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X-WR-CALNAME:LAPTh
X-ORIGINAL-URL:https://www.lapth.cnrs.fr/en/
X-WR-CALDESC:Events for LAPTh
REFRESH-INTERVAL;VALUE=DURATION:PT1H
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X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:UTC
BEGIN:STANDARD
TZOFFSETFROM:+0000
TZOFFSETTO:+0000
TZNAME:UTC
DTSTART:20250101T000000
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END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=UTC:20260128T150000
DTEND;TZID=UTC:20260128T160000
DTSTAMP:20260412T060611
CREATED:20260108T113912Z
LAST-MODIFIED:20260128T155345Z
UID:14401-1769612400-1769616000@www.lapth.cnrs.fr
SUMMARY:Ivano Basile - Horror vacui: instabilities in scale-separated Casimir compactifications
DESCRIPTION:Speakers: Ivano Basile (Garching\, Max Planck Inst.)\n.\nAbstract: Finding reliable scale-separated vacua with no moduli in the string landscape is a considerable challenge\, yet it is essential to connect string theory to our universe. Among several attempts\, toroidal compactifications supported by fluxes and Casimir energy stand out for their simplicity and degree of parametric control. In particular\, there exist simple such compactifications of eleven-dimensional supergravity leading to non-supersymmetric weakly curved anti-de Sitter solutions in four dimensions. I will show that these solutions are perturbatively (and non-perturbatively) unstable\, and thus do not pertain to bona fide four-dimensional effective field theories.\nLink: Zoom\nAnLy: https://sites.google.com/view/anlystringsandfields\n \n \nhttps://indico.in2p3.fr/event/38238/
URL:https://www.lapth.cnrs.fr/en/event/ivano-basile-horror-vacui-instabilities-in-scale-separated-casimir-compactifications/
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260129T130000
DTEND;TZID=UTC:20260129T153000
DTSTAMP:20260412T060611
CREATED:20260122T132329Z
LAST-MODIFIED:20260129T151059Z
UID:15059-1769691600-1769700600@www.lapth.cnrs.fr
SUMMARY:Physique fondamentale à partir de la structure à grande échelle de l'Univers à travers / Fundamental physics from large-scale structure across cosmic times)
DESCRIPTION:Speakers: Azadeh Moradinezhad (Laboratoire d’Annecy-le-Vieux de Physique Théorique (LAPTh))\nLe modèle /CDM décrit remarquablement bien l’Univers observé\, mais il ne rend pas compte de l’origine des structures ni de lanature du secteur sombre. La précision croissante des observations met en évidence des tensions pouvant signaler une nouvellephysique. Dans cet exposé\, je présenterai mes travaux et mon programme à venir pour exploiter les structures à grande échelle etrechercher de telles signatures à partir de deux observables complémentaires : le regroupement des galaxies et la cartographie enintensité de raies spectrales (LIM). L’essentiel de l’information encore sous-exploitée se situe (i) aux petites échelles non linéaires\, oùl’on peut réduire la variance d’échantillonnage en moyennant sur de nombreuses structures indépendantes\, à condition de modélisercorrectement les non-linéarités et les effets baryoniques\, et (ii) à grand décalage vers le rouge\, où les fluctuations restent plusproches des conditions initiales. Je présenterai des avancées pour extraire l’information non gaussienne du regroupement etmontrerai comment la LIM mm/sub-mm étend les analyses de LSS à haut redshift/décalage vers le rouge grâce à une atténuationrobuste des premiers plans et une modélisation précise du signal. Je conclurai en montrant comment la complémentarité desprincipales sondes de la LSS peut être exploitée dans des analyses multi-sondes cohérentes pour une cosmologie de précisionrobuste au-delà de la limite gaussienne.