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Directional Dark Matter Searches with CYGNO

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LIBPhys, Department of Physics, University of Coimbra, 3004-516 Coimbra, Portugal
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Gran Sasso Science Institute, 67100 L’Aquila, Italy
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Laboratori Nazionali del Gran Sasso, Istituto Nazionale di Fisica Nucleare, 67100 Assergi, Italy
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Laboratori Nazionali di Frascati, Istituto Nazionale di Fisica Nucleare, 00044 Frascati, Italy
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ENEA Centro Ricerche Frascati, 00044 Frascati, Italy
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Istituto Nazionale di Fisica Nucleare, Sezione di Roma, 00185 Rome, Italy
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Dipartimento di Fisica, Università La Sapienza di Roma, 00185 Roma, Italy
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Faculdade de Engenharia, Universidade Federal de Juiz de Fora, Juiz de Fora 36036-900, MG, Brazil
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Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, UK
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Brazilian Center for Research in Physics, Rio de Janeiro 22290-180, RJ, Brazil
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Museo Storico della Fisica e Centro Studi e Ricerche “Enrico Fermi”, Piazza del Viminale 1, 00184 Roma, Italy
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Dipartimento di Matematica e Fisica, Università Roma TRE, 00146 Roma, Italy
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Istituto Nazionale di Fisica Nucleare, Sezione di Roma TRE, 00146 Roma, Italy
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Dipartimento di Ingegneria Chimica, Materiali e Ambiente, Sapienza Università di Roma, 00185 Roma, Italy
*
Author to whom correspondence should be addressed.
Academic Editors: Diego González-Díaz and Paul Colas
Particles 2021, 4(3), 343-353; https://doi.org/10.3390/particles4030029
Received: 31 May 2021 / Revised: 1 July 2021 / Accepted: 3 July 2021 / Published: 6 July 2021
(This article belongs to the Special Issue Selected Papers from "New Horizons in Time Projection Chambers")
The CYGNO project aims at developing a high resolution Time Projection Chamber with optical readout for directional dark matter searches and solar neutrino spectroscopy. Peculiar CYGNO’s features are the 3D tracking capability provided by the combination of photomultipliers and scientific CMOS camera signals, combined with a helium-fluorine-based gas mixture at atmospheric pressure amplified by gas electron multipliers structures. In this paper, the performances achieved with CYGNO prototypes and the prospects for the upcoming underground installation at Laboratori Nazionali del Gran Sasso of a 50-L detector in fall 2021 will be discussed, together with the plans for a 1-m3 experiment. The synergy with the ERC consolidator, grant project INITIUM, aimed at realising negative ion drift operation within the CYGNO 3D optical approach, will be further illustrated. View Full-Text
Keywords: dark matter; time projection chamber; optical readout; electroluminescence; negative ion drift dark matter; time projection chamber; optical readout; electroluminescence; negative ion drift
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MDPI and ACS Style

Amaro, F.D.; Baracchini, E.; Benussi, L.; Bianco, S.; Capoccia, C.; Caponero, M.; Cavoto, G.; Cortez, A.; Costa, I.A.; Dané, E.; Dho, G.; Di Marco, E.; D’Imperio, G.; Di Giambattista, F.; Gregorio, R.R.M.; Iacoangeli, F.; Lima Júnior, H.P.; Silva Lopes Júnior, A.d.; Maccarrone, G.; Mano, R.D.P.; Marafini, M.; Mazzitelli, G.; McLean, A.G.; Messina, A.; Bernardes Monteiro, C.M.; Nobrega, R.A.; Pains, I.F.; Paoletti, E.; Passamonti, L.; Pelosi, S.; Petrucci, F.; Piacentini, S.; Piccolo, D.; Pierluigi, D.; Pinci, D.; Prajapati, A.; Renga, F.; Cruz Roque, R.J.d.; Rosatelli, F.; Russo, A.; Santos, J.M.F.d.; Saviano, G.; Spooner, N.; Tesauro, R.; Tomassini, S.; Torelli, S. Directional Dark Matter Searches with CYGNO. Particles 2021, 4, 343-353. https://doi.org/10.3390/particles4030029

AMA Style

Amaro FD, Baracchini E, Benussi L, Bianco S, Capoccia C, Caponero M, Cavoto G, Cortez A, Costa IA, Dané E, Dho G, Di Marco E, D’Imperio G, Di Giambattista F, Gregorio RRM, Iacoangeli F, Lima Júnior HP, Silva Lopes Júnior Ad, Maccarrone G, Mano RDP, Marafini M, Mazzitelli G, McLean AG, Messina A, Bernardes Monteiro CM, Nobrega RA, Pains IF, Paoletti E, Passamonti L, Pelosi S, Petrucci F, Piacentini S, Piccolo D, Pierluigi D, Pinci D, Prajapati A, Renga F, Cruz Roque RJd, Rosatelli F, Russo A, Santos JMFd, Saviano G, Spooner N, Tesauro R, Tomassini S, Torelli S. Directional Dark Matter Searches with CYGNO. Particles. 2021; 4(3):343-353. https://doi.org/10.3390/particles4030029

Chicago/Turabian Style

Amaro, Fernando D., Elisabetta Baracchini, Luigi Benussi, Stefano Bianco, Cesidio Capoccia, Michele Caponero, Gianluca Cavoto, André Cortez, Igor A. Costa, Emiliano Dané, Giorgio Dho, Emanuele Di Marco, Giulia D’Imperio, Flaminia Di Giambattista, Robert R.M. Gregorio, Francesco Iacoangeli, Herman P. Lima Júnior, Amaro d. Silva Lopes Júnior, Giovanni Maccarrone, Rui D.P. Mano, Michela Marafini, Giovanni Mazzitelli, Alasdair G. McLean, Andrea Messina, Cristina M. Bernardes Monteiro, Rafael A. Nobrega, Igor F. Pains, Emiliano Paoletti, Luciano Passamonti, Sandro Pelosi, Fabrizio Petrucci, Stefano Piacentini, Davide Piccolo, Daniele Pierluigi, Davide Pinci, Atul Prajapati, Francesco Renga, Rita J.d. Cruz Roque, Filippo Rosatelli, Andrea Russo, Joaquim M.F.d. Santos, Giovanna Saviano, Neil Spooner, Roberto Tesauro, Sandro Tomassini, and Samuele Torelli. 2021. "Directional Dark Matter Searches with CYGNO" Particles 4, no. 3: 343-353. https://doi.org/10.3390/particles4030029

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