Articolo in rivista, 2020, ENG, 10.1088/1742-6596/1498/1/012008
Chatterjee C.; Cicala G.; Cicuttin A.; Ciliberti P.; Crespo M.L.; Dalla Torre S.; Dasgupta S.; Gregori M.; Levorato S.; Menon G.; Tessarotto F.; Triloki; Valentini A.; Velardi L.; Zhao Y.X.
INFN Trieste, Italy; University of Trieste, Italy; University Aldo Moro of Bari, INFN Bari, Italy; CNR-ISTP Sede di Bari, Italy; Abdus Salam ICTP, Trieste, Italy.
The design of a Ring Imaging CHerenkov (RICH) detector for the identification of high momentum particles at the future Electron Ion Collider (EIC) is extremely challenging by using current technology. Compact collider setups impose to construct RICH with short radiator length, hence limiting the number of generated photons. The number of detected photons can be increased by selecting the far UV region. As standard fused-silica windows is opaque below 165 nm, a windowless RICH can be a possible approach. CsI is widely used photocathode (PC) for photon detection in the far UV range. Due to its hygroscopic nature it is very delicate to handle. In addition, its Quantum Effciency (QE) degrades in high intensity ion fluxes. These are the key reasons to quest for novel PC with sensitivity in the far UV region. Recent development of layers of hydrogenated nanodiamond powders as an alternative PC material and their performance, when coupled to the THick Gaseous Electron Multipliers (THGEM)-based detectors, are the objects of an ongoing R&D. We report here some preliminary results on the initial phase of these studies.
Journal of physics. Conference series (Print) 1498 (1), pp. 012008-1–012008-6
Nanodiamond particle, UV photocathode, THGEM
ID: 429722
Year: 2020
Type: Articolo in rivista
Creation: 2020-09-03 16:24:26.000
Last update: 2023-02-03 16:57:00.000
CNR authors
CNR institutes
External links
OAI-PMH: Dublin Core
OAI-PMH: Mods
OAI-PMH: RDF
DOI: 10.1088/1742-6596/1498/1/012008
URL: https://iopscience.iop.org/article/10.1088/1742-6596/1498/1/012008/meta
External IDs
CNR OAI-PMH: oai:it.cnr:prodotti:429722
DOI: 10.1088/1742-6596/1498/1/012008
Scopus: 2-s2.0-85086721049
ISI Web of Science (WOS): 000577272600052