Corpus ID: 117264169

Simulation of the Event Reconstruction of Ultra High Energy Cosmic Neutrinos with Askaryan Radio Array

@article{Sun2010SimulationOT,
  title={Simulation of the Event Reconstruction of Ultra High Energy Cosmic Neutrinos with Askaryan Radio Array},
  author={Shangyu Sun and Pisin. Chen and Melin Huang},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2010}
}
Askaryan Radio Array (ARA), a large-scale radio Cherenkov observatory which scientists propose to develop in Antarctica, aims at discovering the origin and evolution of the cosmic accelerators that produce the highest energy cosmic rays by means of observing the ultra high energy (UHE) cosmogenic neutrinos. To optimize ARA's angular resolution of the incoming UHE neutrinos, which is essential for pointing pack to its source, the relation between the reconstruction capabilities of ARA and its… Expand
Optimization of an ARA like Radio Neutrino Detector in Ice
Radio ice detectors for Ultra High Energy neutrinos take advantage of large natural ice sheets to detect the impulsive emission of radio signals from Askaryan emission. The Askaryan Radio Array (ARA)Expand
Signal Stability Studies with the Askaryan Under-Ice Radio Array
High energy astrophysical neutrinos are useful for understanding the origins of high energy cosmic rays, which have been a mystery for almost a century. Such neutrinos can be detected via coherentExpand
Observational limits of a large scale neutrino detector in a salt dome
Abstract We are investigating the possibility to construct a radio Askaryan neutrino observatory in a salt mine. The first step is to determine the optimal geometry such that the cost of experimentExpand
Instruments and Methods for the Radio Detection of High Energy Cosmic Rays - ReadingSample
Instruments and Methods for the Radio Detection of High Energy Cosmic Rays Cosmic rays at energies above & 10 eV cannot be measured directly due to the low flux. Instead, the properties of theExpand
Realization of a Self-Triggered Detector for the Radio Emission of Cosmic Rays
Realization of a self-triggered detector for the radio emission of cosmic rays When a high-energetic primary cosmic ray particle penetrates the Earth’s atmosphere, a cascade of secondary particles isExpand
Considerations on an underground neutrino radio detector in salt
This article presents the possibility of in-salt radio detection of high energy neutrinos, and shows the implications that a heterogeneous propagating medium has on both antenna behaviour, and onExpand
Radio Experiments for Air Shower Detection
Already in the 1950s and 1960s, several experiments discovered that cosmic ray air showers emit radio pulses in the MHz regime [39], that the emission is linked to the Earth’s magnetic field, andExpand
ON A LARGE SCALE NEUTRINO DETECTOR IN A SALT DOME
We consider a neutrino large-scale radio Cherenkov observatory in a Romanian salt mine. We include propagation effects on the radio signal generated and make a threshold analysis, taking into accountExpand
Radio Propagation Environment Analysis for Neutrino Radio Detection in Salt Mines
Abstract a We consider a neutrino large-scale radio Cherenkov observatory in a Romanian salt mine. We include propagation effects on the radio signal generated and make a threshold analysis, takingExpand

References

SHOWING 1-9 OF 9 REFERENCES
Ultrahigh-energy neutrino fluxes and their constraints
Applying our recently developed propagation code we review extragalactic neutrino fluxes above 10^{14} eV in various scenarios and how they are constrained by current data. We specifically identifyExpand
Measurement of the UHECR energy spectrum using data from the surface detector of the Pierre Auger Observatory
At the southern site of the Pierre Auger Observatory, which is close to completion, an exposure that significantly exceeds the largest forerunner experiments has already been accumulated. We report aExpand
Upper limit of the spectrum of cosmic rays
"J."
however (for it was the literal soul of the life of the Redeemer, John xv. io), is the peculiar token of fellowship with the Redeemer. That love to God (what is meant here is not God’s love to men)Expand
for the Auger Collaboration
  • ”Measurement of the UHECR energy spectrum using data from the Surface Detector of the Pierre Auger Observatory,” Contribution to the 30th International Cosmic Ray Conference, Merida, Mexico, http : //arxiv.org/abs/0706.2096
  • 2007
Astropart
  • Phys. 4, 253
  • 1996
Astropart . Phys . 3 ( 1995 ) 105 ; also Shigeru Yoshida , Hongyue Dai , ( astro − ph / 9802294 )
  • Journal of Physics G
  • 1985
End to the cosmic ray spectrum
JETP 14
  • 441
  • 1962