25–29 Apr 2026
Kechuang Building
Asia/Shanghai timezone

Modeling of Cosmic Ray Escape into Molecular Clouds surrounding Supernova Remnants

27 Apr 2026, 17:20
5m
A102 (Kechuang Building)

A102

Kechuang Building

NO.1520 Taihu Blvd, Suzhou, Jiangsu, China
Poster report(print size: 0.6m Wide*0.9m High) Supernova Remnants session

Speaker

思羽 陈 (西南交通大学)

Description

we describe the numerical framework used to simulate the 3D propagation of CRs from a SNR into a complex molecular environment. Our model couples the time-dependent injection of particles from the SNR shock with a non-linear transport scheme that accounts for CR self-confinement and environmental damping.

Primary authors

思羽 陈 (西南交通大学) 兵 张 四明 刘

Presentation materials