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J. Ellis

4 papers hereh-index 5202 citations27 works total

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

author position
  • first author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO2
  • hep-ph2
same name
  • J. Ellis — 497 papers, h 123
  • J. Ellis — 44 papers, h 33
  • J. Ellis — 28 papers, h 15
  • J. Ellis — 18 papers, h 11
  • J. Ellis — 18 papers, h 18
  • J. Ellis — 13 papers, h 26

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

most citedProspects for Future Binary Black Hole GW Studies in Light of PTA Measurements

43 citations · 71 across the 4 of their papers we have counts for

collaborators

4 papers

hep-ph2023★ 19 cited

Probing Neutral Triple Gauge Couplings with Z∗γ(ννˉγ) Production at Hadron Colliders

John Ellis, Hong-Jian He, Rui-Qing Xiao

We study probes of neutral triple gauge couplings (nTGCs) via Z∗γ production followed by off-shell decays Z∗→ννˉ at the LHC and future pp colliders, including both CP-…

astro-ph.CO2023★ 8 cited

Cosmic Superstrings Revisited in Light of NANOGrav 15-Year Data

John Ellis, Marek Lewicki, Chunshan Lin +1

We analyze cosmic superstring models in light of NANOGrav 15-year pulsar timing data. A good fit is found for a string tension Gμ∼10−12−10−11 and a string intercommu…

hep-ph2023★ 1 cited

Electroweak Loop Contributions to the Direct Detection of Wino Dark Matter

John Ellis, Natsumi Nagata, Keith A. Olive +1

Electroweak loop corrections to the matrix elements for the spin-independent scattering of cold dark matter particles on nuclei are generally small, typically below the uncertainty…

astro-ph.CO2023★ 43 cited

Prospects for Future Binary Black Hole GW Studies in Light of PTA Measurements

John Ellis, Malcolm Fairbairn, Gert Hütsi +4

NANOGrav and other Pulsar Timing Arrays (PTAs) have discovered a common-spectrum process in the nHz range that may be due to gravitational waves (GWs): if so, they are likely to ha…

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