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X-ORIGINAL-URL:https://ecap.nat.fau.de
X-WR-CALDESC:Events for Erlangen Centre for Astroparticle Physics
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DTSTART:20190331T010000
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DTSTART:20191027T010000
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BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20190606T120000
DTEND;TZID=Europe/Berlin:20190606T130000
DTSTAMP:20260418T005437
CREATED:20190213T201728Z
LAST-MODIFIED:20190213T201728Z
UID:2631-1559822400-1559826000@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Lee Thompson
DESCRIPTION:HyperKamiokande: a next generation long baseline neutrino experiment in Japan\n\nThe seminar will present the HyperKamiokande (HyperK) project which will build a large volume water Cerenkov detector for long baseline neutrino oscillation studies in Japan. A brief historical resume of the discovery of neutrino oscillations will be provided. The presentation will give an overview of the design of the HyperK detector and its main technical features. Details of the scientific programme to be undertaken will also be discussed. The prospects for the project to determine fundamental measurements such as CP violation and mass hierarchy will also be presented.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-lee-thompson/
LOCATION:ECAP\, room 307\, Erwin-Rommel-Str 1\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
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BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20190613T120000
DTEND;TZID=Europe/Berlin:20190613T130000
DTSTAMP:20260418T005437
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
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20190627T120000
DTEND;TZID=Europe/Berlin:20190627T130000
DTSTAMP:20260418T005437
CREATED:20190305T143659Z
LAST-MODIFIED:20190305T143659Z
UID:2641-1561636800-1561640400@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Andreas Haungs
DESCRIPTION:Cosmic rays between the knee and the ankle\nInvestigations of the energy spectrum as well as the mass composition of cosmic rays in the energy range of PeV to EeV are important for understanding both\, the origin of the galactic and the extragalactic cosmic rays. The multi-detector arrangement of KASCADE and its extension KASCADE-Grande was designed for observations of cosmic ray air showers in this energy range. Most important result from KASCADE is the proof that the knee feature at several PeV is due to a decrease in the flux of light atomic nuclei of primary cosmic rays. Results of KASCADE-Grande have now shown two more spectral features: a knee-like structure in the spectrum of heavy primaries at around 90 PeV and a hardening of the spectrum of light primaries at energies just above 100 PeV. These features are meanwhile confirmed by other experiments like Tunka\, IceCube/IceTop\, or TA/TALE. In this seminar the recent results on energy spectrum and composition are compared to each other and with astrophysical models for the energy range\, where the transition from galactic to extragalactic origin of cosmic rays are expected. In addition\, the effects of using different hadronic interaction models for interpreting the measured air-shower data will be discussed. Finally\, the KASCADE Cosmic Ray Data Centre (KCDC) is discussed\, which is a web-based platform to provide astroparticle physics data for the general public. The main purpose of KCDC is to archive original data to offer long-term scientific data for the high-energy astroparticle physics community as well as for students and the interested public via a sophisticated web portal. However\, KCDC can only be a first step into a global analysis and data centre for multi-messenger astroparticle physics.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-andreas-haungs/
LOCATION:ECAP\, room 307\, Erwin-Rommel-Str 1\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
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