12–23 Jul 2021
Online
Europe/Berlin timezone

The Electron-Neutron Detector Array (ENDA), Status and Coincidence with LHAASO

16 Jul 2021, 18:00
1h 30m
TBA

TBA

Talk CRI | Cosmic Ray Indirect Discussion

Speaker

Bingbing Li (College of Physics, Hebei Normal University)

Description

Hadrons are the “skeleton” of extensive air shower (EAS). They possess favorable information concerning the cosmic ray components and energy. The electron-neutron detector (EN-detector) can detect both electrons and thermal neutrons generated by EAS hadrons in surrounding matter. The electron-neutron detector array (ENDA) was proposed to add into the LHAASO project to improve its capability of EAS hybrid detection. Up to present 64 EN-detectors have been produced and are running in China. In 2018, a cluster (of 16 EN-detectors) was installed at Yangbajing (YBJ), Tibet. In 2019, another cluster so called ENDA-16-HZS was installed in LHAASO at Haizishan (HZS), Daocheng, Sichuan. Besides, 2 clusters are tested at Hebei Normal University (HNU), Shijiazhuang, Hebei. ENDA-16-HZS is running normally and get amount of EAS events at energy above 100 TeV. Moreover, a number of coincident events between ENDA and the LHAASO electron detector (ED) and muon detector (MD) arrays composed the KM2A, as well as Cherenkov detectors WFCTA and WCDA are obtained. The events with cores falling into ENDA were selected. The ED array and ENDA accurately offers the EAS directions and the core positions respectively. Both the lateral distributions of neutrons, electrons and muons and the longitudinal development of atmospheric Cherenkov lights are effectively sampled. A hybrid detection of EAS including thermal neutrons, electrons, muons and Cherenkov lights can provide a strong capability of cosmic nuclei discrimination as well as energy measurement with high resolution. In this report, the status of the clusters at the different places are summarized, and the preliminary results of coincident events between ENDA and the LHAASO array are presented.

Subcategory Experimental Methods & Instrumentation
Collaboration Lhaaso

Primary authors

Bingbing Li (College of Physics, Hebei Normal University) Cong Shi (College of Physics, Hebei Normal University) Denis Kuleshov (Institute for Nuclear Research, Russian Academy of Science) Dixuan Xiao (Science School, Tibet University Key Laboratory of Comic Rays, Tibet University, Ministry of Education) Fan Yang (College of Physics, Hebei Normal University) Liangwei Zhang (College of Physics, Hebei Normal University) Liqiao Yin (Institute of High Energy Physics, Chinese Academy of Sciences) Luobu Danzeng (Science School, Tibet University Key Laboratory of Comic Rays, Tibet University, Ministry of Education) Maoyuan Liu (Science School, Tibet University Key Laboratory of Comic Rays, Tibet University, Ministry of Education) Oleg Shchegolev (Institute for Nuclear Research, Russian Academy of Science) Tianlu Chen (Science School, Tibet University Key Laboratory of Comic Rays, Tibet University, Ministry of Education) Vladimir Stepanov (Institute for Nuclear Research, Russian Academy of Science) Xinhua Ma (Institute of High Energy Physics, Chinese Academy of Sciences;TIANFU Cosmic Ray Research Center) Yuri StenKin (Institute for Nuclear Research, Russian Academy of Science) shuwang Cui (Hebei Normal University)

Presentation materials