BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//Erlangen Centre for Astroparticle Physics - ECPv6.2.3.2//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-WR-CALNAME:Erlangen Centre for Astroparticle Physics
X-ORIGINAL-URL:https://ecap.nat.fau.de
X-WR-CALDESC:Events for Erlangen Centre for Astroparticle Physics
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-Robots-Tag:noindex
X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:Europe/Berlin
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20170326T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20171029T010000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20171018T120000
DTEND;TZID=Europe/Berlin:20171018T130000
DTSTAMP:20260426T011250
CREATED:20171010T074632Z
LAST-MODIFIED:20171010T074632Z
UID:2026-1508328000-1508331600@ecap.nat.fau.de
SUMMARY:Anatoli Fedynitch - State-of-the-art atmospheric lepton flux Tools
DESCRIPTION:Atmospheric leptons receive steady interest from several scientific communities. At low and intermediate energies\, atmospheric neutrinos are the signal for studies of fundamental neutrino properties and at high energies\, they constitute the background for the characterization of the features of the astrophysical neutrino flux. We have studied in depth the relation between observable inclusive lepton fluxes/ratios and hadronic interactions by using a novel numerical transport equation solver MCEq. It enables us to characterize\, with an unprecedented precision\, relevant particle interaction energies\, important hadron species\, and the secondary particle production phase-space in terms of typical accelerator observables. Based on our findings\, we improved existing interaction models SIBYLL and DPMJET and created an efficient scheme to propagate correlated model uncertainties into derived lepton fluxes. In this seminar I will present the atmospheric neutrino and hadronic interaction phenomenology\, including the latest results obtained \nwith MCEq and the Global Spline Fit (GSF) flux model.
URL:https://ecap.nat.fau.de/index.php/event/anatoli-fedynitch-state-of-the-art-atmospheric-lepton-flux-tools/
LOCATION:ECAP\, room 307\, Erwin-Rommel-Str 1\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
END:VCALENDAR