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X-ORIGINAL-URL:https://ecap.nat.fau.de
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DTSTART:20190331T010000
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DTSTART:20191027T010000
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DTSTART;TZID=Europe/Berlin:20190613T120000
DTEND;TZID=Europe/Berlin:20190613T130000
DTSTAMP:20260418T144025
CREATED:20190314T164550Z
LAST-MODIFIED:20190314T164550Z
UID:2655-1560427200-1560430800@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Christian Glaser
DESCRIPTION:Radio detection of ultra-high energy neutrinos\nHigh energy neutrino astronomy is a powerful tool to study the high-energy universe. Neutrinos can escape dense source environments and point back to their sources with sub-degree accuracy. In particular\, multi-messenger analyses that combine neutrino detection with electromagnetic (e.g. gamma ray) and gravitational-wave observations bear huge potential to probe the sources of neutrinos and cosmic rays. The detection of neutrinos is challenging because of their small flux and cross-section\, and requires the instrumentation of huge volumes. Ultra-high energy neutrinos (E > 1e16 eV) can be efficiently measured using the radio technique\, and the cold Antarctic ice is an optimal target material. \nBefore discussing the radio detection of neutrinos\, I will briefly present the radio detection of cosmic rays\, highlighting what we can learn from this mature field for neutrino detection. Then\, I will report on the pilot neutrino detectors installed on the Ross ice shelf and at the South Pole\, discuss how neutrinos can be measured with a radio detector and how their properties can be reconstructed from the short radio flash. At the end\, I will present plans for a large-scale radio neutrino detector and discuss its prospects.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-christian-glaser/
LOCATION:ECAP\, room 307\, Erwin-Rommel-Str 1\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
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