Measurement of the cosmic ray proton spectrum around the knee region with LHAASO

dc.contributor.authorZhiyong Y.
dc.contributor.authorShoushan Z.
dc.contributor.authorLiqiao Y.
dc.contributor.authorLingling M.
dc.contributor.authorZhen C.
dc.contributor.authorYudong W.
dc.contributor.authorCao Z.
dc.contributor.authorAharonian F.
dc.contributor.authorAn Q.
dc.contributor.authorAxikegu
dc.contributor.authorBai L.X.
dc.contributor.authorBai Y.X.
dc.contributor.authorBai L.X.
dc.contributor.authorBai Y.X.
dc.contributor.authorBao Y.W.
dc.contributor.authorBastieri D.
dc.contributor.authorBi X.J.
dc.contributor.authorBi Y.J.
dc.contributor.authorCai H.
dc.contributor.authorCai J.T.
dc.contributor.authorCao Z.
dc.contributor.authorChang J.
dc.contributor.authorChang J.F.
dc.contributor.authorChen B.M.
dc.contributor.authorChen E.S.
dc.contributor.authorChen J.
dc.contributor.authorChen L.
dc.contributor.authorChen L.
dc.contributor.authorChen L.
dc.contributor.authorChen M.J.
dc.contributor.authorChen M.L.
dc.contributor.authorChen Q.H.
dc.contributor.authorChen S.H.
dc.contributor.authorChen S.Z.
dc.contributor.authorChen T.L.
dc.contributor.authorChen X.L.
dc.contributor.authorChen Y.
dc.contributor.authorCheng N.
dc.contributor.authorCheng Y.D.
dc.contributor.authorCui S.W.
dc.contributor.authorCui X.H.
dc.contributor.authorCui Y.D.
dc.contributor.authorD’Ettorre Piazzoli B.
dc.contributor.authorDai B.Z.
dc.contributor.authorDai H.L.
dc.contributor.authorDai Z.G.
dc.contributor.authorDanzengluobu
dc.contributor.authordella Volpe D.
dc.contributor.authorDong X.J.
dc.contributor.authorDuan K.K.
dc.contributor.authorFan J.H.
dc.contributor.authorFan Y.Z.
dc.contributor.authorFan Z.X.
dc.contributor.authorFang J.
dc.contributor.authorFang K.
dc.contributor.authorFeng C.F.
dc.contributor.authorFeng L.
dc.contributor.authorFeng S.H.
dc.contributor.authorFeng Y.L.
dc.contributor.authorGao B.
dc.contributor.authorGao C.D.
dc.contributor.authorGao L.Q.
dc.contributor.authorGao Q.
dc.contributor.authorGao W.
dc.contributor.authorGe M.M.
dc.contributor.authorGeng L.S.
dc.contributor.authorGong G.H.
dc.contributor.authorGou Q.B.
dc.contributor.authorGu M.H.
dc.contributor.authorGuo F.L.
dc.contributor.authorGuo J.G.
dc.contributor.authorGuo X.L.
dc.contributor.authorGuo Y.Q.
dc.contributor.authorGuo Y.Y.
dc.contributor.authorHan Y.A.
dc.contributor.authorHe H.H.
dc.contributor.authorHe H.N.
dc.contributor.authorHe J.C.
dc.contributor.authorHe S.L.
dc.contributor.authorHe X.B.
dc.contributor.authorHe Y.
dc.contributor.authorHeller M.
dc.contributor.authorHor Y.K.
dc.contributor.authorHou C.
dc.contributor.authorHu H.B.
dc.contributor.authorHu S.
dc.contributor.authorHu S.C.
dc.contributor.authorHu X.J.
dc.contributor.authorHuang D.H.
dc.contributor.authorHuang Q.L.
dc.contributor.authorHuang W.H.
dc.contributor.authorHuang X.T.
dc.contributor.authorHuang X.Y.
dc.contributor.authorHuang Z.C.
dc.contributor.authorJi F.
dc.contributor.authorJi X.L.
dc.contributor.authorJia H.Y.
dc.contributor.authorJiang K.
dc.contributor.authorJiang Z.J.
dc.contributor.authorJin C.
dc.contributor.correspondenceZhiyong Y.
dc.contributor.otherMahidol University
dc.date.accessioned2024-12-23T18:15:39Z
dc.date.available2024-12-23T18:15:39Z
dc.date.issued2024-09-27
dc.description.abstractOne of the main scientific aims of LHAASO is to measure the energy spectra of cosmic rays for individual mass compositions. LHAASO is made up of three detector arrays, which are WFCTA, KM2A, and WCDA. The three detector arrays can achieve hybrid observation, so several extensive air shower observables that are sensitive to mass compositions can be measured simultaneously. ROOT-TMVA package is used to combine these component-sensitive parameters for selecting proton events. The selected proton events have a purity of over 90%. In this paper, we have selected simulated events with shower cores located in the KM2A array to investigate the feasibility of the analysis method for studying the proton energy spectrum. We have also studied the associated systematic uncertainties, including those introduced by the composition models, proton selection, energy reconstruction method, and hadronic interaction models.
dc.identifier.citationProceedings of Science Vol.444 (2024)
dc.identifier.eissn18248039
dc.identifier.scopus2-s2.0-85212278401
dc.identifier.urihttps://repository.li.mahidol.ac.th/handle/20.500.14594/102483
dc.rights.holderSCOPUS
dc.subjectMultidisciplinary
dc.titleMeasurement of the cosmic ray proton spectrum around the knee region with LHAASO
dc.typeConference Paper
mu.datasource.scopushttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85212278401&origin=inward
oaire.citation.titleProceedings of Science
oaire.citation.volume444
oairecerif.author.affiliationState Key Laboratory of Particle Detection & Electronics
oairecerif.author.affiliationNanjing University
oairecerif.author.affiliationShanghai Astronomical Observatory Chinese Academy of Sciences
oairecerif.author.affiliationShandong University
oairecerif.author.affiliationWuhan University
oairecerif.author.affiliationYunnan University
oairecerif.author.affiliationInstitute of High Energy Physics, Chinese Academy of Sciences
oairecerif.author.affiliationUniversity of Chinese Academy of Sciences
oairecerif.author.affiliationGuangzhou University
oairecerif.author.affiliationTsinghua University
oairecerif.author.affiliationSun Yat-Sen University
oairecerif.author.affiliationUniversity of Science and Technology of China
oairecerif.author.affiliationZhengzhou University
oairecerif.author.affiliationInstitiúid Ard-Lénn Bhaile Átha Cliath
oairecerif.author.affiliationUniversità degli Studi di Napoli Federico II
oairecerif.author.affiliationSichuan University
oairecerif.author.affiliationNational Astronomical Observatories Chinese Academy of Sciences
oairecerif.author.affiliationMax-Planck-Institut für Kernphysik
oairecerif.author.affiliationSouthwest Jiaotong University
oairecerif.author.affiliationPurple Mountain Observatory Chinese Academy of Sciences
oairecerif.author.affiliationUniversité de Genève
oairecerif.author.affiliationHebei Normal University
oairecerif.author.affiliationTibet University
oairecerif.author.affiliationTIANFU Cosmic Ray Research Center

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