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20162021
most citedConsistent explanation for the cosmic-ray positron excess in -wave Breit-Wigner enhanced dark matter annihilation

6 citations · 8 across the 2 of their papers we have counts for

collaborators

5 papers

hep-ph2021★ 6 cited

Consistent explanation for the cosmic-ray positron excess in -wave Breit-Wigner enhanced dark matter annihilation

Yu-Chen Ding, Yu-Lin Ku, Chun-Cheng Wei +1

Dark matter (DM) annihilation in the galactic halo can be enhanced relative to that in the early Universe due to the Breit-Wigner enhancement, if the DM particles annihilate throug…

hep-ph2021★ 2 cited

Consistent explanation for the cosmic-ray positron excess in p-wave Sommerfeld-enhanced dark matter annihilation

Yu-Chen Ding, Yu-Lin Ku, Chun-Cheng Wei +1

Sommerfeld-enhanced dark matter (DM) annihilation through -wave has been widely considered as a consistent explanation for both the observed cosmic-ray (CR) positron excess and…

astro-ph.HE2020

Implications of a possible TeV break in the cosmic-ray electron and positron flux

Yu-Chen Ding, Nan Li, Chun-Cheng Wei +2

A TeV spectral break in the total flux of cosmic-ray electrons and positrons (CREs) at which the spectral power index softens from to has been observed by H.E.S.S…

hep-ph2020

The high energy window of probing dark matter with cosmic-ray antideuterium and antihelium

Yu-Chen Ding, Nan Li, Chun-Cheng Wei +1

Cosmic-ray (CR) anti-nuclei are often considered as important observables for dark matter (DM) indirect detections at low kinetic energies below GeV per nucleon. Since the primary…

hep-ph2016

Antiprotons from dark matter annihilation through light mediators and a possible excess in AMS-02 data

Xian-Jun Huang, Chun-Cheng Wei, Yue-Liang Wu +2

We show that in the scenario where dark matter (DM) particles annihilate through light mediators, the energy spectra of the final state cosmic-ray particles depend strongly on the…