\nThe /CDM model has been remarkably successful in describing the observed Universe\, yet it does not explain the origin of structureor the nature of the dark sector. Growing observational precision is exposing tensions that may be early signs of new physics\,offering dues to these puzzles. ln this talk\, 1 will present my research over the last decade and outline my future program to exploitlarge-scale structure (LSS) to search for new-physics imprints using two complementary observables: galaxy clustering and lineintensitymapping (LIM). Much of the untapped information in LSS resides on small nonlinear scales\, where averaging over manyindependent features of the cosmic web can beat down sample variance if nonlinear and baryonic effects are modeled accurately\,and at high redshifts\, where fluctuations remain doser to the initial conditions. 1 will present advances in extracting non-Gaussianinformation from nonlinear clustering and show how mm/sub-mm LIM extends LSS analyses to the high-redshift Universe throughrobust foreground mitigation and accurate signal modeling. 1 will conclude by outlining how the complementarity of key LSS probescan be leveraged in coherent multi-probe analyses for robust precision cosmology beyond the Gaussian limit.\nhttps://indico.in2p3.fr/event/38478/
URL:https://www.lapth.cnrs.fr/en/event/azadeh-moradinezhad/
LOCATION:Auditorium (Annecy)
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260130T100000
DTEND;TZID=UTC:20260130T110000
DTSTAMP:20260412T060611
CREATED:20251221T122329Z
LAST-MODIFIED:20260130T105332Z
UID:13662-1769767200-1769770800@www.lapth.cnrs.fr
SUMMARY:Simulations and modeling for precision cosmology
DESCRIPTION:Speakers: Zarija Lukic\nOngoing and upcoming cosmology surveys aim to address some of the deepest questions in fundamental physics—from the nature of dark energy and dark matter to tests of gravity and particle physics on the largest observable scales. Interpreting these data\, which probe multiple cosmic epochs and physical scales\, is a formidable challenge: it is fundamentally an inverse problem in which we infer the underlying physics from imperfect\, biased\, and noisy observations. In this talk I will describe our simulation and modeling program at Berkeley Lab’s Computational Cosmology Center to support inference using Lyman-α forest and intergalactic medium measurements. We have developed Nyx\, a highly efficient and scalable cosmological hydrodynamics code\, to generate high-fidelity realizations needed to connect theory to data\, such as DESI observations. However\, producing suites of full-physics simulations at the required accuracy remains computationally expensive\, motivating complementary approaches. I will discuss our work on emulators—surrogate models trained on finite ensembles of simulations—as well as new hybrid strategies that combine physical modeling with generative ML/AI approaches.\nhttps://indico.in2p3.fr/event/38053/
URL:https://www.lapth.cnrs.fr/en/event/tba/
LOCATION:Auditorium Vivargent (LAPTh)
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260205T090000
DTEND;TZID=UTC:20260205T160000
DTSTAMP:20260412T060611
CREATED:20260109T153919Z
LAST-MODIFIED:20260113T143942Z
UID:14488-1770282000-1770307200@www.lapth.cnrs.fr
SUMMARY:Repas de Noel
DESCRIPTION:https://indico.in2p3.fr/event/38246/
URL:https://www.lapth.cnrs.fr/en/event/repas-de-noel/
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260206T080000
DTEND;TZID=UTC:20260206T210000
DTSTAMP:20260412T060611
CREATED:20260107T073908Z
LAST-MODIFIED:20260206T205333Z
UID:14351-1770364800-1770411600@www.lapth.cnrs.fr
SUMMARY:Hommage à Richard Taillet
