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19992026
most citedBlack hole shadows in fourth-order conformal Weyl gravity

43 citations · 447 across the 30 of their papers we have counts for

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hep-ph2004★ 18 cited

Bounds on Relic Neutrino Masses in the Z-burst Model

Graciela Gelmini, Gabriele Varieschi, Thomas Weiler

Neutrinos from far-away sources annihilating at the Z resonance on relic neutrinos may give origin to the extreme-energy cosmic rays (EECR). If ``Z-bursts'' are responsible for the…

hep-ph2002★ 23 cited

Measuring the prompt atmospheric neutrino flux with down-going muons in neutrino telescopes

Graciela Gelmini, Paolo Gondolo, Gabriele Varieschi

In the TeV energy region and above, the uncertainty in the level of prompt atmospheric neutrinos would limit the search for diffuse astrophysical neutrinos. We suggest that neutrin…

hep-ph2002★ 7 cited

Cosmic rays above the ankle from Z-bursts

Graciela Gelmini, Gabriele Varieschi

Neutrinos from far away sources annihilating at the Z resonance on relic neutrinos may give origin to the ultrahigh-energy cosmic rays. Here we present predictions of this mechanis…

hep-ph2000★ 9 cited

Measurement of the gluon PDF at small x with neutrino telescopes

Graciela Gelmini, Paolo Gondolo, Gabriele Varieschi

We analyze the possibility that neutrino telescopes may provide an experimental determination of the slope lambda of the gluon distribution in the proton at momentum fractions x sm…

hep-ph1999★ 39 cited

Prompt atmospheric neutrinos and muons: dependence on the gluon distribution function

Graciela Gelmini, Paolo Gondolo, Gabriele Varieschi

We compute the next-to-leading order QCD predictions for the vertical flux of atmospheric muons and neutrinos from decays of charmed particles, for different PDF's (MRS-R1, MRS-R2,…

hep-ph1999★ 29 cited

Prompt atmospheric neutrinos and muons: NLO vs LO QCD predictions

Graciela Gelmini, Paolo Gondolo, Gabriele Varieschi

We compare the leading and next-to-leading order QCD predictions for the flux of atmospheric muons and neutrinos from decays of charmed particles. We find that the full NLO lepton…