1.
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The MURAVES muon telescope: a low power consumption muon tracker for muon radiography applications
/ D'Errico, M (CERN ; Naples U. ; INFN, Naples) ; Ambrosino, F (CERN ; Naples U. ; INFN, Naples) ; Baccani, G (Florence U. ; INFN, Florence) ; Bonechi, L (INFN, Florence) ; Bongi, M (Florence U. ; INFN, Florence) ; Bross, A (Fermilab) ; Ciaranfi, R (INFN, Florence) ; Cimmino, L (CERN ; Naples U. ; INFN, Naples) ; Ciulli, V (Florence U. ; INFN, Florence) ; D'Alessandro, R (Florence U. ; INFN, Florence) et al.
Muon Radiography or muography is based on the measurement of the absorption or scattering of cosmic muons, as they pass through the interior of large scale bodies, In particular, absorption muography has been applied to investigate the presence of hidden cavities inside the pyramids or underground, as well as the interior of volcanoes’ edifices. The MURAVES project has the challenging aim of investigating the density distribution inside the summit of Mt. [...]
FERMILAB-CONF-22-961-ND-PPD.-
2022 - 6 p.
- Published in : J. Phys. : Conf. Ser. 2374 (2022) 012190
Fulltext: FERMILAB-CONF-22-961-ND-PPD - PDF; document - PDF; External link: Fermilab Library Server
In : International Conference on Technology and Instrumentation in Particle Physics (TIPP 2021), Online, Canada, 24 - 29 May 2021, pp.012190
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2.
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Long term performance and ageing of CsI photocathodes for the ALICE/HMPID detector
/ Hoedlmoser, H (CERN) ; Braem, André (CERN) ; De Cataldo, G (CERN ; INFN-Sez. di Bari, Bari, Italy) ; Davenport, M (CERN) ; Di Mauro, A (CERN) ; Franco, A (INFN-Sez. di Bari, Bari, Italy) ; Gallas, A (INFN-Sez. di Bari, Bari, Italy) ; Martinengo, P (CERN) ; Nappi, E (INFN-Sez. di Bari, Bari, Italy) ; Piuz, François (CERN) et al.
2007
- Published in : Nucl. Instrum. Methods Phys. Res., A 574 (2007) 28-38
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3.
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RPC-based Muon Identification System for the neutrino detector of the SHiP experiment
/ Albanese, R (INFN, Naples ; Naples U.) ; Alexandrov, A (INFN, Naples) ; Buontempo, S (INFN, Naples) ; Choi, K Y (Sungkyunkwan U.) ; Congedo, L (INFN, Bari ; Bari U.) ; de Asmundis, R (INFN, Naples) ; De Lellis, G (INFN, Naples ; Naples U.) ; de Magistris, M (INFN, Naples ; Naples U.) ; De Robertis, G (INFN, Bari) ; De Serio, M (INFN, Bari ; Bari U.) et al.
The SHiP experiment has been proposed at CERN to shed light
on phenomena still unexplained in the framework of the Standard
Model, such as the nature of dark matter, the baryonic asymmetry of
the Universe and the neutrino oscillations, searching for hints of
New Physics. A section of the detector will be dedicated to the
study of neutrino physics with special emphasis on tau neutrino
properties, still very poorly measured. [...]
2023 - 13 p.
- Published in : JINST 18 (2023) P02022
Fulltext: PDF;
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4.
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Development of radiation hard silicon detectors: the SMART project
/ Messineo, A (INFN sez. di Pisa and Università di Pisa, Italy) ; Borrello, L (INFN sez. di Pisa and Università di Pisa, Italy) ; Segneri, G (INFN sez. di Pisa and Università di Pisa, Italy) ; Sentenac, D (INFN sez. di Pisa and Università di Pisa, Italy) ; Creanza, D (INFN sez. di Bari and Università di Bari, Italy) ; Depalma, M (INFN sez. di Bari and Università di Bari, Italy) ; Manna, N (INFN sez. di Bari and Università di Bari, Italy) ; Radicci, V (INFN sez. di Bari and Università di Bari, Italy) ; Borchi, E (INFN sez. di Firenze and Università di Firenze, Italy) ; Bruzzi, M (INFN sez. di Firenze and Università di Firenze, Italy) et al.
2006
In : 9th ICATPP Conference on Astroparticle, Particle, Space Physics, Detectors and Medical Physics Applications, Como, Italy, 17 - 21 Oct 2005, pp.843-849
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5.
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High granularity resistive Micromegas for high particle rates environment
/ Della Pietra, M (INFN, Naples ; Naples U.) ; Alviggi, M (INFN, Naples ; Naples U.) ; Camerlingo, M T (INFN, Rome3) ; Di Donato, C (INFN, Naples ; Naples U.) ; Di Nardo, R (INFN, Rome3) ; Franchellucci, S (INFN, Rome3) ; Iengo, P (INFN, Naples ; CERN) ; Iodice, M (INFN, Rome3) ; Petrucci, F (INFN, Rome3) ; Sekhniaidze, G (INFN, Naples) et al.
