The CYGNO experiment, a directional detector for direct Dark Matter searches

被引：3

作者：

Amaro, Fernando Domingues ^{[1
]}

Baracchini, Elisabetta ^{[2
,3
]}

Benussi, Luigi ^{[4
]}

Bianco, Stefano ^{[4
]}

Capoccia, Cesidio ^{[4
]}

Caponero, Michele ^{[4
,5
]}

Cardoso, Danilo Santos ^{[6
]}

Cavoto, Gianluca ^{[7
]}

Cortez, Andre ^{[2
,3
]}

Costa, Igor Abritta ^{[9
,10
]}

Dane, Emiliano ^{[4
]}

Dho, Giorgio ^{[2
,3
]}

Di Giambattista, Flaminia ^{[2
,3
]}

Di Marco, Emanuele ^{[8
]}

D'Imperio, Giulia ^{[8
]}

Iacoangeli, Francesco ^{[8
]}

Lima Junior, Herman Pessoa ^{[6
]}

Lopes, Guilherme Sebastiao Pinheiro ^{[11
]}

Maccarrone, Giovanni ^{[4
]}

Mano, Rui Daniel Passos ^{[1
]}

Gregorio, Robert Renz Marcelo ^{[12
]}

Marques, David Jose Gaspar ^{[2
,3
]}

Mazzitelli, Giovanni ^{[4
]}

Mclean, Alasdair Gregor ^{[12
]}

Messina, Andrea ^{[7
,8
]}

Monteiro, Cristina Maria Bernardes

Nobrega, Rafael Antunes

Pains, Igor Fonseca

Paoletti, Emiliano

Passamonti, Luciano

Pelosi, Sandro

Petrucci, Fabrizio

Piacentini, Stefano

Piccolo, Davide

Pierluigi, Daniele

Pinci, Davide

Prajapati, Atul

Renga, Francesco

Roque, Rita Joanna da Cruz

Rosatelli, Filippo

Russo, Alessandro

dos Santos, Joaquim Marques Ferreira ^{[1
]}

Saviano, Giovanna ^{[4
,13
]}

Spooner, Neil John Curwen ^{[12
]}

Tesauro, Roberto ^{[4
]}

Tommasini, Sandro ^{[4
]}

Torelli, Samuele ^{[2
,3
]}

机构：

[1] Univ Coimbra, Dept Phys, LIBPhys, P-3004516 Coimbra, Portugal

[2] Gran Sasso Sci Inst, I-67100 Laquila, Italy

[3] Ist Nazl Fis Nucleare, Lab Nazl Gran Sasso, I-67100 Assergi, Italy

[4] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy

[5] ENEA Ctr Ric Frascati, I-00044 Frascati, Italy

[6] Ctr Brasileiro Pesquisas Fis, BR-22290180 Rio De Janeiro, RJ, Brazil

[7] Univ Sapienza Roma, Dipartimento Fis, I-00185 Rome, Italy

[8] Ist Nazl Fis Nucleare, Sez Roma, I-00185 Rome, Italy

[9] Univ Roma Tre, Dipartimento Matemat & Fis, I-00146 Rome, Italy

[10] Ist Nazl Fis Nucl, Sez Roma Tre, I-00146 Rome, Italy

[11] Univ Fed Juiz De Fora, Fac Engn, BR-36036900 Juiz De Fora, MG, Brazil

[12] Univ Sheffield, Dept Phys & Astron, Sheffield S3 7RH, England

[13] Sapienza Univ Roma, Dipartimento Ingn Chim Mat & Ambiente, I-00185 Rome, Italy

来源：

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2023年 / 1054卷

关键词：

Dark matter; Time projection chamber; Optical readout;

D O I：

10.1016/j.nima.2023.168325

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

The CYGNO project aims at the development of a high precision optical readout gaseous Tima Projection Chamber (TPC) for directional dark matter (DM) searches, to be hosted at Laboratori Nazionali del Gran Sasso (LNGS). CYGNO employs a He:CF4 gas mixture at atmospheric pressure with a Gas Electron Multiplier (GEM) based amplification structure coupled to an optical readout comprised of sCMOS cameras and photomultiplier tubes (PMTs). This experimental setup allows to achieve 3D tracking and background rejection down to O(1) keV energy, to boost sensitivity to low WIMP masses. The characteristics of the optical readout approach in terms of the light yield will be illustrated along with the particle identification properties. The project timeline foresees, in the next 2-3 years, the realisation and installation of a 0.4 m3 TPC in the underground laboratories at LNGS to act as a demonstrator. Finally, the studies of the expected DM sensitivities of the CYGNO demonstrator will be presented.

引用

页数：3

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