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researcher

R. Keeley

42 papers hereh-index 212.4k citations52 works total

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

author position
  • first author12
  • middle author27
  • last author1

Across the 40 of 42 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO36
  • hep-ph3
  • astro-ph.HE2
  • astro-ph.IM1
same name
  • R. Keeley — 4 papers, h 3
  • R. Keeley — 1 paper, h 1
  • R. Keeley — 1 paper, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20132026
most citedTying Dark Matter to Baryons with Self-interactions

163 citations · 1.2k across the 42 of their papers we have counts for

collaborators
Showing hep-phShow all

3 papers · 1 filter

hep-ph2022★ 10 cited

Report of the Topical Group on Cosmic Probes of Fundamental Physics for for Snowmass 2021

Rana X. Adhikari, Luis A. Anchordoqui, Ke Fang +118

Cosmic Probes of Fundamental Physics take two primary forms: Very high energy particles (cosmic rays, neutrinos, and gamma rays) and gravitational waves. Already today, these probe…

hep-ph2020★ 79 cited

Strong constraints on thermal relic dark matter from Fermi-LAT observations of the Galactic Center

Kevork N. Abazajian, Shunsaku Horiuchi, Manoj Kaplinghat +2

The extended excess toward the Galactic Center (GC) in gamma rays inferred from Fermi-LAT observations has been interpreted as being due to dark matter (DM) annihilation. Here, we…

hep-ph2015★ 58 cited

Bright gamma-ray Galactic Center excess and dark dwarfs: Strong tension for dark matter annihilation despite Milky Way halo profile

Kevork N. Abazajian, Ryan E. Keeley

We incorporate Milky Way dark matter halo profile uncertainties, as well as an accounting of diffuse gamma-ray emission uncertainties in dark matter annihilation models for the Gal…

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