The detection of extraterrestrial EHE neutrinos requires detection volumes at least one order of magnitude larger than currently constructed km(3) optical neutrino detectors. In ice, it is anticipated that the absorption length for acoustic waves reaches up to to several kilometers. This makes ice an attractive host environment for a next generation acoustic neutrino detector. To measure the acoustic properties of ice at South Pole, a test setup has been developed, ready to be deployed in the 2006/07 summer season
We have measured the speed of both pressure waves and shear waves as a function of depth between 80 ...
Neutrino astronomy is a new field of astroparticle physics that uses neutrino detectors to observe a...
We have measured the speed of both pressure waves and shear waves as a function of depth between 80 ...
The detection of extraterrestrial EHE neutrinos requires detection volumes at least one order of mag...
The feasibility and design of an acoustic neutrino detection array in the South Pole ice depend on t...
Abstract: Astrophysical neutrinos in the EeV range (particularly those generated by the interaction ...
Due to the low flux of ultrahigh energetic neutrinos induced in interactions of cosmic rays with the...
The South Pole Acoustic Test Setup (SPATS) was built to evaluate the acoustic characteristics of the...
When high-energy particles interact in dense media to produce a particle shower, most of the shower ...
We present development work aiming towards a large scale ice-based hybrid detector including acousti...
The detection of acoustic signals from ultra-high energy neutrino interactions is a promising method...
The detection of acoustic signals from ultra-high energy neutrino interactions is a promising method...
The South Pole Acoustic Test Setup consists of four strings, each instrumented with seven acoustic s...
In order to detect the small neutrino fluxes expected at ultra-high energies, large volumes of ma...
Over the last few decades, several dedicated neutrino telescopes have been built to detect high ener...
We have measured the speed of both pressure waves and shear waves as a function of depth between 80 ...
Neutrino astronomy is a new field of astroparticle physics that uses neutrino detectors to observe a...
We have measured the speed of both pressure waves and shear waves as a function of depth between 80 ...
The detection of extraterrestrial EHE neutrinos requires detection volumes at least one order of mag...
The feasibility and design of an acoustic neutrino detection array in the South Pole ice depend on t...
Abstract: Astrophysical neutrinos in the EeV range (particularly those generated by the interaction ...
Due to the low flux of ultrahigh energetic neutrinos induced in interactions of cosmic rays with the...
The South Pole Acoustic Test Setup (SPATS) was built to evaluate the acoustic characteristics of the...
When high-energy particles interact in dense media to produce a particle shower, most of the shower ...
We present development work aiming towards a large scale ice-based hybrid detector including acousti...
The detection of acoustic signals from ultra-high energy neutrino interactions is a promising method...
The detection of acoustic signals from ultra-high energy neutrino interactions is a promising method...
The South Pole Acoustic Test Setup consists of four strings, each instrumented with seven acoustic s...
In order to detect the small neutrino fluxes expected at ultra-high energies, large volumes of ma...
Over the last few decades, several dedicated neutrino telescopes have been built to detect high ener...
We have measured the speed of both pressure waves and shear waves as a function of depth between 80 ...
Neutrino astronomy is a new field of astroparticle physics that uses neutrino detectors to observe a...
We have measured the speed of both pressure waves and shear waves as a function of depth between 80 ...