High-Energy Astro-Plasma Physics Workshop 2024

Black holes and neutron stars exhibit interesting phenomena through emissions of broad energy range of photons, charged particles, neutrinos, and gravitational waves. For understanding these phenomena, recently more and more attention is being paid to physics of strongly magnetized plasma. We discuss and share ideas to activate theoretical and observational researches.

Program

June 24th Mon., at the seminar room in FRIS (Frontier Research Institute for Interdisciplinary Sciences)

10:30 - 11:30

Shinpei Shibata (Yamagata U) "The relativistic centrifugal acceleration in pulsars"

12:30 - 13:30

Shota Kisaka (Hiroshima U) "Analysis of magnetospheric gaps around Kerr black holes using 2D GRPIC simulations"

(15:00-16:00 Astronomical Institute Colloquium by S. Fujibayashi)

June 25th Tue., at Aoba Science Hall

10:30 - 11:30

Kenji Toma (Tohoku U) "On the BH energy reduction mechanism in the BZ process and a new observational strategy of M87 BH magnetosphere"

13:00 - 14:00

Shuta Tanaka (Aoyama-gakuin U) "A Self-regulated Stochastic Acceleration Model of Pulsar Wind Nebulae"

14:30 - 15:30

W. Zaq (Tohoku U) "Relativistic parametric decay instability of MHD Alfven wave: Discovery of three new decay channels and their properties"

16:00 - 17:00

Tomoki Wada (Tohoku U) "Fireball model for the MeV line emission in GRB 221009A"