DESCRIPTION:L’UFR Science et Montagne (SceM) et le Laboratoire d’Annecy de Physique Théorique (LAPTh) de l’Université Savoie Mont Blanc organisent une journée en hommage à notre collègue Richard Taillet\, qui nous a quitté en été 2025.\nCette journée sera l’occasion de nous remémorer un collègue engagé et apprécié\, autant sur le plan de la recherche\, de l’enseignement\, de l’engagement au sein de notre établissement et de la vulgarisation scientifique\, que sur le plan personnel.\nLa capacité des salles étant limitée\, l’inscription est nécessaire si vous souhaitez participer en personne à la journée. Un formulaire de demande d’inscription est à votre disposition en ligne sur cette page. Les inscriptions seront confirmées dans la limite des places disponibles.\nhttps://indico.in2p3.fr/event/38226/
URL:https://www.lapth.cnrs.fr/en/event/hommage-a-richard-taillet/
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260206T090000
DTEND;TZID=UTC:20260206T160000
DTSTAMP:20260412T060611
CREATED:20251204T141951Z
LAST-MODIFIED:20260206T154005Z
UID:12910-1770368400-1770393600@www.lapth.cnrs.fr
SUMMARY:Journée hommage à Richard Taillet
DESCRIPTION:Plus d’information\nhttps://indico.in2p3.fr/event/37826/
URL:https://www.lapth.cnrs.fr/en/event/journee-hommage-a-richard-taillet/
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260212T100000
DTEND;TZID=UTC:20260212T110000
DTSTAMP:20260412T060611
CREATED:20260112T155444Z
LAST-MODIFIED:20260212T105324Z
UID:14606-1770890400-1770894000@www.lapth.cnrs.fr
SUMMARY:Gravitational probes of dark matter: off the beaten path
DESCRIPTION:Speakers: Kfir Blum (weizmann institute of science)\nMany astrophysical and cosmological systems show compelling positive evidence for the existence of dark matter. Yet\, as all of this positive evidence is based on gravitational effects\, the fundamental particle nature of dark matter remains unknown\, hidden behind the veil of the equivalence principle. I will discuss attempts to penetrate this veil\, still focusing on gravitational dynamics alone. First\, I consider ultralight dark matter\, a regime that arises if dark matter particles are so light that their de-Broglie wavelength attains astronomical scales. Dark matter in this regime can be constrained by detailed analyses of stellar distributions in galaxies of various shapes and sizes\, and can also leave an imprint in gravitational lensing observations. Second\, I consider\, more broadly\, the phenomenon of gravitational dynamical friction\, which offers a probe of dark matter beyond the mean-field level\, and — in some systems — provides compelling new evidence for dark matter in galaxies\, qualitatively different and independent from traditional stellar kinematics.\n \nhttps://indico.in2p3.fr/event/38255/
URL:https://www.lapth.cnrs.fr/en/event/kfir-blum/
LOCATION:Auditorium Vivargent (LAPTh)
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260217T100000
DTEND;TZID=UTC:20260217T110000
DTSTAMP:20260412T060611
CREATED:20260122T090924Z
LAST-MODIFIED:20260217T103845Z
UID:15026-1771322400-1771326000@www.lapth.cnrs.fr
SUMMARY:Journal Club
DESCRIPTION:see https://sdrive.cnrs.fr/s/NJmNfMtzFBfCkQy\nhttps://indico.in2p3.fr/event/38461/
URL:https://www.lapth.cnrs.fr/en/event/journal-club-2/
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260225T150000
DTEND;TZID=UTC:20260225T160000
DTSTAMP:20260412T060611
CREATED:20260202T092346Z
LAST-MODIFIED:20260225T155321Z
UID:15485-1772031600-1772035200@www.lapth.cnrs.fr
SUMMARY:Naman Agarwal - Toward an Effective Theory of the Volume Modulus
