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:20200329T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20201025T010000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20200109T120000
DTEND;TZID=Europe/Berlin:20200109T130000
DTSTAMP:20260418T070456
CREATED:20191017T130525Z
LAST-MODIFIED:20191017T130525Z
UID:2800-1578571200-1578574800@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Klaus Desch
DESCRIPTION:Axions from Sun? Exploring the low-energy frontier with the IAXO experiment\nAxions are ultralight hypothetical particles originally postulated to explain the observed smallness of the neutron´s electric dipole moment and its connection with the so-called strong CP-problem\, i.e. the fact that QCD allows for CP violation while Nature apparently does not. Meanwhile it is clear that axions\, and more generally axion-like particles (ALPs)\, may also serve as interesting candidates for the observed Dark Matter and may explain certain astrophysical anomalies. If axions exist\, they are copiously produced in our Sun and may be detected through their small effective coupling to electro-magnetic fields. A promising approach is their conversion into soft X-ray photons in strong magnetic fields and subsequent detection.\nIn the talk\, I will lay out the experimental scene of axion searches around the globe and then focus on a new proposal\, the International Axion Observatory (IAXO) and its smaller predecessor\, BabyIAXO to be constructed at DESY in Hamburg. I will discuss the layout of the experiment\, ongoing R&D towards its realization and its sensitivity and discovery potential as well the time scale towards realization.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-klaus-desch/
LOCATION:ECAP\, room 307\, Erwin-Rommel-Str 1\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20200116T120000
DTEND;TZID=Europe/Berlin:20200116T130000
DTSTAMP:20260418T070456
CREATED:20191203T133851Z
LAST-MODIFIED:20191203T133851Z
UID:2913-1579176000-1579179600@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Jim Hinton
DESCRIPTION:HAWC\n[abstract not available yet]
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-jim-hinton/
LOCATION:ECAP\, room 307\, Erwin-Rommel-Str 1\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20200123T120000
DTEND;TZID=Europe/Berlin:20200123T130000
DTSTAMP:20260418T070456
CREATED:20191203T133711Z
LAST-MODIFIED:20191203T133711Z
UID:2911-1579780800-1579784400@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Brian Reville
DESCRIPTION:Cosmic-ray acceleration – limits and laboratories\nI will review the current theoretical status of shock acceleration at supernova type shocks\, with an emphasis on the plasma theory and implications for limitation on maximum energy. The current hypotheses will be put to the test in a surprising scaled down laboratory\, the binary system Eta Carinae.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-brian-reville/
LOCATION:ECAP\, room 307\, Erwin-Rommel-Str 1\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
END:VCALENDAR