报告讲座

主持人:刘四明 教授

时间:2022年3月23 14:00-18:15

地点:犀浦校区1号教学楼1403

ZOOM会议号:89892292668

会议链接: https://ihep-ac-cn.zoom.us/j/89892292668?

会议密码:123456

 

主讲人:Reinhard Schlickeiser   德国  Ruhr-University Bochum教授

主题:Cosmic rays and MHD turbulence generation in giant molecular clouds

摘要The diffusive propagation of nonrelativistic cosmic ray (CR) protons undergoing energy losses by ionization in a dense homogeneous infinitely extended interstellar molecular cloud (MC) is investigated. The steady-state transport equation for the differential number density of nonrelativistic CR protons is solved with the boundary condition that at the edge of cloud it agrees with the interstellar CR number density. It is shown that giant interstellar MCs with column depths much greater  than about 7 ·1022 cm−2 are an efficient sink of nonrelativistic CRs. At small penetration depths the CRs lose energy by ionizing  and heating the molecular gas, whereas at large penetration depths they are collectively dissipated by the streaming instability, which transfers one-half of the energy density of the incoming interstellar nonrelativistic CRs to Alfvenic magnetic field turbulence.

                 

 

上一条:格物致理第7期:Plasma fluctuations in the intergalactic medium 下一条:以项目为导向课程-高能天体物理 The Theory of Cosmic Ray Acceleration and Transport I by Reinhard Schlickeis​er

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