Supported by National Natural Science Foundation in China(NSFC)(U2031103,U1831208,11805209,11775233);NSFC for Distinguished Young Scholars(12025502);the Science and Technology Department of Sichuan Province(2021YFSY0031);the International Partnership Program of Chinese Academy of Sciences(113111KYSB20170055)。
The Large High Altitude Air Shower Observatory(LHAASO)(Fig.1)is located at Mt.Haizi(4410 m a.s.l.,600 g/cm^(2),29°21'27.56"N,100°08'19.66"E)in Daocheng,Sichuan province,P.R.China.LHAASO consists of 1.3 km^(2) array(...
Supported by Key Research and Development Project(2018YFA0404204,2016YFA0400804);the National Natural Science Foundation of China(11905043,11803011,12173018,12121003,11773014,11633007,U1931204,U1731136);the Original Innovation Program of the Chinese Academy of Sciences(E085021002);Guangdong Major Project of Basic and Applied Basic Research(2019B030302001);science research grant from the China Manned Space Project(CMS-CSST-2021-B09)。
In theγ-ray sky,the highest fluxes come from Galactic sources:supernova remnants(SNRs),pulsars and pulsar wind nebulae,star forming regions,binaries and micro-quasars,giant molecular clouds,Galactic center,and the la...
Supported by the National Key R&D program of China(2018YFA0404203);National Natural Science Foundation Of China(12121003,11625312);China Manned Space Project(CMS-CSST-2021-B11)。
Extra-galactic gammaray sources,such as gamma-ray bursts,active galactic nuclei,starburst galaxies,are interesting and important targets for LHAASO observations.In this chapter,the prospects of detecting these sources...
Supported by the National Key R&D Program of China(2018YFA0404203);the International Scholarship Program of the MOST of China(G2021166002L);National Natural Science Foundation of China(NSFC)(12147208,U2031103,U1931204);the Science and Technology Department of Sichuan Province(2021YFSY0031)。
In the first part of this Chapter the present state of knowledge from the observations of cosmic rays between 10^(13) and 10^(20) eV is summarized.This is not intended to be a complete review,but rather a broad overvi...
In order to reveal the nature of dark matter,it is crucial to detect its non-gravitational interactions with the standard model particles.The traditional dark matter searches focused on the so-called weakly interactin...
Supported by the Natural Science Foundation of China(11773003,11875264,12003007,12173091,U1931201,U2031105);the Fundamental Research Funds for the Central Universities(2020kfyXJJS039)。
Combining observations of multi-messengers help in boosting the sensitivity of astrophysical source searches,and probe various aspects of the source physics.In this chapter we discuss how LHAASO observations of very h...
Supported in China by National Natural Science Foundation(NSFC)(12047576,U2031101,11475141);the National Key R&D Program of China(2018YFA0404201,2018YFA0404202);in Thailand by the Thailand Science Research and Innovation(RTA6280002)。
In the following sub-sections,studies of solar-heliospheric effects on cosmic rays,investigating a possible link between cosmic ray flux and Earth’s climate,and detection of MeV-rangeγ-rays from thunderstorms with t...