DESCRIPTION:Speakers: Naman Agarwal (University of Manitoba)\n.\nAbstract: In this talk\, I will talk about my recent work with collaborators where we investigate the 4-dimensional effective theory of the warped volume modulus in the presence of stabilizing effects from gaugino condensation by analyzing the linearized 10-dimensional supergravity equations of motion. Warping is generally expected to scale down the masses of bulk modes to the IR scale at the tip of a throat. We find that the mass of the warped volume modulus evades expectations and is largely insensitive to the effects of warping\, even in strongly warped backgrounds. Instead\, the mass is parametrically tied to the 4-dimensional AdS curvature scale m2∼O(1)R^AdSm2∼O(1)R^AdS​\, presenting a challenge for scale separation in these backgrounds. We trace this effect to a universal contribution arising from the 10-dimensional equations of motion\, and comment on the importance of a 10-dimensional treatment of the warped volume modulus for effective field theories and model building.\nLink: Zoom\nAnLy: https://sites.google.com/view/anlystringsandfields\n \n \nhttps://indico.in2p3.fr/event/38783/
URL:https://www.lapth.cnrs.fr/en/event/naman-agarwal-tba/
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260226T100000
DTEND;TZID=UTC:20260226T110000
DTSTAMP:20260412T060611
CREATED:20251216T160900Z
LAST-MODIFIED:20260226T103823Z
UID:13453-1772100000-1772103600@www.lapth.cnrs.fr
SUMMARY:Integrable boundary-driven quantum circuits with different geometries
DESCRIPTION:Speakers: Ana Retore (DESY)\nA quantum circuit is a way to simulate the time evolution of many-body operators where the scattering can be factorized into two body scattering operators for the bulk and one body operators for the boundaries.  Integrability is a property where the presence of hidden symmetries in a model gives rise to a  powerful toolkit to solve this model. This talk brings these two concepts together.\nIntegrability in a quantum circuit means that the circuit time evolution commutes with the conserved charges of the model giving rise to many tools to solve this model.They present several advantages\, including reduced noise propagation when compared to non-integrable circuits\, as well as the possibility to use integrability-based techniques to understand transport properties of quantum many-body systems.\nThese features motivated us to systematically classify integrable quantum circuits with open boundary conditions. In this talk\, after an introduction to quantum circuits and their importance\, I will present a construction of integrable boundary-driven quantum circuits with different geometries (positions of the gates) and discuss some examples.\n \nhttps://indico.in2p3.fr/event/38028/
URL:https://www.lapth.cnrs.fr/en/event/ana-retore/
LOCATION:Auditorium Vivargent (LAPTh)
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260303T100000
DTEND;TZID=UTC:20260303T110000
DTSTAMP:20260412T060611
CREATED:20260122T091011Z
LAST-MODIFIED:20260303T105327Z
UID:15027-1772532000-1772535600@www.lapth.cnrs.fr
SUMMARY:Journal Club
DESCRIPTION:see https://sdrive.cnrs.fr/s/NJmNfMtzFBfCkQy\nhttps://indico.in2p3.fr/event/38462/
URL:https://www.lapth.cnrs.fr/en/event/journal-club-3/
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260305T100000
DTEND;TZID=UTC:20260305T110000
DTSTAMP:20260412T060611
CREATED:20251230T145415Z
LAST-MODIFIED:20260305T105420Z
UID:14033-1772704800-1772708400@www.lapth.cnrs.fr
SUMMARY:Colliders in the Sky: Constraining High-Energy Physics with CMB and LSS Observations
