activity
20172022
most citedInterpretations of the DAMPE electron data

44 citations · 48 across the 3 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2022

Prospective Study on Observations of γ-Ray Sources in the Galaxy Using the HADAR Experiment

Xiangli Qian, Huiying Sun, Tianlu Chen +18

The High Altitude Detection of Astronomical Radiation (HADAR) experiment is a refracting terrestrial telescope array based on the atmospheric Cherenkov imaging technique. It focuse…

astro-ph.HE20214 cited

Galactic cosmic ray propagation: sub-PeV diffuse gamma-ray and neutrino emission

Bing-Qiang Qiao, Wei Liu, Meng-Jie Zhao +2

The Tibet ASgamma experiment just reported their measurement of sub-PeV diffuse gamma ray emission from the Galactic disk, with the highest energy up to 957 TeV. These gamma-rays a…

astro-ph.HE2021

Constraining the cosmic ray propagation halo thickness using Fermi-LAT observations of high-latitude clouds

Yu-Hua Yao, Bing-Qiang Qiao, Wei Liu +5

As a basic characteristic of cosmic ray (CR) propagation, the diffusive halo can advance our understanding of many CR-related studies and indirect dark matter. The method to derive…

astro-ph.CO2021

A preliminary study about gravitational wave radiation and cosmic heat death

Jianming Zhang, Qiyue Qian, Yiqing Guo +2

We study the role of gravitational waves (GW) in the heat death of the universe. Due to the GW emission, in a very long period, dynamical systems in the universe suffer from persis…

astro-ph.HE2021

Possible bump structure of cosmic ray electrons unveiled by AMS-02 data and its common origin along with the nuclei and positron

Pei-pei Zhang, Bing-qiang Qiao, Wei Liu +3

The local pulsar and its progenitor, SNR, can together accelerate the positron, electron and nuclei to very high energy. The famous excesses of positron(nuclei) above () G…

astro-ph.HE2019

Two Numerical Methods for the 3D Anisotropic Propagation of Galactic Cosmic Rays

Wei Liu, Su-jie Lin, Hong-bo Hu +2

Conventional cosmic-ray propagation models usually assume an isotropic diffusion coefficient to account for the random deflection of cosmic rays by the turbulent interstellar magne…