Chapter 5 Dark Matter and New Physics Beyond the Standard Model with LHAASO  

作　　者：Xiao-Jun Bi Andrea Addazi Konstantin Belotsky Vitaly Beylin Marco Cirelli Arman Esmaili Nicolao Fornengo Qing-Yu Gan Michael Kachekriess Maxim Khlopov Vladimir Korchagin Alexander Korochkin Vladimir Kuksa Antonino Marciano Andrei Neronov Paolo Panci Roman Pasechnick Alexander Sakharov Filippo Sala Giuseppe Di Sciascio Dimiri Semikoz Pasquale Dario Serpico Nikolay Volchanskiy Peng-Fei Yin 毕效军;Andrea Addazi;Konstantin Belotsky;Vitaly Beylin;Marco Cirelli;Arman Esmaili;Nicolao Fornengo;甘庆余;Michael Kachekriess;Maxim Khlopov;Vladimir Korchagin;Alexander Korochkin;Vladimir Kuksa;Antonino Marciano;Andrei Neronov;Paolo Panci;Roman Pasechnick;Alexander Sakharov;Filippo Sala;Giuseppe Di Sciascio;Dimiri Semikoz;Pasquale Dario Serpico;Nikolay Volchanskiy;殷鹏飞(Key Laboratory of Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences,Beijing 100049,China;Center for Theoretical Physics,College of Physics Science and Technology,Sichuan University,Chengdu 610065,China;Laboratori Nazionali di Frascati INFN,Frasacati(Rome),Italy,EU;National Research Nuclear University MEPHI(Moscow State Engineering Physics Institute),31 Kashirskoe chaussee,Moscow 115409,Russia;Institute of Physics,Southern Federal University Stachki 194,Rostov on Don 344090,Russia;LPTHE,CNRS and Sorbonne Universit′e,4 Place Jussieu,F-75252,Paris,France;Departamento de Fisica,Pontificia Universidade Catolica do Rio de Janeiro,Rio de Janeiro 22452-970,Brazil;Dipartimento di Fisica,Universita di Torino,Via P.Giuria 1,10125 Torino,Italy;Istituto Nazionale di Fisica Nucleare,Sezione di Torino,Via P.Giuria 1,10125,Torino,Italy;Institutt for fysikk,NTNU,7491 Trondheim,Norway;Universite de Paris,CNRS,Astroparticule et Cosmologie,F-75013 Paris,France;Department of Physics and Center for Field Theory and Particle Physics,Fudan University,Shanghai 200433,China;Astronomy Department,University of Geneve,Ch.d’Ecogia 16,1290,Versolx,Switzerland;Dipartimento di Fisica,Universita di Pisa and INFN,Sezione di Pisa Largo Pontecorvo 3,56127 Pisa,Italy;Department of Astronomy and Theoretical Physics,Lund University,22100 Lund,Sweden,EU;Experimental Physics Department,CERN,Geneva 23 CH 1211,Switzerland;Department of Physics,New York University,New York NY;United States of America;INFN sezione Roma Tor Vergata,I-00133 Rome,Italy;LAPTh,Univ.Grenoble Alpes,USMB,CNRS,F-74000 Annecy,France;Bogoliubov Laboratory of Theoretical Pj

机构地区：[1]Key Laboratory of Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences,Beijing 100049,China [2]Center for Theoretical Physics,College of Physics Science and Technology,Sichuan University,Chengdu 610065,China [3]Laboratori Nazionali di Frascati INFN,Frasacati(Rome),Italy,EU [4]National Research Nuclear University MEPHI(Moscow State Engineering Physics Institute),31 Kashirskoe chaussee,Moscow 115409,Russia [5]Institute of Physics,Southern Federal University Stachki 194,Rostov on Don 344090,Russia [6]LPTHE,CNRS and Sorbonne Universit′e,4 Place Jussieu,F-75252,Paris,France [7]Departamento de Fisica,Pontificia Universidade Catolica do Rio de Janeiro,Rio de Janeiro 22452-970,Brazil [8]Dipartimento di Fisica,Universita di Torino,Via P.Giuria 1,10125 Torino,Italy [9]Istituto Nazionale di Fisica Nucleare,Sezione di Torino,Via P.Giuria 1,10125,Torino,Italy [10]Institutt for fysikk,NTNU,7491 Trondheim,Norway [11]Universite de Paris,CNRS,Astroparticule et Cosmologie,F-75013 Paris,France [12]Department of Physics and Center for Field Theory and Particle Physics,Fudan University,Shanghai 200433,China [13]Astronomy Department,University of Geneve,Ch.d’Ecogia 16,1290,Versolx,Switzerland [14]Dipartimento di Fisica,Universita di Pisa and INFN,Sezione di Pisa Largo Pontecorvo 3,56127 Pisa,Italy [15]Department of Astronomy and Theoretical Physics,Lund University,22100 Lund,Sweden,EU [16]Experimental Physics Department,CERN,Geneva 23 CH 1211,Switzerland [17]Department of Physics,New York University,New York NY [18]United States of America [19]INFN sezione Roma Tor Vergata,I-00133 Rome,Italy [20]LAPTh,Univ.Grenoble Alpes,USMB,CNRS,F-74000 Annecy,France [21]Bogoliubov Laboratory of Theoretical Pjysics,JINR,Dubna,Russia

出　　处：《Chinese Physics C》2022年第3期126-138,共13页中国物理C（英文版）

摘　　要：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 interacting massive particles.However,this paradigm is strongly constrained by the null results of current experiments with high precision.Therefore there is a renewed interest of searches for heavy dark matter particles above TeV scale.The Large High Altitude Air Shower Observatory(LHAASO)with large effective area and strong background rejection power is very suitable to investigate the gamma-ray signals induced by dark matter annihilation or decay above TeV scale.In this document,we review the theoretical motivations and background of heavy dark matter.We review the prospects of searching for the gamma-ray signals resulted from dark matter in the dwarf spheroidal satellites and Galactic halo for LHAASO,and present the projected sensitivities.We also review the prospects of searching for the axion-like particles,which are a kind of well motivated light pseudo-scalars,through the LHAASO measurement of the very high energy gamma-ray spectra of astrophysical sources.

关 键 词：dark matter GAMMA-RAY axion-like particle 

分 类 号：P145.9[天文地球—天体物理]