DESCRIPTION:Speakers: Oliver Philcox (Stanford University)\nInflation is amongst the most mysterious phenomena in physics. With an energy scale potentially reaching 10^13 TeV\, its physical description likely lies far beyond the realm of the standard model. This leaves many questions unanswered: what fields were present during inflation? how did they interact with each other? In this talk\, I will discuss how modern cosmological datasets can be used to shed light on the early Universe by searching for the tell-tale signs of “primordial non-Gaussianity”. In particular\, I will present new searches for inflationary signals in Cosmic Microwave Background and Galaxy Survey data\, which allow for a detailed study of the primordial three- and four-point functions. Leveraging an array of theoretical and computational tricks\, these methods can place constraints on the microphysics of inflation and directly probe particle scattering processes in the early Universe\, acting as a “cosmological collider”. I will close by discussing future avenues of exploration and prospects for upcoming galaxy surveys. \nhttps://indico.in2p3.fr/event/38090/
URL:https://www.lapth.cnrs.fr/en/event/tba-2/
LOCATION:Salle des Sommets (LAPTh)
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260309T070000
DTEND;TZID=UTC:20260313T170000
DTSTAMP:20260412T060611
CREATED:20251204T142027Z
LAST-MODIFIED:20260313T165455Z
UID:12911-1773039600-1773421200@www.lapth.cnrs.fr
SUMMARY:2nd UNDARK School: The multi-messenger non-thermal universe
DESCRIPTION:The UNDARK’s Second Scientific School will be held in Annecy (France) at the LAPTh\, a world-class research laboratory just 40 km away from CERN\, from the 9th – 13th March 2026.\n \nUNDARK Scientific Schools are week-long events aimed at equipping PhD students in the field of astroparticle physics with theoretical\, phenomenological and numerical tools at the forefront of their field of research. The 2nd UNDARK Scientific School will focus on the multi-messenger non-thermal universe\, including astrophysics of radio to gamma-ray observations and tests of fundamental physics.\nNo fee will be charged to participating students. A maximum of 30 students will be accepted. Coffee breaks\, lunches and up to two dinners will be offered to the participants.Upon request and depending on funding\, a few travel grants will be awarded to students. \nThe UNDARK consortium\, where UNDARK stands for Unravelling the Dark Universe from the Canary islands Observatories\, aims at resolving the constituents and the laws which govern this dark side of the universe. The consortium is led by the IAC\, in partnership with CERN\, IFAE\, WIS and LAPTh. More information can be found in the UNDARK’s website.\nUNDARK’s first school was organized by IFAE and held at the Benasque Science Center (Benasque\, Spain) from March 9 to March 15\, 2025.\n \nGraphic design: Ève Barlier\, UNDARK\, 2025\n \nSchool Picture 1\nSchool Picture 2\n \nhttps://indico.in2p3.fr/event/36693/
URL:https://www.lapth.cnrs.fr/en/event/2nd-undark-school-the-multi-messenger-non-thermal-universe/
LOCATION:Auditorium Vivargent (Campus du CNRS)
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260317T100000
DTEND;TZID=UTC:20260317T110000
DTSTAMP:20260412T060611
CREATED:20260122T091059Z
LAST-MODIFIED:20260317T105305Z
UID:15028-1773741600-1773745200@www.lapth.cnrs.fr
SUMMARY:Journal Club
DESCRIPTION:see https://sdrive.cnrs.fr/s/NJmNfMtzFBfCkQy\nhttps://indico.in2p3.fr/event/38463/
URL:https://www.lapth.cnrs.fr/en/event/journal-club-4/
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260318T150000
DTEND;TZID=UTC:20260318T160000
DTSTAMP:20260412T060611
CREATED:20260315T153807Z
LAST-MODIFIED:20260318T155312Z
UID:17305-1773846000-1773849600@www.lapth.cnrs.fr
SUMMARY:Victor Franken - Holographic quantum tasks in the static patch