The new era of particle physics experiments is moving towards new upgrades of present accelerators (Large Hadron Collider at CERN) and the design of high energy (tens/hundreds TeV scale) and very high intensity new particle accelerators (FCC-ee/hh, EIC, Muon Collider). Cost effective, high efficiency particle detection in a high background and high radiation environment is fundamental to accomplish their physics program. [...]
2022 - 6 p.
- Published in : JINST 17 (2022) C08002
In : 12th International Conference on Positional Sensitive Detectors, Online, Online, 12 - 17 Sep 2021, pp.C08002
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6.
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Monitoring the long term stability of civil buildings through the MRPC telescopes of the EEE Project
/ Pinto, C (Enrico Fermi Ctr., Rome ; INFN, Catania ; Catania U.) ; Abbrescia, M (INFN, Bari ; Bari U. ; Enrico Fermi Ctr., Rome) ; Avanzini, C (Enrico Fermi Ctr., Rome ; INFN, Pisa ; Pisa U.) ; Baldini, L (INFN, Pisa ; Pisa U. ; Enrico Fermi Ctr., Rome) ; Baldini Ferroli, R (Frascati ; Enrico Fermi Ctr., Rome) ; Batignani, G (INFN, Pisa ; Pisa U. ; Enrico Fermi Ctr., Rome) ; Battaglieri, M (Enrico Fermi Ctr., Rome ; INFN, Genoa ; Genoa U.) ; Boi, S (Enrico Fermi Ctr., Rome ; INFN, Cagliari ; Cagliari U.) ; Bossini, E (Enrico Fermi Ctr., Rome ; INFN, Siena ; Siena U.) ; Carnesecchi, F (Enrico Fermi Ctr., Rome ; INFN, Bologna ; Bologna U.) et al.
Cosmic ray muons are a penetrating component of extensive air showers created in the Earth atmosphere by the interaction of highly energetic primary particles, mostly protons, which continuously bombard our Planet. The secondary cosmic radiation is the result of the complex interplay between the production cross section and the interaction mechanisms with the atmosphere (including the energy loss, multiple scattering and particle decay). [...]
2020 - 10 p.
- Published in : J. Phys.: Conf. Ser. 1561 (2020) 012019
Fulltext: PDF;
In : Detection Systems and Techniques in Nuclear and Particle Physics, Messina, Italy, 11 - 13 Sep 2019, pp.012019
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7.
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An integrated flux-symmetric spectrometer-magnet system for the SND@LHC experiment upgrade
/ SND@LHC Collaboration
The proposed upgrade of the SND@LHC experiment for the High Luminosity phase of the LHC (HL-LHC) will strongly benefit from the presence of a magnetized region, allowing for muon momentum and chargemeasurement. In this paper we describe an iron core magnet system that is partly integrated with the calorimeter and that is designed to respect the strict constraints from the available space in the experimental cavern, power consumption, and field requirements.Semi-analytical tools are introduced to explore the parameter space, in order to define the primary design options. [...]
2024 - 26 p.
- Published in : JINST 19 (2024) P12002
Fulltext: PDF;
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8.
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CaloCube: a novel calorimeter for high-energy cosmic rays in space
/ Calocube Collaboration
In order to extend the direct observation of high-energy cosmic rays up to the PeV region, highly performing calorimeters with large geometrical acceptance and high energy resolution are required. Within the constraint of the total mass of the apparatus, crucial for a space mission, the calorimeters must be optimized with respect to their geometrical acceptance, granularity and absorption depth. [...]
arXiv:1705.07027.-
2017-06-05 - 7 p.
- Published in : JINST 12 (2017) C06004
Fulltext: PDF; Preprint: PDF;
In : Instrumentation for Colliding Beam Physics, Novosibirsk, Russia, 27 Feb - 3 Mar 2017, pp.C06004
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9.
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Mirror system of the RICH detector of the NA62 experiment
/ Aisa, D (Perugia U. ; INFN, Perugia) ; Anzivino, G (Perugia U. ; INFN, Perugia) ; Barbanera, M (Perugia U. ; INFN, Perugia) ; Bizzarri, M (Perugia U. ; INFN, Perugia) ; Bizzeti, A (Modena U. ; INFN, Florence) ; Bucci, F (INFN, Florence) ; Campeggi, C (Perugia U. ; INFN, Perugia) ; Carassiti, V (INFN, Ferrara) ; Cassese, A (Florence U. ; INFN, Florence) ; Cenci, P (INFN, Perugia) et al.
A large RICH detector is used in NA62 to suppress the muon contamination in the charged pion selection by a factor 100 in the momentum range between 15 and 35 GeV/c. The detector consists of a 17 m long tank (vessel), filled with neon gas at atmospheric pressure. [...]
2017 - 23 p.
- Published in : JINST 12 (2017) P12017
Fulltext: pdf - PDF; 10.1088_1748-0221_12_12_P12017 - PDF;
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10.
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