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TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:19700329T020000
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BEGIN:VEVENT
UID:https://www.lupm.in2p3.fr/users/qcd/hepmad19
DTSTAMP:20191014T000000Z
SUMMARY:HEPMAD19
DTSTART:20191014T000000
DTEND:20191020T000000
LOCATION: Montpellier UM2
CLASS:PUBLIC
CATEGORIES:CONGRES
URL:https://www.lupm.in2p3.fr/users/qcd/hepmad19
END:VEVENT
BEGIN:VEVENT
UID:https://cfrcos2.sciencesconf.org/
DTSTAMP:20191113T000000Z
SUMMARY:CFRCOS2: l'astrophysique du rayonnement cosmique de basse énergie
DTSTART:20191113T000000
DTEND:20191115T000000
LOCATION: Montpellier UM2
CLASS:PUBLIC
CATEGORIES:CONGRES
URL:https://cfrcos2.sciencesconf.org/
END:VEVENT
BEGIN:VEVENT
UID:https://caffelattes.sciencesconf.org
DTSTAMP:20200511T000000Z
SUMMARY:CAFFE LATTES
DTSTART:20200511T000000
DTEND:20200515T000000
LOCATION: Montpellier UM2
CLASS:PUBLIC
CATEGORIES:CONGRES
URL:https://caffelattes.sciencesconf.org
END:VEVENT
BEGIN:VEVENT
UID:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=306
CLASS:PUBLIC
DTSTAMP:20190121T202431Z
CATEGORIES:SEMINAR
SUMMARY:The role of cosmic rays in the star formation process - RODGERS-LEE Dona
DESCRIPTION:Young stars are born surrounded in an envelope of dust and gas which in many cases forms a protoplanetary disk. These disks evolve and disperse within a few million years leaving behind newly-formed planetary systems. Nonetheless\, formulating a coherent explanation of the evolution of protoplanetary disks remains challenging. The importance and influence of magnetic fields\, for instance\, continues for the large part to be unclear. Protoplanetary disks are relatively cool and are thought to be only very weakly ionised which provides imperfect coupling to magnetic fields. Understanding the sources of ionisation\, such as cosmic rays\, present in the disks underpins our overall understanding of how these systems evolve and form planets. In recent years\, ALMA (Atacama Large Millimeter Array) observations have revolutionised the field. ALMA observations have been able to resolve substructure in protoplanetary disks\, to constrain the level of turbulence and in some cases to even constrain the ionisation rate. In this context\, numerical models are being developed to estimate the ionising effect of cosmic rays originating from the young star itself. These simulations can probe the ionisation rate\, as well as the effect on disk chemistry. Recent simulations also suggest that the ability of cosmic rays to penetrate and ionise disks is a disk mass dependent process and can be discussed in comparison to ALMA observations.
ATTENDEE;CN=RODGERS-LEE Dona:
STATUS:CONFIRMED
URL:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=306
DTSTART:20190917T140000
DTEND:20190917T160000
LOCATION:Grande Ourse Bât:13 Etg:1 No:0
END:VEVENT
BEGIN:VEVENT
UID:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=323
CLASS:PUBLIC
DTSTAMP:20190826T121223Z
CATEGORIES:SEMINAR
SUMMARY:TBA - INMAN Derek
DESCRIPTION:TBA
ATTENDEE;CN=INMAN Derek:
STATUS:CONFIRMED
URL:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=323
DTSTART:20190923T110000
DTEND:20190923T121500
LOCATION:Grande Ourse Bât:13 Etg:1 No:0
END:VEVENT
BEGIN:VEVENT
UID:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=320
CLASS:PUBLIC
DTSTAMP:20190718T123816Z
CATEGORIES:SEMINAR
SUMMARY:TBA - GIRART Josep m.
DESCRIPTION:TBA
ATTENDEE;CN=GIRART Josep m.:
STATUS:CONFIRMED
URL:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=320
DTSTART:20190926T140000
DTEND:20190926T163000
LOCATION:Andromede Bât:11 Etg:3 No:0
END:VEVENT
BEGIN:VEVENT
UID:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=318
CLASS:PUBLIC
DTSTAMP:20190420T183439Z
CATEGORIES:SEMINAR
SUMMARY:Towards high precision predictions for non-linear clustering of dark matter - JOYCE Michael
DESCRIPTION:tba
ATTENDEE;CN=JOYCE Michael:
STATUS:CONFIRMED
URL:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=318
DTSTART:20191003T140000
DTEND:20191003T153000
LOCATION:Grande Ourse Bât:13 Etg:1 No:0
END:VEVENT
BEGIN:VEVENT
UID:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=322
CLASS:PUBLIC
DTSTAMP:20190729T104638Z
CATEGORIES:SEMINAR
SUMMARY:Simulating the formation of primordial black holes - MUSCO Ilia
DESCRIPTION:TBA
ATTENDEE;CN=MUSCO Ilia:
STATUS:CONFIRMED
URL:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=322
DTSTART:20191008T140000
DTEND:20191008T151500
LOCATION:Grande Ourse Bât:13 Etg:1 No:0
END:VEVENT
BEGIN:VEVENT
UID:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=321
CLASS:PUBLIC
DTSTAMP:20190727T110756Z
CATEGORIES:SEMINAR
SUMMARY:A confirmer : LFV - UESAKA Yuichi
DESCRIPTION:A confirmer:LFV
ATTENDEE;CN=UESAKA Yuichi:
STATUS:CONFIRMED
URL:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=321
DTSTART:20191015T140000
DTEND:20191015T153000
LOCATION:Grande Ourse Bât:13 Etg:1 No:0
END:VEVENT
BEGIN:VEVENT
UID:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=317
CLASS:PUBLIC
DTSTAMP:20190419T091500Z
CATEGORIES:SEMINAR
SUMMARY:TBD - SETA Amit
DESCRIPTION:TBA
ATTENDEE;CN=SETA Amit:
STATUS:CONFIRMED
URL:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=317
DTSTART:20191112T140000
DTEND:20191112T160000
LOCATION:Grande Ourse Bât:13 Etg:1 No:0
END:VEVENT
BEGIN:VEVENT
UID:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=324
CLASS:PUBLIC
DTSTAMP:20190902T153810Z
CATEGORIES:SEMINAR
SUMMARY:Axions and anomalies - SMITH Christopher

ATTENDEE;CN=SMITH Christopher:
STATUS:CONFIRMED
URL:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=324
DTSTART:20191114T140000
DTEND:20191114T153000
LOCATION:Grande Ourse Bât:13 Etg:1 No:0
END:VEVENT
BEGIN:VEVENT
UID:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=325
CLASS:PUBLIC
DTSTAMP:20190912T144546Z
CATEGORIES:SEMINAR
SUMMARY:Lecture on Gravity mediated dark matter in extra dimensions - RIUS Nuria

ATTENDEE;CN=RIUS Nuria:
STATUS:CONFIRMED
URL:http://www.lupm.univ-montp2.fr/?page=seminaires&id_seminar=325
DTSTART:20191128T140000
DTEND:20191128T153000
LOCATION:Grande Ourse Bât:13 Etg:1 No:0
END:VEVENT
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