DESCRIPTION:Speakers: Victor Franken (Gent Univ.)\n.\nAbstract: In the AdS/CFT correspondence\, direct scattering in the bulk may not have a local boundary analog. A nonlocal implementation on the boundary requires O(1/G​) mutual information. This statement is formalized by the connected wedge theorem\, which can be proven using general relativity within AdS_3​ but also by applying quantum information theory on the boundary\, suggesting that the theorem applies to any holographic duality. We examine scattering within the static patch of asymptotically dS_3 spacetime\, which is conjectured to be described by a quantum theory on the stretched horizon in static patch holography. We prove that causality on the horizon should be induced from null infinities to maintain consistency with the theorem. Specifically\, signals propagating in the static patch are associated with local operators at null infinity. These results suggest a novel connection between static patch holography and the dS/CFT correspondence.\nLink: Visio\nAnLy: https://sites.google.com/view/anlystringsandfields\n \n \nhttps://indico.in2p3.fr/event/39166/
URL:https://www.lapth.cnrs.fr/en/event/victor-franken-holographic-quantum-tasks-in-the-static-patch/
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260331T090000
DTEND;TZID=UTC:20260331T100000
DTSTAMP:20260412T060611
CREATED:20260122T091105Z
LAST-MODIFIED:20260319T053804Z
UID:15029-1774947600-1774951200@www.lapth.cnrs.fr
SUMMARY:Journal Club
DESCRIPTION:see https://sdrive.cnrs.fr/s/NJmNfMtzFBfCkQy\nhttps://indico.in2p3.fr/event/38464/
URL:https://www.lapth.cnrs.fr/en/event/journal-club-5/
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260402T090000
DTEND;TZID=UTC:20260402T100000
DTSTAMP:20260412T060611
CREATED:20260309T142439Z
LAST-MODIFIED:20260319T053804Z
UID:17039-1775120400-1775124000@www.lapth.cnrs.fr
SUMMARY:Abhishek MANIYAR
DESCRIPTION:Speakers: Abhishek Maniyar (CNRS – LAPTh)\nTBA\nhttps://indico.in2p3.fr/event/39119/
URL:https://www.lapth.cnrs.fr/en/event/tba-4/
LOCATION:Auditorium Vivargent (LAPTh)
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260414T090000
DTEND;TZID=UTC:20260414T100000
DTSTAMP:20260412T060611
CREATED:20260122T091113Z
LAST-MODIFIED:20260319T053805Z
UID:15030-1776157200-1776160800@www.lapth.cnrs.fr
SUMMARY:Journal Club
DESCRIPTION:see https://sdrive.cnrs.fr/s/NJmNfMtzFBfCkQy\nhttps://indico.in2p3.fr/event/38465/
URL:https://www.lapth.cnrs.fr/en/event/journal-club-6/
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260428T090000
DTEND;TZID=UTC:20260428T100000
DTSTAMP:20260412T060611
CREATED:20260122T091118Z
LAST-MODIFIED:20260319T053805Z
UID:15031-1777366800-1777370400@www.lapth.cnrs.fr
SUMMARY:Journal Club
DESCRIPTION:see https://sdrive.cnrs.fr/s/NJmNfMtzFBfCkQy\nhttps://indico.in2p3.fr/event/38467/
URL:https://www.lapth.cnrs.fr/en/event/journal-club-7/
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260507T090000
DTEND;TZID=UTC:20260507T100000
DTSTAMP:20260412T060611
CREATED:20251219T142601Z
LAST-MODIFIED:20260319T053805Z
UID:13579-1778144400-1778148000@www.lapth.cnrs.fr
SUMMARY:Viktor EISLER
DESCRIPTION:Speakers: Viktor Eisler (Institute of Theoretical and Computational Physics  TU Graz)\nTBA\nhttps://indico.in2p3.fr/event/38044/
URL:https://www.lapth.cnrs.fr/en/event/viktor-eisler/
LOCATION:Auditorium Vivargent (LAPTh)
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260512T090000
DTEND;TZID=UTC:20260512T100000
DTSTAMP:20260412T060611
CREATED:20260122T091204Z
LAST-MODIFIED:20260319T053806Z
UID:15032-1778576400-1778580000@www.lapth.cnrs.fr
SUMMARY:Journal Club
DESCRIPTION:see https://sdrive.cnrs.fr/s/NJmNfMtzFBfCkQy\nhttps://indico.in2p3.fr/event/38468/
URL:https://www.lapth.cnrs.fr/en/event/journal-club-8/
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260521T090000
DTEND;TZID=UTC:20260521T100000
DTSTAMP:20260412T060611
CREATED:20260318T175313Z
LAST-MODIFIED:20260319T053806Z
