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A Possible Mass Distribution of Primordial Black Holes Implied by LIGO-Virgo

06/01 2021 Seminar
  • Title A Possible Mass Distribution of Primordial Black Holes Implied by LIGO-Virgo
  • Speaker 邓鹤凌
  • Date 10:00 am, Tuesday, June 1st, 2021 (Beijing Time)
  • Venue Online Zoom meeting: 954 8794 0061
  • Abstract

    CAS Key Laboratory of Theoretical Physics

    Institute of Theoretical Physics

    Chinese Academy of Sciences

     Seminar

    Title

    题目

    A Possible Mass Distribution of Primordial Black Holes Implied by LIGO-Virgo

    Speaker

    报告人

    邓鹤凌

    Affiliation

    所在单位

    亚利桑那州立大学

    Date

    日期

    10:00 am, Tuesday, June 1st, 2021 (Beijing Time)

    Venue

    地点

    Online Zoom meeting: 954 8794 0061

    Contact Person

    所内联系人

    王少江 Shao-Jiang Wang

    Abstract

    摘要

    The LIGO-Virgo Collaboration has so far detected around 90 black holes, whose mass distribution appears to have a peak at ~ 30M☉ and two tails on the ends. By assuming that they all have a primordial origin, we analyze the GWTC-1 (O1&O2) and GWTC-2 (O3a) datasets by performing maximum likelihood estimation on a broken power-law mass function, which appears to behave better than the popular log-normal mass function. Surprisingly, such a simple distribution can be realized in our previously proposed mechanism of PBH formation, where the black holes are formed by vacuum bubbles that nucleate during inflation via quantum tunneling.