收藏本站  |  联系我们  |  高能所主站  |  中国科学院  |  English
 
 首 页  理论室概况 科研队伍 学术活动 人才培养 科研成果 访问须知 人才需求 下载专区 HETH-Forum CFHEP
 
  当前位置:首页>学术活动>学术报告  
学术活动  
学术报告
学术会议
理论室青年论坛
学术报告
[4.14]Neutrino flavor oscillations in supernovae and in neutron star mergers
文章来源:  |  发布时间:2016-03-25  |  浏览:

                                    Seminar

Title: Neutrino flavor oscillations in supernovae and in neutron star mergers

Speaker: Dr. Meng-Ru Wu (吴孟儒 (Technische Universität Darmstadt)

Time: 10:00AM, Apr. 14th (Thursday)

Place: Theoretical Physics Division319

Abstract:

Neutrinos play key roles in explosive astrophysical environments such as core-collapse supernovae and mergers of binary neutron stars or a neutron star with a black hole in terms of both transporting the energy and setting up the composition of the system. Neutrino flavor oscillations that alter the flavor content of neutrinos emitted from the central objects maytherefore affect physical processes such as neutrino heating, nucleosynthesis of elements, and the neutrino signals. Due to the non-linear couplings among neutrino themselves, rich phenomena can occur in these environments, such as collective neutrino oscillations in supernovae and matter-neutrino resonances in black-hole accretion disks. I will discuss our recent works in improving the modelling and understanding of neutrino flavor oscillations in both environments, the indications on nucleosynthesis of elements and neutrino signals, and future challenges.

附件
版权所有 © 中国科学院高能物理研究所理论物理研究室 京ICP备05002790号
地址:北京市石景山区玉泉路19号乙院918-4 邮编:100049