UID:17453-1779354000-1779357600@www.lapth.cnrs.fr
SUMMARY:Frank Qu
DESCRIPTION:Speakers: Frank Qu (Stanford University)\nTBA\nhttps://indico.in2p3.fr/event/39269/
URL:https://www.lapth.cnrs.fr/en/event/frank-qu/
LOCATION:Auditorium Vivargent (LAPTh)
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260526T090000
DTEND;TZID=UTC:20260526T100000
DTSTAMP:20260412T060611
CREATED:20260122T091209Z
LAST-MODIFIED:20260319T053807Z
UID:15033-1779786000-1779789600@www.lapth.cnrs.fr
SUMMARY:Journal Club
DESCRIPTION:see https://sdrive.cnrs.fr/s/NJmNfMtzFBfCkQy\nhttps://indico.in2p3.fr/event/38469/
URL:https://www.lapth.cnrs.fr/en/event/journal-club-9/
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260528T090000
DTEND;TZID=UTC:20260528T100000
DTSTAMP:20260412T060611
CREATED:20260209T085448Z
LAST-MODIFIED:20260319T053807Z
UID:15780-1779958800-1779962400@www.lapth.cnrs.fr
SUMMARY:Azadeh MALEKNEJAD
DESCRIPTION:Speakers: Azadeh Maleknejad (Swansea University)\nTBA\nhttps://indico.in2p3.fr/event/38874/
URL:https://www.lapth.cnrs.fr/en/event/tba-3/
LOCATION:Auditorium Vivargent (LAPTh)
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260604T090000
DTEND;TZID=UTC:20260604T100000
DTSTAMP:20260412T060611
CREATED:20251219T142610Z
LAST-MODIFIED:20260319T053807Z
UID:13580-1780563600-1780567200@www.lapth.cnrs.fr
SUMMARY:Eric VERNIER
DESCRIPTION:Speakers: Eric Vernier\nTBA\nhttps://indico.in2p3.fr/event/38045/
URL:https://www.lapth.cnrs.fr/en/event/eric-vernier/
LOCATION:Auditorium Vivargent (LAPTh)
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260609T060000
DTEND;TZID=UTC:20260609T170000
DTSTAMP:20260412T060611
CREATED:20260204T221025Z
LAST-MODIFIED:20260319T053808Z
UID:15602-1780984800-1781024400@www.lapth.cnrs.fr
SUMMARY:AnLy 8th in-person Meeting
DESCRIPTION:This is the 8th instance of the in-person AnLy meetings between neighboring institutions (IP2I Lyon\, LAPTh Annecy\, LPENSL Lyon) on string and field theory topics. It will take place at LAPTh\, Annecy\, on the 09th June 2026.\n \nTravel: Options between Lyon and Annecy are train (or train + bus)\, Flixbus\, or car (and car-sharing).\nRecommended trains: 08:08 (Lyon Part-Dieu) – 10:07 (Annecy) ; 17:43 (Annecy) – 19:52 (Lyon Part-Dieu)\n \nLunch: It will be provided to registered participants of the meeting.\n \nRegistration: It opens on the 15th April and closes on the 15th May 2026.\n \nhttps://indico.in2p3.fr/event/38840/
URL:https://www.lapth.cnrs.fr/en/event/anly-8th-in-person-meeting/
LOCATION:Auditorium – Grande Galerie (LAPTh)
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260907T113000
DTEND;TZID=UTC:20260911T120000
DTSTAMP:20260412T060611
CREATED:20260219T150949Z
LAST-MODIFIED:20260319T053808Z
UID:16194-1788780600-1789128000@www.lapth.cnrs.fr
SUMMARY:RAQIS 26
DESCRIPTION:Recent Advances in Quantum Integrable Systems 2026\nThis international meetings aim at bringing in contact people working on various aspects of the Theory of Quantum Integrable Systems. Applications of Integrable Systems\, such as string/gauge theories\, condensed matter physics or statistical physics are also emphasized.\nFees\nThe registration fee is 200 EUR up to June 30th. It is 250 EUR for late registration (up to July 31st). Fees include lunches (08-09-10-11/09)\, coffee-breaks and the conference dinner. Fee payment confirms participation and inscription on the list of participants.\nAccomodation\nThe participants are asked to book their accommodation by themselves. Be aware that Annecy is a very touristic place\, book in advance!\n \nWeb site addresshttps://indico.in2p3.fr/e/raqis26\nhttps://indico.in2p3.fr/event/38960/
URL:https://www.lapth.cnrs.fr/en/event/raqis-26/
LOCATION:Auditorium (LAPTh)
END:VEVENT
END:VCALENDAR