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20122025
most citedPerturbative charm production and the prompt atmospheric neutrino flux in light of RHIC and LHC

123 citations · 203 across the 9 of their papers we have counts for

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hep-ph2025

Beyond standard model particles in the atmospheric flux: a long-lived stau example

Atri Bhattacharya, Mary Hall Reno, Ina Sarcevic

We discuss fluxes of long-lived supersymmetric (SUSY) particles produced in the atmosphere from ultra-high energy cosmic-ray interactions with air nuclei. We consider long-lived pa…

hep-ph2020

Perturbative Charm Production and the Prompt Atmospheric Neutrino Flux in light of RHIC and LHC

Atri Bhattacharya, Rikard Enberg, Mary Hall Reno +2

Prompt neutrinos due to the decay of charmed mesons produced in the atmosphere from cosmic-ray and atmospheric nuclei interactions may be a significant source of background to ultr…

hep-ph20201 cited

The proton inelastic cross section at ultrahigh energies

Atri Bhattacharya, Jean-René Cudell, Rami Oueslati +1

We study the consequences of high-energy collider data on the best fits to total, elastic, and inelastic cross sections for and scattering using two very distinct u…

hep-ph201737 cited

Probing decaying heavy dark matter with the 4-year IceCube HESE data

Atri Bhattacharya, Arman Esmaili, Sergio Palomares-Ruiz +1

After the first four years of data taking, the IceCube neutrino telescope has observed 54 high-energy starting events (HESE) with deposited energies between 20 TeV and 2 PeV. The b…

hep-ph2015123 cited

Perturbative charm production and the prompt atmospheric neutrino flux in light of RHIC and LHC

Atri Bhattacharya, Rikard Enberg, Mary Hall Reno +2

We re-evaluate the prompt atmospheric neutrino flux, using the measured charm cross sections at RHIC and the Large Hadron Collider to constrain perturbative QCD parameters such as…

hep-ph201215 cited

On the interpretation of IceCube cascade events in terms of the Glashow resonance

Atri Bhattacharya, Raj Gandhi, Werner Rodejohann +1

The IceCube experiment (IC) has recently observed 2 cascade events with energies between 1 and 10 PeV. This energy combined with the fact that no muon-track events are observed may…