曼哈顿娱乐城_曼哈顿娱乐场,官网,官方网站,官方网址

<dfn id="xzvfx"><address id="xzvfx"><progress id="xzvfx"></progress></address></dfn>

    <font id="xzvfx"></font>

    <big id="xzvfx"></big>

    <cite id="xzvfx"></cite>
    <mark id="xzvfx"><th id="xzvfx"><b id="xzvfx"></b></th></mark>

           
       
        您现在的位置:首页 > 新闻动态 > 学术活动
       
      【4.11】Stochastic Background of Gravitational Waves
      2019-04-11|文章来源: |【
       

        高能所理论物理室学术活动

        Title: Stochastic Background of Gravitational Waves

        Speaker: Dr. Shi Pi (Kavli, IPMU )

        Time: 3:00PM, April 11th, 2019 (Thursday)

        Place: Library Building 319

        Abstract: The discovery of gravitational waves from the coalescence of binary black holes in 2015 has marked the dawn of the gravitational waves astronomy/cosmology. Besides the gravitational wave bursts from black hole/neutron star mergers, our universe is fulfilled by stochastic background of gravitational waves with a large range of frequencies, which may have various astrophysical/cosmological origins in the early universe, for instance incoherent superposition of binary systems, first order phase transitions, reheating after inflation, topological defects, and primordial gravitational waves. As our universe is transparent to gravitational wave, it is a fossil recording the information of its generation and how our universe evolves. In this talk I will briefly review the stochastic background of the gravitational waves (GWs), especially the secondary gravitational waves induced by scalar perturbations, and discuss their connection to the primordial black holes which may be candidates for dark matter or the seeds for galaxy formation.

       


       
      中国科学院高能物理研究所    备案序号:京ICP备05002790-1号    文保网安备案号:110402500050
      地址:北京市918信箱    邮编:100049    电话:86-10-88235008    Email:ihep@ihep.ac.cn

      Sitemap

      AG百家乐官方网址| 葡京_澳门葡京官网| 皇冠体育|官网| HB电子平台|HB电子游戏| 靠谱重庆时时彩平台|