摘要： With the development of multi-messenger astronomy and the detection of astrophysical neutrinos, we are in a golden age of new cosmic ray (CR) measurements and studies. Supernova remnants are believed as the leading candidate for the source of Galactic CRs. Recent observations, however, challenge the well-developed theory of diffusive shock acceleration of CRs in supernova remnants. I will reexamine the assumptions in the standard shock acceleration model and discuss the key missing physics for shocks propagating in the turbulent and inhomogeneous interstellar medium. A more realistic shock acceleration model holds the promise to understand the observational puzzles and the origin of Galactic CRs.
报告人简介：徐思遥，2011年山东大学物理与微电子专业本科，2017年北京大学天体物理专业博士，2017-2020，美国威斯康星大学NASA Hubble Fellow，2020年至今，美国普林斯顿高等研究院NASA Hubble Fellow。研究方向是磁流体湍流物理的天文应用。