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researcher

W. Carvalho

4 papers hereh-index 314 citations7 works total

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

author position
  • middle author3

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.IM1
  • hep-ph1
same name
  • W. Carvalho — 412 papers
  • W. Carvalho — 222 papers, h 70
  • W. Carvalho — 127 papers, h 0
  • W. Carvalho — 66 papers, h 47
  • W. Carvalho — 64 papers, h 106
  • W. Carvalho — 25 papers, h 14

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
20202025
most citedProspects for High-Elevation Radio Detection of >100 PeV Tau Neutrinos

36 citations · 38 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2025★ 2 cited

Sensitivity of BEACON to Ultra-High Energy Diffuse and Transient Neutrinos

Andrew Zeolla, Jaime Alvarez-Muñiz, Sergio Cabana-Freire +16

Ultra-high energy neutrinos (E>1017 eV) can provide insight into the most powerful accelerators in the universe, however their flux is extremely low. The Beamforming Elevated…

hep-ph2023

Secondary Lepton Production, Propagation, and Interactions with NuLeptonSim

Austin Cummings, Ryan Krebs, Stephanie Wissel +5

Charged current interactions of neutrinos inside the Earth can result in secondary muons and τ-leptons which are detectable by several existing and planned neutrino experiments t…

astro-ph.HE2023

TAMBO: Searching for Tau Neutrinos in the Peruvian Andes

William G. Thompson

The detection of high-energy astrophysical neutrinos by IceCube has opened a new window on our Universe. While IceCube has measured the flux of these neutrinos at energies up to se…

astro-ph.IM2020★ 36 cited

Prospects for High-Elevation Radio Detection of >100 PeV Tau Neutrinos

Stephanie Wissel, Andrés Romero-Wolf, Harm Schoorlemmer +16

Tau neutrinos are expected to comprise roughly one third of both the astrophysical and cosmogenic neutrino flux, but currently the flavor ratio is poorly constrained and the expect…

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