activity
20132025
most citedCharge Measurement of Cosmic Ray Nuclei with the Plastic Scintillator Detector of DAMPE

45 citations · 198 across the 13 of their papers we have counts for

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Showing astro-ph.HEShow all

7 papers · 1 filter

astro-ph.HE2025★ 6 cited

Charge-dependent spectral softenings of primary cosmic-rays below the knee

DAMPE Collaboration, Francesca Alemanno, Qi An +146

In most particle acceleration or propagation theories, the characteristic features of the cosmic ray spectra due to acceleration limits or propagation phase changes are charge depe…

astro-ph.HE2021★ 22 cited

Observations of Forbush Decreases of cosmic ray electrons and positrons with the Dark Matter Particle Explorer

Francesca Alemanno, Qi An, Philipp Azzarello +146

The Forbush Decrease (FD) represents the rapid decrease of the intensities of charged particles accompanied with the coronal mass ejections (CMEs) or high-speed streams from corona…

astro-ph.HE2021★ 6 cited

Explanation of nearby SNRs for primary electron excess and proton spectral bump

Tian-Peng Tang, Zi-Qing Xia, Zhao-Qiang Shen +5

Several groups have reported a possible excess of primary electrons at high energies with the joint fit of the positron fraction and total electron/positron spectra. With the lates…

astro-ph.HE2019★ 26 cited

Searching for the possible signal of the photon-axionlike particle oscillation in the combined GeV and TeV spectra of supernova remnants

Zi-Qing Xia, Yun-Feng Liang, Lei Feng +3

The conversion between photons and axionlike particles (ALPs) in the Milky Way magnetic field could result in the detectable oscillation phenomena in -ray spectra of Galactic so…

astro-ph.HE2018★ 36 cited

Searching for spectral oscillations due to photon-axionlike particle conversion using the Fermi-LAT observations of bright supernova remnants

Zi-Qing Xia, Cun Zhang, Yun-Feng Liang +4

Axionlike-particles (ALPs) are one promising type of dark matter candidate particle that may generate detectable effects on -ray spectra other than the canonical weakly interact…

astro-ph.HE2016★ 14 cited

3FGL J1924.8-1034 : A Spatially-Extended Stable Unidentified GeV Source?

Zi-Qing Xia, Kai-Kai Duan, Shang Li +8

Milky Way-like galaxies are predicted to host a very large number of dark matter subhalos. Some massive and nearby subhalos could generate detectable gamma-rays, appearing as unide…

astro-ph.HE2013★ 4 cited

The spatial distribution of dark-matter-annihilation originated gamma-ray line signal

Tong-Suo Lu, Tie-Kuang Dong, Jian Wu

The GeVTeV ray line signal is the smoking gun signature of the dark matter annihilation or decay. The detection of such a signal is one of the main targets of some space-bas…