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researcher

Xiao-Jun Bi

5 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author1
  • last author1

Across the 3 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph2
  • astro-ph.HE2
  • hep-ph1
ORCID 0000-0002-5334-9754

identity via Semantic Scholar / OpenAlex

activity
20072014
most citedUnified model for the gamma-ray emission of supernova remnants

56 citations · 93 across the 5 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

2 papers · 1 filter

astro-ph.HE2012★ 12 cited

Gamma-rays From Warm WIMP Dark Matter Annihilation

Qiang Yuan, Yixian Cao, Jie Liu +4

The weakly interacting massive particle (WIMP) often serves as a candidate for the cold dark matter, however when produced non-thermally it could behave like warm dark matter. In t…

astro-ph.HE2012★ 56 cited

Unified model for the gamma-ray emission of supernova remnants

Qiang Yuan, Siming Liu, Xiao-Jun Bi

Shocks of supernova remnants (SNRs) are important (and perhaps the dominant) agents for production of the Galactic cosmic rays. Recent γ-ray observations of several SNRs have mad…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.