The CYGNO/INITIUM experiment-Reference-Cited by-同舟云学术

The CYGNO/INITIUM experiment

Published:2023-07-03 Issue:12 Volume: Page:
ISSN:2666-4003
Container-title:SciPost Physics Proceedings
language:
Short-container-title:SciPost Phys. Proc.

Author:

Amaro F. D.¹,Baracchini Elisabetta²³,Benussi L.⁴,Bianco S.⁴,Capoccia C.⁴,Caponero M.⁴⁵,Santos Cardoso D.⁶,Cavoto Gianluca⁷,Cortez A.²³,Costa I. A.⁸⁹,Dané E.⁴,Dho Giorgio²³,Di Giambattista F.²³,Di Marco E.¹⁰,D’Imperio G.¹⁰,Iacoangeli F.¹⁰,Jùnior H. P.⁶,Lopes G. S. P.¹,Maccarrone G.⁴,Mano R. D. P.¹,Gregorio R. R. M.¹¹,Marques D. J. G.²³,Mazzitelli G.⁴,McLean A. G.¹¹,Messina A.¹⁰⁷,Monteiro C. M. B.¹,Nobrega R. A.¹²,Fonseca Pains I.¹²,Paoletti E.⁴,Passamonti L.⁴,Pelosi S.¹⁰,Petrucci F.⁸⁹,Piacentini S.¹⁰⁷,Piccolo D.⁴,Pierluigi D.⁴,Pinci D.¹⁰,Prajapati A.²³,Renga F.¹⁰,Roque R. J. C.¹,Rosatelli F.⁴,Russo A.⁴,dos Santos J. M. F.¹,Saviano G.⁴⁷,Spooner N. J. C.¹¹,Tesauro R.⁴,Tommasini S.⁴,Torelli S.²³

Affiliation:

1. University of Coimbra

2. Gran Sasso National Laboratory

3. Gran Sasso Science Institute

4. National Accelerator Laboratory at Frascati

5. National Agency for New Technologies, Energy and Sustainable Economic Development

6. Brazilian Center for Research in Physic

7. Sapienza University of Rome

8. INFN Sezione di Roma III

9. Roma Tre University

10. INFN Sezione di Roma-1

11. University of Sheffield

12. Juiz de Fora Federal University

Abstract

The CYGNO project for the development of a high precision optical readout gaseous TPC for directional Dark Matter search and solar neutrino spectroscopy will be presented. It is to be hosted at Laboratori Nazionali del Gran Sasso. CYGNO peculiar features are the use of sCMOS cameras and PMTs coupled to GEMs amplification of a helium-based gas mixture at atmospheric pressure, in order to achieve 3D tracking with head tail capability and background rejection down to O(keV) energy, to boost sensitivity to low WIMP masses. The latest R&D results within the CYGNO project will be discussed along with the underground installation and operation of a 50 l prototype, soon to be followed by a O(1) m3 experiment demonstrator in 2024-2026. The latest results on the negative ion drift operation at atmospheric pressure within CYGNO optical readout approach will be illustrated, which is the aim of the ERC Consolidator Grant project INITIUM.

Funder

Horizon 2020

Publisher

Stichting SciPost

Subject

General Medicine

Link

https://scipost.org/10.21468/SciPostPhysProc.12.019/pdf

Reference8 articles.

1. INTRODUCTION TO DARK MATTER EXPERIMENTS

2. A review of the discovery reach of directional Dark Matter detection

3. How high is the neutrino floor?

4. New Definition of the Neutrino Floor for Direct Dark Matter Searches

5. The CYGNO Experiment