The sensitivity of an ice radiowave detector to the anticipated high energy neutrino fluxes is calculated on the basis of a detailed threshold analysis and computation of the shower production rate. We show that diffuse neutrinos from Active Galactic Nuclei could be detectable in a radio detector of 1 sq.km area established in Central Antarctica
Neutrinos of astrophysical origin could be detected through the electromagnetic radiation of the par...
Since summer 2021, the Radio Neutrino Observatory in Greenland (RNO-G) is searching for astrophysica...
Ph.D. University of Hawaii at Manoa 2010.Includes bibliographical references.This work describes a s...
Radio Cherenkov radiation is arguably the most efficient mechanism for detecting showers from ultra-...
High energy astrophysical neutrinos are useful for understanding the origins of high energy cosmic r...
We study the Cherenkov radiopulses emitted in PeV and EeV neutrino interactions in ice. We discuss h...
Radio waves, perhaps because our terrestrial atmosphere and the cosmos beyond are uniquely transpare...
We discuss the radar detection technique as a probe for high-energy cosmic neutrino induced particle...
We study the longitudinal development of hadronic showers in ice for energies up to 100 EeV and its ...
In this article we try to answer the question whether the radar detection technique can be used for ...
Current experiments aimed at measuring the UHE (E>100 PeV) neutrino flux via detection of coherent C...
The emerging field of radio based neutrino astronomy holds promise in answering long lasting questio...
Since summer 2021, the Radio Neutrino Observatory in Greenland (RNO-G) is searching for astrophysica...
Since summer 2021, the Radio Neutrino Observatory in Greenland (RNO-G) is searching for astrophysica...
Since summer 2021, the Radio Neutrino Observatory in Greenland (RNO-G) is searching for astrophysica...
Neutrinos of astrophysical origin could be detected through the electromagnetic radiation of the par...
Since summer 2021, the Radio Neutrino Observatory in Greenland (RNO-G) is searching for astrophysica...
Ph.D. University of Hawaii at Manoa 2010.Includes bibliographical references.This work describes a s...
Radio Cherenkov radiation is arguably the most efficient mechanism for detecting showers from ultra-...
High energy astrophysical neutrinos are useful for understanding the origins of high energy cosmic r...
We study the Cherenkov radiopulses emitted in PeV and EeV neutrino interactions in ice. We discuss h...
Radio waves, perhaps because our terrestrial atmosphere and the cosmos beyond are uniquely transpare...
We discuss the radar detection technique as a probe for high-energy cosmic neutrino induced particle...
We study the longitudinal development of hadronic showers in ice for energies up to 100 EeV and its ...
In this article we try to answer the question whether the radar detection technique can be used for ...
Current experiments aimed at measuring the UHE (E>100 PeV) neutrino flux via detection of coherent C...
The emerging field of radio based neutrino astronomy holds promise in answering long lasting questio...
Since summer 2021, the Radio Neutrino Observatory in Greenland (RNO-G) is searching for astrophysica...
Since summer 2021, the Radio Neutrino Observatory in Greenland (RNO-G) is searching for astrophysica...
Since summer 2021, the Radio Neutrino Observatory in Greenland (RNO-G) is searching for astrophysica...
Neutrinos of astrophysical origin could be detected through the electromagnetic radiation of the par...
Since summer 2021, the Radio Neutrino Observatory in Greenland (RNO-G) is searching for astrophysica...
Ph.D. University of Hawaii at Manoa 2010.Includes bibliographical references.This work describes a s...