The Multimessenger Sky at Extreme Energies: From Sources to Fundamental Physics

Europe/Rome
Room D (Institute for Fundamental Physics of the Universe (IFPU))

Room D

Institute for Fundamental Physics of the Universe (IFPU)

Carmelo Evoli (Gran Sasso Science Institute), Mirko Boezio (INFN - Sezione di Trieste), Piero Ullio (SISSA)
Description

The coming decade will see a rapid expansion of multimessenger observations at the highest energies, from ultra-high-energy cosmic rays and very-high-energy gamma rays to neutrinos and gravitational waves. 

Bringing these messengers together offers a unique opportunity to pinpoint the most extreme astrophysical accelerators, unravel the physical conditions in their sources and environments, and test the fundamental laws of nature in regimes inaccessible on Earth. 

This workshop aims to create a focused forum for theorists and experimentalists to identify the key open questions, define robust strategies to connect data across messengers, and assess the discovery potential for physics beyond the Standard Model through ultra-high-energy radiation.

Invited speakers (confirmed): 

  • Roberto Aloisio (GSSI and INFN LNGS, Italy)
  • Denise Boncioli (University of L'Aquila and INFN LNGS, Italy)
  • Mauricio Bustamante (NBI, Denmark)
  • Zhen Cao (IHEP Beijing, China)
  • Marco Cirelli (LPTHE CNRS, Paris)
  • Luca Comisso (Columbia University, US)
  • Rosa Coniglione (INFN-LNS)
  • Olivier Deligny (Université Paris-Saclay, France)
  • Ralph Engel (KIT, Germany)
  • Stefano Gabici (APC, Paris)
  • Noémie Globus (UNAM, Mexico)
  • Glenny Farrar (New York University, US)
  • Francis Halzen (University of Wisconsin–Madison, US)
  • Dmitriy Khangulyan (IHEP Beijing, China)
  • Martin Lemoine (APC, Paris)
  • Paolo Lipari (INFN Rome, Italy)
  • Miguel Mostafá (Temple University, US)
  • Kotha Murase (Pennsylvania State University, US)
  • Andrii Neronov (ISDC, Geneva)
  • Lorenzo Perrone (INFN Lecce, Italy)
  • Elisa Resconi (TUM, Germany)
  • Michael Unger (KIT, Germany)

 

 

 

    • 9:30 AM 10:50 AM
      Multimessenger Detections: Status and Highlights: 1
    • 10:50 AM 11:20 AM
      Coffee break 30m
    • 11:20 AM 12:40 PM
      Multimessenger Detections: Status and Highlights: 2
    • 12:40 PM 2:00 PM
      Lunch break 1h 20m
    • 2:00 PM 3:20 PM
      Multimessenger Detections: Status and Highlights: 3
    • 3:20 PM 3:50 PM
      Coffee break 30m
    • 3:50 PM 5:00 PM
      Synthesis, Discussion & Outlook: Monday
    • 9:30 AM 10:50 AM
      The Galactic PeVatron Landscape: 1
    • 10:50 AM 11:20 AM
      Coffee break 30m
    • 11:20 AM 12:40 PM
      The Galactic PeVatron Landscape: 2
    • 12:40 PM 2:00 PM
      Lunch break 1h 20m
    • 2:00 PM 3:20 PM
      The Galactic PeVatron Landscape: 3
    • 3:20 PM 3:50 PM
      Coffee break 30m
    • 3:50 PM 4:50 PM
      Synthesis, Discussion & Outlook: Tuesday
    • 9:30 AM 10:50 AM
      Extragalactic Accelerators and Cosmological Messengers: 1
    • 10:50 AM 11:20 AM
      Coffee break 30m
    • 11:20 AM 12:40 PM
      Extragalactic Accelerators and Cosmological Messengers: 2
    • 12:40 PM 2:00 PM
      Lunch break 1h 20m
    • 2:00 PM 3:20 PM
      Extragalactic Accelerators and Cosmological Messengers: 3
    • 3:20 PM 3:50 PM
      Coffee break 30m
    • 3:50 PM 5:00 PM
      Synthesis, Discussion & Outlook: Wed
    • 9:30 AM 10:50 AM
      New Physics with Extreme-Energy Messengers: 1
    • 10:50 AM 11:20 AM
      Coffee break 30m
    • 11:20 AM 12:40 PM
      Next-Generation Observatories: 1
    • 12:40 PM 2:00 PM
      Lunch break 1h 20m
    • 2:00 PM 3:20 PM
      Next-Generation Observatories: 2
    • 3:20 PM 3:50 PM
      Coffee break 30m
    • 3:50 PM 5:00 PM
      Synthesis, Discussion & Outlook: Thursday
    • 9:30 AM 12:30 PM
      Synthesis, Discussion & Outlook: Friday
      • 9:30 AM
        Coffee break 30m
    • 12:30 PM 2:00 PM
      Lunch break 1h 30m