arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 2001.02453physics.ins-dethep-ex
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A 1 m$^3$ Gas Time Projection Chamber with Optical Readout for Directional Dark Matter Searches: the CYGNO Experiment

E. Baracchini, R. Bedogni, F. Bellini, L. Benussi, S. Bianco, C. Capoccia, M. Caponero, G. Cavoto, I. A. Costa, E. Di Marco, G. D'Imperio, F. Iacoangeli, G. Mac… 展开作者

E. Baracchini, R. Bedogni, F. Bellini, L. Benussi, S. Bianco, C. Capoccia, M. Caponero, G. Cavoto, I. A. Costa, E. Di Marco, G. D'Imperio, F. Iacoangeli, G. Maccarone, M. Marafini, G. Mazzitelli, A. Messina, A. Orlandi, E. Paoletti, L. Passamonti, A. Pelosi, F. Petrucci, D. Piccolo, D. Pierluigi, D. Pinci, F. Renga, A. Russo, G. Saviano, S. Tomassini

英文摘要:

The aim of the CYGNO project is the construction and operation of a 1~m$^3$ gas TPC for directional dark matter searches and coherent neutrino scattering measurements, as a prototype toward the 100-1000~m$^3$ (0.15-1.5 tons) CYGNUS network of underground experiments. In such a TPC, electrons produced by dark-matter- or neutrino-induced nuclear recoils will drift toward and will be multiplied by a three-layer GEM structure, and the light produced in the avalanche processes will be readout by a sCMOS camera, providing a 2D image of the event with a resolution of a few hundred micrometers. Photomultipliers will also provide a simultaneous fast readout of the time profile of the light production, giving information about the third coordinate and hence allowing a 3D reconstruction of the event, from which the direction of the nuclear recoil and consequently the direction of the incoming particle can be inferred. Such a detailed reconstruction of the event topology will also allow a pure and efficient signal to background discrimination. These two features are the key to reach and overcome the solar neutrino background that will ultimately limit non-directional dark matter searches.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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