BEGIN:VCALENDAR
PRODID://WordPress//Event-Post-V5.9.2//EN
VERSION:2.0
BEGIN:VTIMEZONE
TZID:Europe/Madrid
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
DTSTART:19700329T020000
RRULE:FREQ=YEARLY;BYDAY=-1SU;BYMONTH=3
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:19701025T030000
RRULE:FREQ=YEARLY;BYDAY=-1SU;BYMONTH=10
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
SUMMARY:Charla de Bodo Schwabe sobre "fuzzy dark matter"
UID:https://capa.unizar.es/?p=1228
LOCATION:
DTSTAMP:20211104T120000
DTSTART;TZID=Europe/Madrid:20211104T120000
DTEND;TZID=Europe/Madrid:20211104T120000
DESCRIPTION:Bodo Schwabe is a PostDoc Researcher at CAPA, focused on dark matter,
axions and numerical simulations.

Abstract: On linear scales much larger than the typical extend of galaxies
the standard model of cosmology with cold dark matter and a cosmological
constant can reproduce observational data with high precision. But there
are potential difficulties on galactic scales. In this 50 minutes master
level lecture I will present the main concepts of fuzzy dark matter, a well
motivated dark matter candidate that reproduces the successes of cold dark
matter on large scales, while implying unique observable features like
solitons and interference patterns within halos and filaments. During the
lecture I will derive the equations of motion governing the evolution of
fuzzy dark matter, concentrating on their physical implications. While
conceptionally simply, solving these non-linear equations requires
intensive numerical computations. Alongside the theoretical considerations
I will therefore present numerical methods that have been used to analyse
non-linear dynamics of fuzzy dark matter on (sub-)galactic scales
END:VEVENT
END:VCALENDAR