Abstract: There are strong motivations for a flux of ultra-high energy (UHE) neutrinos that is observable on earth. Although they remain undetected, UHE neutrinos are expected to be produced when cosmic rays above 1019.5 eV interact with cosmic microwave background photons through the GZK process, and they would also be produced through photohadronic interactions in the same sources that accelerate UHE cosmic rays. The radio Cerenkov technique is the most promising technique for a sustained program measuring the UHE neutrino flux and extracting its rich physics and astrophysics potential. ANITA is an antenna array that searches for neutrino interactions in the Antarctic Ice from 37 km altitude, launched under NASA’s long-duration balloon pr...
Abstract: OWL [1] uses the Earth’s atmosphere as a vast calorimeter to fully enable the emerging fie...
Journal ArticleThe ANITA project is designed to investigate ultra-high energy (>1017 eV) cosmic ray ...
The Payload for Ultrahigh Energy Observations (PUEO) long-duration balloon experiment is designed to...
Ultra-high energy (UHE) neutrinos are a promising messenger particle, and their discovery would be a...
A flux of ultrahigh energy neutrinos is expected both directly from sources and from interactions be...
Abstract: The Askaryan Radio Array (ARA) is an ultra-high energy (UHE) cosmic neutrino detector loca...
The field of experimental ultra-high-energy (UHE) neutrino physics has seen significant expansion in...
We report initial results of the first flight of the Antarctic Impulsive Transient Antenna (ANITA-1)...
We report new limits on cosmic neutrino fluxes from the test flight of the Antarctic Impulsive Trans...
The Antarctic Impulsive Transient Antenna (ANITA) completed its second Long Duration Balloon flight ...
Abstract: We describe the physics goals and detector capabilities of the the ARIANNA High Energy Neu...
We summarize results from the third flight of the Antarctic Impulsive Transient Antenna (ANITA), a N...
Ph.D. University of Hawaii at Manoa 2010.Includes bibliographical references.This work describes a s...
Abstract: The ANtarctic Impulsive Transient Antenna (ANITA) searches for ultra high energy neutrinos...
The chargeless, light elementary particles known as neutrinos can be used as probes of extremely ene...
Abstract: OWL [1] uses the Earth’s atmosphere as a vast calorimeter to fully enable the emerging fie...
Journal ArticleThe ANITA project is designed to investigate ultra-high energy (>1017 eV) cosmic ray ...
The Payload for Ultrahigh Energy Observations (PUEO) long-duration balloon experiment is designed to...
Ultra-high energy (UHE) neutrinos are a promising messenger particle, and their discovery would be a...
A flux of ultrahigh energy neutrinos is expected both directly from sources and from interactions be...
Abstract: The Askaryan Radio Array (ARA) is an ultra-high energy (UHE) cosmic neutrino detector loca...
The field of experimental ultra-high-energy (UHE) neutrino physics has seen significant expansion in...
We report initial results of the first flight of the Antarctic Impulsive Transient Antenna (ANITA-1)...
We report new limits on cosmic neutrino fluxes from the test flight of the Antarctic Impulsive Trans...
The Antarctic Impulsive Transient Antenna (ANITA) completed its second Long Duration Balloon flight ...
Abstract: We describe the physics goals and detector capabilities of the the ARIANNA High Energy Neu...
We summarize results from the third flight of the Antarctic Impulsive Transient Antenna (ANITA), a N...
Ph.D. University of Hawaii at Manoa 2010.Includes bibliographical references.This work describes a s...
Abstract: The ANtarctic Impulsive Transient Antenna (ANITA) searches for ultra high energy neutrinos...
The chargeless, light elementary particles known as neutrinos can be used as probes of extremely ene...
Abstract: OWL [1] uses the Earth’s atmosphere as a vast calorimeter to fully enable the emerging fie...
Journal ArticleThe ANITA project is designed to investigate ultra-high energy (>1017 eV) cosmic ray ...
The Payload for Ultrahigh Energy Observations (PUEO) long-duration balloon experiment is designed to...