Addendum to "Coherent radio pulses from GEANT generated electromagnetic showers in ice"
arXiv:astro-ph/0306291 · doi:10.1103/PhysRevD.69.047101
Abstract
We reevaluate our published calculations of electromagnetic showers generated by GEANT 3.21 and the radio frequency pulses they produce in ice. We are prompted by a recent report showing that GEANT 3.21-modeled showers are sensitive to internal settings in the electron tracking subroutine. We report the shower and pulse characteristics obtained with different settings of GEANT 3.21 and with GEANT 4. The default setting of electron tracking in GEANT 3.21 we used in previous work speeds up the shower simulation at the cost of information near the end of the tracks. We find that settings tracking electron and positron to lower energy yield a more accurate calculation, a more intense shower, and proportionately stronger radio pulses at low frequencies. At high frequencies the relation between shower tracking algorithm and pulse spectrum is more complex. We obtain radial distributions of shower particles and phase distributions of pulses from 100 GeV showers that are consistent with our published results.
4 pages, 3 figures
References in corpus (4)
Cited by in corpus (17)
- RICE Limits on the Diffuse Ultra-High Energy Neutrino Flux
- Updated Results from the RICE Experiment and Future Prospects for Ultra-High Energy Neutrino Detection at the South Pole
- Cherenkov radio pulses from electromagnetic showers in the time-domain
- Practical and accurate calculations of Askaryan radiation
- Coherent radio pulses from showers in different media: A unified parameterization
- Radio emission from cosmic ray air showers: Monte Carlo simulations
- Coherent Cherenkov radio pulses from hadronic showers up to EeV energies
- Ross Ice Shelf in situ radio-frequency ice attenuation
- Time-Domain Measurement of Broadband Coherent Cherenkov Radiation
- Simulation of in-ice cosmic ray air shower induced particle cascades
- Calculations of electric fields for radio detection of Ultra-High Energy particles
- Comparative study of radio pulses from simulated hadron-, electron-, and neutrino-initiated showers in ice in the GeV-PeV range
- Radiowave Detection of Ultra-High Energy Neutrinos and Cosmic Rays
- Simulation of radio signals from cosmic-ray cascades in air and ice as observed by in-ice Askaryan radio detectors
- Cherenkov Radiation from Pairs and Its Effect on Induced Showers
- Evidence for Observation of Virtual Radio Cherenkov Fields
- Comparison with experimental data of different theoretical approaches to high-energy electron bremsstrahlung including quantum coherence effects