Registration & Coffee Room: Albano 3: 6203 - Floor 6 Large Lunch Room (44 seats)

Weclome

• Christian Glaser (Uppsala University)
• Chad Finley (Stockholm University)

Room: Albano 3: 4205 - SU Conference Room (40 seats)

Overview of the Experimental Landscape

• Christian Glaser (Uppsala University)

Room: Albano 3: 4205 - SU Conference Room (40 seats)

Discussion Room: Albano 3: 4205 - SU Conference Room (40 seats)

Optical Cherenkov from Space

• Mary Reno

Room: Albano 3: 4205 - SU Conference Room (40 seats)

Discussion Room: Albano 3: 4205 - SU Conference Room (40 seats)

Fundamental physics with PeV-EeV neutrinos

• Carlos Argüelles (Harvard)

Expectations for cosmogenic neutrinos

• Walter Winter (DESY)

AGN Neutrino factories beyond PeV energies

• Elisa Resconi (TU Munich)

What can we learn from UHE neutrino sources?

• Kohta Murase (Penn State)

Discussion

• Kohta Murase (Penn State)

Coffee

UHE detection forecasts for fluxes and cross sections

• Mauricio Bustamante (NBI)

Discussion

• Mauricio Bustamante (NBI)

Discussion, radio detection technique and performance

• Nils Heyer (Uppsala University)
• Christian Glaser (Uppsala University)

Flavor Composition fromm 100 TeV to EeV

• Mauricio Bustamante (NBI)

UHE Neutrinos and UHECRs from sources. Example: Tidal Disruption Events

• Walter Winter (DESY)

Cosmogenic neutrino sources

• Markus Ahlers (NBI)

Future radar echo telescope

• Krijn de Vries (VUB, Brussels)

Discussion (all)

Prompt neutrinos from GRBs in internal shock models

• Walter Winter (DESY)

Discussion

Cosmogenic neutrinos from a subdominant UHE proton component

• Arjen van Vliet (Khalifa University)

Discussion

O(10-100) GeV neutrino astronomy

• Jason Koskinen (NBI)

Discussion

Multimessenger connection in diffuse neutrino and gamma-ray fluxes

• Kohta Murase (Penn State)

Discussion

Non-jetted active galactic nuclei as neutrino emitters, with a focus on NGC 1068

• Paolo Padovani (European Southern Observatory)

Discussion

Coffee

High-energy neutrinos from supermassive black holes

• Kohta Murase (Penn State)

Discussion

KM3NeT and detection of an extremely high-energy neutrino

• Aart Heijboer (Univ. Amsterdam)

Discussion

Coffee

Galactic Diffuse Neutrino Emission from Sources beyond the Discovery Horizon

• Kathrine Groth (NBI)
• Markus Ahlers (NBI)

Discussion

Neutrino emission from (Ultra-)Luminous Infrared Galaxies

• Krijn de Vries (VUB, Brussels)

Discussion

Neutrinos from blazar flares

• Foteini Oikonomou (NTNU)

High-energy neutrino transients

• Kohta Murase (Penn State)

Discussion

What can multiple high-energy neutrino telescopes achieve together?

• Mauricio Bustamante (NBI)

Welcome to Week 3 and Supernova Neutrinos (Evan O'Connor, Erin O'Sullivan)

Day 1: High energy supernova neutrinos (above 100 MeV) Erin O’Sullivan - Detecting supernovae with high energy neutrinos in IceCube Shunsaku Horiuchi - Quasi-thermal neutrinos Hiroki Nagakura - Neutrino shock acceleration Evan O’Connor - Neutrino Echos (almost 100MeV)

Day 2: Supernova neutrino detection and multi-messenger followup Jim Kneller - SNEWPY 2.0 Shuai Zha - JUNO Erin O’Sullivan - Complementarity between supernova neutrino detectors Haakon Andresen - Neutrinos and Gravitational Waves David Vartanyan - CCSNe Physics from Neutrino Detection Hiroki Nagakura - Joint analysis of neutrinos and GWs for nearby CCSNe Shunsaku Horiuchi - Target lists Shirley Li - Simulations and 87A data

Day 3: Oscillations and flavour physics Hiroki Nagakura - Neutrino quantum kinetics Jim Kneller - Quantum Moments Evan O’Connor - Oscillation Explorations in FLASH Sean Couch - Constraining Neutrino Oscillations with Gravitational Waves

Day 4: Diffuse supernova neutrino background and nuclear physics Shunsaku Horiuchi - pyDSNB Shuai Zha - QCD phase transition in supernovae and related neutrino signals

Day 5: Advances in supernova neutrino simulations (for example, transport, interactions) Haakon Andresen - Grey Neutrino Transport for Core-Collapse Supernovae (and possibly mergers) David Vartanyan - Many-Body Effects and Scattering in CCSNe