BEGIN:VCALENDAR
VERSION:2.0
METHOD:PUBLISH
CALSCALE:GREGORIAN
PRODID:-//WordPress - MECv6.4.2//EN
X-ORIGINAL-URL:https://www.lps.u-psud.fr/
X-WR-CALNAME:Laboratoire de physique des Solides
X-WR-CALDESC:
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-PUBLISHED-TTL:PT1H
X-MS-OLK-FORCEINSPECTOROPEN:TRUE
BEGIN:VEVENT
CLASS:PUBLIC
DTSTART;TZID=Europe/Paris:20230608T110000
DTEND;TZID=Europe/Paris:20230608T120000
DTSTAMP:20230527T093700
UID:MEC-ef0eff6088e2ed94f6caf720239f40d5@lps.u-psud.fr
CREATED:20230527
LAST-MODIFIED:20230920
PRIORITY:5
TRANSP:OPAQUE
SUMMARY:A.TOSCHI:Fluctuation diagnostics of pseudogap and d-wave superconductivity in the two-dimensional Hubbard model
DESCRIPTION:\n	In recent years, reliable approaches have been developed [1] to identify the dominant fluctuations driving the multifaceted phenomena of many-electron physics. Among those, the “fluctuation diagnostics" [2] was hitherto applied only to normal, paramagnetic phases, allowing to pinpoint the spin-fluctuation nature of the pseudogap occurring in the two-dimensional Hubbard model [1-2]. After extending the approach to the superconducting phase [3], we were able to identify antiferromagnetic fluctuations as the "pairing glue" of d-wave superconductivity both in the underdoped and the overdoped regime of the Hubbard model. However, the predominant magnetic fluctuations might significantly differ [4] from those of conventional spin-fluctuation theory.\n\n[1] T. Schäfer and A. Toschi, Journal of Physics: Condensed Matter 33, 214001 (2021). \n[2] O. Gunnarsson et al., Phys. Rev. Lett. 114, 236402 (2015). \n[3] Xinyang Dong, L. Del Re, A. Toschi and E. Gull, PNAS 119 e2205048119 (2022). \n[4] F. Krien, P. Worm, P. Chalupa-Gantner, A. Toschi and K. Held, Comm. Phys. 5, 336 (2022).\n
URL:https://www.lps.u-psud.fr/events/toschi2023/
ORGANIZER;CN=Andrej Mesaros:MAILTO:andrej.mesaros@universite-paris-saclay.fr
CATEGORIES:Séminaire de la Théorie de la Matière Condensée
LOCATION:Moyen amphi (LPS) + ONLINE (Zoom)
END:VEVENT
END:VCALENDAR
