Cosmic Rays and Neutrinos in the Multi-Messenger Era

9 déc. 2024, 08:00 → 13 déc. 2024, 19:00 Europe/Paris

APC Laboratory (Paris)

The 'Cosmic Rays  in the Multi-Messenger Era' conference aims to bring together the scientific communities working on high-energy cosmic rays, from an experimental point of view as well as from a theoretical and phenomenological sides. In addition to detailed presentations of theoretical models dealing with the production of cosmic rays and secondary neutrinos and gamma-rays, the conference will include reviews of the latest experimental results as well as prospects for the next decade.

Each session will end with general discussion of presented results. Additionally we organize poster session for PhD students and young researchers.

Organizing committee: 

G. de Wasseige, co-chair 
S. Gabici 
M. Kachelriess, co-chair  
A. Kouchner
M. Lemoine 
A. Neronov 
D. Semikoz, chair 
S.Vydelingum, secretary

lundi 9 décembre

08:30 → 09:00 Registration

09:00 → 09:10 Welcome

Orateur: Dmitri SEMIKOZ (APC, Paris)

09:10 → 12:00 UHECRs

09:10 Telescope Array results

Orateur: Yoshiki Tsunesada

09:40 Auger results

Orateur: Ralph Engel

10:10 Coffee

10:30 New developments in EPOS : toward a global approach from Heavy Ions to Cosmic Rays

Orateur: Tanguy Pierog

11:00 QGSJet 3.1

Orateur: Sergey Ostapchenko

11:30 Discussion UHECR

12:00 → 13:30 Lunch

13:30 → 15:30 GMF

13:30 GMF I

Orateur: Prof. Han

14:00 GMF II

Orateur: Prof. Michael Unger

14:30 GMF III

Orateur: Alexander Korochkin (ULB, Bruxelles)

15:00 Tomography Local Bubble+ all local stuff

Orateur: Vincent Pelgrims

15:30 → 16:00 Coffee

16:00 → 17:00 GMF2

16:00 CR and GMF

Orateur: Ch. Pfommer

16:30 Discussion GMF

17:00 → 20:30 Poster session

17:30 Poster Talks

18:30 Wine & cheese poster discussion

mardi 10 décembre

09:00 → 18:00 UHECR / Knee -- CRs

09:00 EGMF1

Orateur: Franco Vazza

09:30 EGMF2

Orateur: Klaus Dolag

10:00 Dipole Anisotopies UHECR

Orateur: Julien Aubert

10:30 Coffee

11:00 UHECR sources search review

Orateur: Teresa Bister

11:30 Discussion UHECR sources

12:00 Lunch

13:30 Theory propagation <-> GMF

Orateur: Gwenael Giacinti

14:00 Theory acceleration

Orateur: Luca Comisso

14:30 CR other experiments and IceTop; connection to HE

Orateur: Denis Soldin

15:00 LHAASO CRs

Orateur: Huihai He

15:30 Coffee

16:00 diffuse gamma-rays: summary experimental results

Orateur: TBD

16:30 Galactic diffuse gamma-rays (theory)

Orateur: Andrii Neronov

17:00 Discussion

mercredi 11 décembre

09:00 → 12:00 HE-gamma sources

09:00 Cherenkov telescopes new

Orateur: Jim Hinton

09:30 LHAASO gamma-ray review

Orateur: Zhen Cao

10:00 Leptonic/PSW nebula

Orateur: D. Khangulyan

10:30 Coffee

11:00 TeV halos

Orateur: T. Linden

11:30 SNR acceleration

Orateur: J. Vink

12:00 → 13:30 Lunch

13:30 → 15:30 MM

13:30 SNR Hadronic PeVatrons observations

Orateur: Ruizhi Yang

14:00 Hadronic PeVatrons/Super-bubbles

Orateur: Thibault Vieu

14:30 Transients

Orateur: Kohta Murase

15:00 Discussion

15:30 → 16:00 Coffee

16:00 → 19:30 Poster session

16:00 Poster Talks

18:00 Wine & cheese poster discussion

jeudi 12 décembre

09:00 → 18:30 Neutrinos

09:00 General update neutrinos

Orateur: Francis Halzen

10:00 The ANTARES legacy results

Orateur: Antoine Kouchner

10:30 Coffee

11:00 Baikal GVD

Orateur: Rastislav Dvornicky

11:30 IceCube from MeV to PeV

Orateur: Erin O'Sullivan

12:00 KM3NeT from MeV to PeV

Orateur: Aart Heijboer

12:30 Lunch

14:00 Radio detection of neutrinos

Orateur: Kumiko Kotera

14:30 Galactic neutrino searches (combined)

Orateur: Naoko Kurahashi

15:00 High energy astrophysical neutrinos: Open questions and future prospects

The main goals of high-energy neutrino astronomy are to identify the sources of high-energy cosmic rays, particularly ultra-high-energy ones, and to provide information on the acceleration process and constraints on models of high-energy astronomical objects. The detection of high-energy astronomical neutrinos demonstrates the potential for achieving these goals. I will discuss what we have learned from current neutrino observations and the prospects for making progress on identifying the sources.

Orateur: Eli Waxman

15:30 Coffee

15:30 Discussion

16:30 MM in transients

Orateur: Walter Winter

17:00 Real-time astronomy

Orateur: Marcos Santander

17:30 Connection gamma-neutrino-CR

Orateur: Foteini Oikonomou

18:00 New physics with neutrino telescopes

Orateur: Carlos Argüelles

20:00 → 22:00 Conference dinner

vendredi 13 décembre

09:00 → 12:30 Low-energy CRs -- "Escape problem"

09:00 DAMPE: B/C, heavier nuclei, e^++e^-

Orateur: Francesca Alemanno

09:30 CALET, B/C, heavier nuclei, e^++e^-

Orateur: Paolo Maestro

10:00 AMS-02: Be9/10, escape times

Orateur: Alberto Oliva

10:30 Coffee

11:00 Interpretation breaks 200GV, 10TV: source/diffusion

Orateur: Carmelo Evoli

12:00 Discussion

12:30 → 13:15 Conference summary

Orateur: Felix Aharonian