BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//LAPTh - ECPv6.15.17//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-WR-CALNAME:LAPTh
X-ORIGINAL-URL:https://www.lapth.cnrs.fr
X-WR-CALDESC:Évènements pour LAPTh
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-Robots-Tag:noindex
X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:UTC
BEGIN:STANDARD
TZOFFSETFROM:+0000
TZOFFSETTO:+0000
TZNAME:UTC
DTSTART:20240101T000000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=UTC:20250515T090000
DTEND;TZID=UTC:20250515T100000
DTSTAMP:20260405T105207
CREATED:20250408T130455Z
LAST-MODIFIED:20250508T120500Z
UID:10325-1747299600-1747303200@www.lapth.cnrs.fr
SUMMARY:Loops in the EFT/PT of Structure Formation
DESCRIPTION:Speakers: Zvonomir Vlah (Ruđer Bošković Institute and University of Cambridge)\n I will discuss recent developments in cosmological perturbation theory and the effective field theory (EFT) of large-scale structure. Current galaxy surveys like DESI and Euclid provide some of the cleanest probes of the universe on large cosmological scales. While the one-loop power spectrum (the two-point correlator) remains the standardised and widely adopted theoretical tool\, fully exploiting the potential of these new datasets requires extending our theoretical framework to higher loops and N-point correlators. I will outline the theoretical and computational challenges involved in going beyond the one-loop level and present recent results in the context of DESI and forthcoming Euclid data.\n \n \nhttps://indico.in2p3.fr/event/36159/
URL:https://www.lapth.cnrs.fr/event/zvonomir-vlah/
LOCATION:Auditorium Vivargent (LAPTh)
END:VEVENT
END:VCALENDAR