LHAASO-KM2A detector simulation using Geant4
dc.contributor.author | Cao Z. | |
dc.contributor.author | Aharonian F. | |
dc.contributor.author | An Q. | |
dc.contributor.author | Axikegu | |
dc.contributor.author | Bai Y.X. | |
dc.contributor.author | Bao Y.W. | |
dc.contributor.author | Bastieri D. | |
dc.contributor.author | Bi X.J. | |
dc.contributor.author | Bi Y.J. | |
dc.contributor.author | Cai J.T. | |
dc.contributor.author | Cao Q. | |
dc.contributor.author | Cao W.Y. | |
dc.contributor.author | Cao Z. | |
dc.contributor.author | Chang J. | |
dc.contributor.author | Chang J.F. | |
dc.contributor.author | Chen A.M. | |
dc.contributor.author | Chen E.S. | |
dc.contributor.author | Chen L. | |
dc.contributor.author | Chen L. | |
dc.contributor.author | Chen L. | |
dc.contributor.author | Chen M.J. | |
dc.contributor.author | Chen M.L. | |
dc.contributor.author | Chen Q.H. | |
dc.contributor.author | Chen S.H. | |
dc.contributor.author | Chen S.Z. | |
dc.contributor.author | Chen T.L. | |
dc.contributor.author | Chen Y. | |
dc.contributor.author | Cheng N. | |
dc.contributor.author | Cheng Y.D. | |
dc.contributor.author | Cui M.Y. | |
dc.contributor.author | Cui S.W. | |
dc.contributor.author | Cui X.H. | |
dc.contributor.author | Cui Y.D. | |
dc.contributor.author | Dai B.Z. | |
dc.contributor.author | Dai H.L. | |
dc.contributor.author | Dai Z.G. | |
dc.contributor.author | Danzengluobu | |
dc.contributor.author | Dong X.Q. | |
dc.contributor.author | Duan K.K. | |
dc.contributor.author | Fan J.H. | |
dc.contributor.author | Fan Y.Z. | |
dc.contributor.author | Fang J. | |
dc.contributor.author | Fang K. | |
dc.contributor.author | Feng C.F. | |
dc.contributor.author | Feng L. | |
dc.contributor.author | Feng S.H. | |
dc.contributor.author | Feng X.T. | |
dc.contributor.author | Feng Y.L. | |
dc.contributor.author | Gabici S. | |
dc.contributor.author | Gao B. | |
dc.contributor.author | Gao C.D. | |
dc.contributor.author | Gao L.Q. | |
dc.contributor.author | Gao Q. | |
dc.contributor.author | Gao W. | |
dc.contributor.author | Gao W.K. | |
dc.contributor.author | Ge M.M. | |
dc.contributor.author | Geng L.S. | |
dc.contributor.author | Giacinti G. | |
dc.contributor.author | Gong G.H. | |
dc.contributor.author | Gou Q.B. | |
dc.contributor.author | Gu M.H. | |
dc.contributor.author | Guo F.L. | |
dc.contributor.author | Guo X.L. | |
dc.contributor.author | Guo Y.Q. | |
dc.contributor.author | Guo Y.Y. | |
dc.contributor.author | Han Y.A. | |
dc.contributor.author | He H.H. | |
dc.contributor.author | He H.N. | |
dc.contributor.author | He J.Y. | |
dc.contributor.author | He X.B. | |
dc.contributor.author | He Y. | |
dc.contributor.author | Hor Y.K. | |
dc.contributor.author | Hou B.W. | |
dc.contributor.author | Hou C. | |
dc.contributor.author | Hou X. | |
dc.contributor.author | Hu H.B. | |
dc.contributor.author | Hu Q. | |
dc.contributor.author | Hu S.C. | |
dc.contributor.author | Huang D.H. | |
dc.contributor.author | Huang T.Q. | |
dc.contributor.author | Huang W.J. | |
dc.contributor.author | Huang X.T. | |
dc.contributor.author | Huang X.Y. | |
dc.contributor.author | Huang Y. | |
dc.contributor.author | Huang Z.C. | |
dc.contributor.author | Ji X.L. | |
dc.contributor.author | Jia H.Y. | |
dc.contributor.author | Jia K. | |
dc.contributor.author | Jiang K. | |
dc.contributor.author | Jiang X.W. | |
dc.contributor.author | Jiang Z.J. | |
dc.contributor.author | Jin M. | |
dc.contributor.author | Kang M.M. | |
dc.contributor.author | Ke T. | |
dc.contributor.author | Kuleshov D. | |
dc.contributor.author | Kurinov K. | |
dc.contributor.author | Li B.B. | |
dc.contributor.author | Li C. | |
dc.contributor.author | Li C. | |
dc.contributor.author | Li D. | |
