiu, B. (Bologna U. ; INFN, Bologna) ; Strazzi, S. (Bologna U. ; INFN, Bologna) ; Vignola, G. (INFN, Bologna) ; Agrawal, N. (Bologna U. ; INFN, Bologna) ; Alici, A. (Bologna U. ; INFN, Bologna) ; Antonioli, P. (INFN, Bologna) ; Arcelli, S. (Bologna U. ; INFN, Bologna) ; Bellini, F. (Bologna U. ; INFN, Bologna) ; Cavazza, D. (INFN, Bologna) et al.
In this paper, different Silicon PhotoMultiplier (SiPM) sensors have been tested with charged particles to characterize the Cherenkov light produced in the sensor protection layer. A careful position scan of the SiPM response has been performed with different prototypes, confirming the large number of firing cells and proving almost full efficiency, with the SiPM filling factor essentially negligible. [...]
arXiv:2305.17762.- 2023-09-05 - Published in : Eur. Phys. J. Plus 138 (2023) 788 Fulltext: 2305.17762 - PDF; document - PDF;
10.
Measurement of the cosmic charged particle rate at sea level in the latitude range 35$^{\circ }\div $ 82$^{\circ }$ N with the PolarquEEEst experiment / Abbrescia, M (Bari U. ; INFN, Bari) ; Avanzini, C (Pisa U.) ; Baldini, L (Pisa U.) ; Ferroli, R Baldini (Frascati) ; Batignani, G (Pisa U.) ; Battaglieri, M (INFN, Genoa) ; Boi, S (Cagliari U. ; INFN, Cagliari) ; Bossini, E (Pisa U.) ; Carnesecchi, F (CERN) ; Cavazza, D (INFN, Bologna) et al.
After its successful campaign of measurements beyond the Polar Arctic Circle, the PolarquEEEst experiment measured the cosmic charged particle rate at sea level in a latitude interval between 35$^{\circ }$ N and 82$^{\circ }$ N. In this paper, these measurements are described and the corresponding results are discussed..
2023 - 9 p. - Published in : Eur. Phys. J. C 83 (2023) 293 Fulltext: PDF;

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