6月6日下午学术报告:非线性光学&引力波与多信使天文学
2017-06-01 20:17   审核人:

 两场学术报告:

 

地点:理学实验楼718报告厅

 

一、66日下午1:30学术报告:意大利DOMENICO PAPARO教授(非线性光学)
报告题目:Nonlinear Optical Spectroscopy of surfaces and interfaces:the case study of the LaAlO3/SrTiO3 interface.
时间:201766日下午1:30 
(
预计1小时报告,半小时交流,下午3:00结束)
Domenico Paparo is a permanent researcher of the Italian National Council for Research (CNR) since 2005. Presently he leads the group of ‘Nonlinear Optical Spectroscopy’ located at the Department of Physics of the University of Naples 'Federico II', where he conducts the major part of his research.
He graduated in Physics on 1996 at the University of Naples 'Federico II' and the following year he was appointed as a post-doc fellow at the University of Technology in Darmstadt (Germany) where he spent one year. 
On 2006 he has been awarded of a Marie Curie fellowship to be trained on Time-Domain THz Spectroscopy at the FOM-Amolf Institute in Amsterdam, where he spent fifteen months.
On 2012 he has got the ‘National Scientific Abilitation’ as Associated Professor in Experimental Condensed Matter Physics.
His research activity is located at the intersection between optics and condensed matter physics. In particular he is an expert in the field of nonlinear optics and ultrafast laser science. His scientific interests include surface science, oxide heterostructures and interfaces, nonlinear optics of surfaces and interfaces, THz time-domain spectroscopy, pump-probe spectroscopy, time-resolved luminescence, soft matter, coherent anti-Stokes Raman spectroscopy, liquid-crystal physics, ionic liquids, singular optics, laser micro and nano structuring.
He is author of more than 60 communications to conferences, more than 60 papers (3 invited chapters of books). His works have got more than 1500 citations.

 

二、引力波与多信使天文学

报告人胡一鸣博士  中山大学天琴引力中心
时间: 66号下午2:50-410
地点理学实验楼718报告厅

 

摘要:
在这个报告中,我将简单回顾第一次引力波事件GW150914的探测历史。LIGO等地面引力波探测正走向常规化,日常化,而多信使天文学由于可以结合引力波与其他不同观测手段,为全方位研究中心天体物理过程将是未来引力波天文学的重要组成部分。我将介绍多信使天文学的发展现状,以及我们提出的一种针对引力波电磁对应体的搜寻工作的优化算法。在引力波定位能力有限、电磁对应体暗弱的双重限制下,我们的算法可以综合各类不确定性,并最大化其探测概率。针对不同口径,不同视场的望远镜,我们同时给出了对引力波事件电磁对应体的最优观测视场数。

报告人简介:
胡一鸣博士毕业于格拉斯哥大学,主要研究方向为引力波天文学和引力波数据处理,主要的研究对象为致密双星并合。在德国马普引力所(阿尔伯特·爱因斯坦研究所)和清华大学任职博士后期间,致力于连续引力波源的数据处理。胡一鸣博士现在在中山大学天琴引力物理研究中心从事引力波天文学相关工作。

 

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