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SUMMARY:INAF PhD School Francesco Lucchin - Venezia 2027 - Gravitational W
 aves\, Neutrinos and the Transient Universe
DTSTART:20270404T140000Z
DTEND:20270409T120000Z
DTSTAMP:20261031T212600Z
UID:indico-event-3694@indico.ict.inaf.it
CONTACT:Lucchin_mm_soc@googlegroups.com\;Lucchin_mm_loc@googlegroups.com
DESCRIPTION:The School will take place on San Servolo island\, Venice\, f
 rom April 4 to 9\, 2027.\nAbout the School\nForty years after SN 1987A—t
 he first astrophysical event observed with both electromagnetic radiation 
 and neutrinos—and ten years after GW170817\, which ushered in the era of
  multi-messenger astronomy with gravitational wave (GW) sources\, the stud
 y of the transient Universe is entering a new frontier.\nToday’s GW astr
 onomy relies on LIGO\, Virgo\, and KAGRA\, while neutrino astronomy is dri
 ven by facilities like Super-Kamiokande\, IceCube\, and KM3NeT. In the com
 ing years\, next-generation facilities such as the Einstein Telescope\, LI
 SA\, and LGWA will revolutionize GW astronomy\, complemented by Hyper-Kami
 okande and upgrades to existing neutrino detectors. At the same time\, maj
 or electromagnetic observatories — including the Vera C. Rubin Observato
 ry\, SKAO\, and CTAO — will dramatically expand our capacity to discover
  and follow up on transient sources. This evolving landscape offers early-
 career researchers a unique opportunity to probe the high-energy\, rapidly
  changing Universe through a multi-messenger\, multi-wavelength approach.\
 nProgram Overview\nThe curriculum is organized into two complementary focu
 s areas:\nMulti-Messenger Astrophysics: Covers the physics of GWs across a
  wide frequency spectrum and astrophysical neutrinos across a broad energy
  range—from MeV energies (critical for early-phase core-collapse superno
 vae) to the TeV–PeV regime characteristic of high-energy sources. Key de
 tection principles and instrumentation will also be addressed.\nTransient 
 Astronomy: Focuses on electromagnetic counterparts to GW and neutrino even
 ts\, including Novae\, Supernovae\, Kilonovae\, GRBs\, and AGNs. Lectures 
 will cover observing strategies\, modern survey facilities\, and advanced 
 monitoring and follow-up methods.\nThe primary objective of the program is
  to accelerate participants' academic and professional development by buil
 ding a strong\, shared foundation in theoretical and observational frontie
 rs.\nTarget Audience & Application Details\nThe Lucchin schools are primar
 ily designed for PhD students enrolled in Physics and Astronomy programs i
 n Italy. International PhD students and interested early-career postdocs/r
 esearchers are also welcome to apply.\nNote: Because capacity is limited\,
  foreign applicants and non-PhD researchers are welcome to register\, but 
 their admission must be confirmed by the organizers.\n\n\n \n        
    \n\nhttps://indico.ict.inaf.it/event/3694/
URL:https://indico.ict.inaf.it/event/3694/
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