Solar Modulation and Dark Matter Workshop

Session

Morning session:

Nov 15, 2021, 10:30 AM

IFPU - Trieste

Conveners

Morning session:: Heliosphere modeling and cosmic rays propagation

• Riccardo Munini (Istituto Nazionale di Fisica Nucleare)

Morning session:: Solar modulation measurements and models

• Riccardo Munini (Istituto Nazionale di Fisica Nucleare)
• Bernd Heber (Christian-Albrechts-Universität zu kiel)

Morning session:: Indirect search for dark matter with low energy antinucleus

• Fiorenza Donato (Istituto Nazionale di Fisica Nucleare)

Morning session:: Propagation of cosmic rays in the galaxy and experimental measurements

• Carmelo Evoli (Gran Sasso Science Institute)

30. Welcome and general infomation

Riccardo Munini (Istituto Nazionale di Fisica Nucleare)

11/15/21, 10:30 AM

28. Cosmic rays below 100 TeV in the Galaxy and the heliosphere

Prof. Igor Moskalenko

11/15/21, 10:40 AM

5. Solar modulation theory and charge-sign dependent modulation.

Prof. Potgieter Marius (Kiel University)

11/15/21, 11:20 AM

7. Discussion

11/15/21, 12:00 PM

11. Time dependent GCR intensity with PAMELA, AMS02 and Neutron Monitor measuraments

Dr Sergey koldobsky (MEPHI)

11/16/21, 2:30 PM

4. Real time monitoring of the radiation environment on the ISS with the AMS-02 detector

Francesco Faldi (Istituto Nazionale di Fisica Nucleare)

11/16/21, 3:15 PM

12. Discussion

11/16/21, 4:00 PM

16. Current Status of the GAPS experiment:

Prof. Chuck Hailey (Columbia University)

11/17/21, 10:30 AM

17. How solar modulation impacts indirect search of dark matter with low energy antinuclei

Mirko Boezio (Istituto Nazionale di Fisica Nucleare)

11/17/21, 11:15 AM

18. Discussion

11/17/21, 12:00 PM

22. Implications of Li to O data of AMS-02 on our understanding cosmic-ray propagation

Dr Michael Korsmaier

11/18/21, 10:30 AM

23. Unified Picture of Galactic CR Transport

Benedikt Schroer (GSSI)

11/18/21, 11:15 AM

24. Discussion

11/18/21, 12:00 PM

6. Contribution 2

Bernd Heber (Christian-Albrechts-Universität zu kiel)

3. Modelling the solar modulation