dc.contributor.correspondence | Cao Z. | |
dc.contributor.other | Mahidol University | |
dc.date.accessioned | 2024-05-21T18:24:08Z | |
dc.date.available | 2024-05-21T18:24:08Z | |
dc.date.issued | 2024-01-01 | |
dc.description.abstract | KM2A is one of the main sub-arrays of LHAASO, working on gamma ray astronomy and cosmic ray physics at energies above 10 TeV. Detector simulation is the important foundation for estimating detector performance and data analysis. It is a big challenge to simulate the KM2A detector in the framework of Geant4 due to the need to track numerous photons from a large number of detector units (>6000) with large altitude difference (30 m) and huge coverage (1.3 km2). In this paper, the design of the KM2A simulation code G4KM2A based on Geant4 is introduced. The process of G4KM2A is optimized mainly in memory consumption to avoid memory overflow. Some simplifications are used to significantly speed up the execution of G4KM2A. The running time is reduced by at least 30 times compared to full detector simulation. The particle distributions and the core/angle resolution comparison between simulation and experimental data of the full KM2A array are also presented, which show good agreement. | |
dc.identifier.citation | Radiation Detection Technology and Methods (2024) | |
dc.identifier.doi | 10.1007/s41605-024-00467-8 | |
dc.identifier.eissn | 25099949 | |
dc.identifier.issn | 25099930 | |
dc.identifier.scopus | 2-s2.0-85192813670 | |
dc.identifier.uri | https://repository.li.mahidol.ac.th/handle/20.500.14594/98407 | |
dc.rights.holder | SCOPUS | |
dc.subject | Energy | |
dc.subject | Physics and Astronomy | |
dc.title | LHAASO-KM2A detector simulation using Geant4 | |
dc.type | Article | |
mu.datasource.scopus | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85192813670&origin=inward | |
oaire.citation.title | Radiation Detection Technology and Methods | |
oairecerif.author.affiliation | State Key Laboratory of Particle Detection & Electronics | |
oairecerif.author.affiliation | Université Paris Cité | |
oairecerif.author.affiliation | Yunnan Observatories | |
oairecerif.author.affiliation | Nanjing University | |
oairecerif.author.affiliation | Shanghai Astronomical Observatory Chinese Academy of Sciences | |
oairecerif.author.affiliation | Institute for Nuclear Research of the Russian Academy of Sciences | |
oairecerif.author.affiliation | Shandong University | |
oairecerif.author.affiliation | Yunnan University | |
oairecerif.author.affiliation | Institute of High Energy Physics, Chinese Academy of Sciences | |
oairecerif.author.affiliation | University of Chinese Academy of Sciences | |
oairecerif.author.affiliation | Guangzhou University | |
oairecerif.author.affiliation | Tsinghua University | |
oairecerif.author.affiliation | Shanghai Jiao Tong University | |
oairecerif.author.affiliation | Sun Yat-Sen University | |
oairecerif.author.affiliation | University of Science and Technology of China | |
oairecerif.author.affiliation | Zhengzhou University | |
oairecerif.author.affiliation | Institiúid Ard-Lénn Bhaile Átha Cliath | |
oairecerif.author.affiliation | Sichuan University | |
oairecerif.author.affiliation | National Astronomical Observatories Chinese Academy of Sciences | |
oairecerif.author.affiliation | Max-Planck-Institut für Kernphysik | |
oairecerif.author.affiliation | Southwest Jiaotong University | |
oairecerif.author.affiliation | Purple Mountain Observatory Chinese Academy of Sciences | |
oairecerif.author.affiliation | Hebei Normal University | |
oairecerif.author.affiliation | Tibet University | |
oairecerif.author.affiliation | Moscow Institute of Physics and Technology | |
oairecerif.author.affiliation | TIANFU Cosmic Ray Research Center |