activity
20202024
most citedImplications of a possible TeV break in the cosmic-ray electron and positron flux

16 citations · 30 across the 6 of their papers we have counts for

collaborators

6 papers

hep-ph2024★ 1 cited

Constraints on evaporating primordial black holes from the AMS-02 positron data

Jia-Zhi Huang, Yu-Feng Zhou

Cosmic-ray (CR) positrons are relatively rare due to their secondary origin and thus sensitive to exotic contributions. Primordial black holes (PBHs) with masses above $\sim 5\time…

hep-ph2022★ 4 cited

Enhanced cosmic-ray antihelium production from dark matter annihilation through light mediators

Yu-Chen Ding, Nan Li, Yu-Feng Zhou

Cosmic-ray (CR) antihelium is an important probe for the indirect search of dark matter (DM) annihilation in the Galaxy. However, due to stringent constraints from the measurements…

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★ 16 cited

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★ 1 cited

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…