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2016年10月28日 英国伯明翰大学缪海兴博士学术报告

发布时间:2016-10-27          来源:办公室           浏览次数:

报告人

缪海兴

单位

Astrophysics and  Space Research Group School of Physics and Astronomy, University of  Birmingham

报告时间

20161028

下午3:40

报告地点

引力中心3楼会议室

报告题目

The Beginning of Gravitational Wave Astronomy

报告内容摘要

For the first  part of this talk, I will give a brief overview of the recent LIGO  discoveries: GW150914 and GW151226—gravitational wave signals from binary  black hole coalescences. The focus is on the instruments and techniques that  enable these discoveries, and also on the science that we have learned. For  the second part, I will talk about   both near-term and long-term future of ground-based gravitational-wave  detectors, particular on the main sources of noise that limit the detector  sensitivity and how we reduce the noise to allow for exciting  gravitational-wave astronomy.

报告人简介

Haixing Miao

Education:

Sep. 2010: Ph.D.in Physics, University of Western Australia  (UWA),

Jun. 2006: B.A. in Astrophysics, University of Science and  Technology of China

Employments:

Mar. 2016 – Present Birmingham  Fellow & STFC Ernest Rutherford Fellow Astrophysics and Space Research  (ASR) Group & UK National Quantum Hub University of Birmingham (UoB)

Mar. 2014 – Feb. 2016Marie-Curie  International Incoming Fellow Astrophysics and Space Research Group, UoB

Nov. 2013 – Oct. 2010: Postdoctoral scholar 1. Theoretical  AstroPhysics Including Relativity and Cosmology (TAPIR); 2. Laser  Interferometer Gravitational-wave Observatory (LIGO) Laboratory; 3. Institute  for Quantum Information and Matter (IQIM), Caltech

上一篇:2016年11月2日 德国斯图加特大学Sneeuw教授学术报告
下一篇:2016年10月20日 华中科技大学马修泉教授学术报告
 
 
 

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