Seminars & Lectures
| * TITLE | Searching cosmic ultra high energy neutrinos with radio-frequency detectors | ||||||
|---|---|---|---|---|---|---|---|
| * SPEAKERS | |||||||
|
|||||||
| * HOST(Applicant) | |||||||
|
|||||||
| * DATE / TIME | 2012-12-24, 11:00 am, 503 conference room | ||||||
| * ABSTRACT | |||||||
| In the ultra high energy (UHE) region (above 10^18eV), there is an expected neutrino flux due to pion photo production followed by pion decay. This process was predicted by Greisen, Zatsepin, and Kuzmin (GZK process) in the 1960\\\'s, and motivated us to search this UHE neutrinos. Radio-frequency (RF) detection method is a promising technology for detecting UHE neutrinos. I will talk about some past, present and new RF experiments. I will also talk about some simulation results and test station data analysis results from Askaryan Radio Array (ARA) experiment. | |||||||
