| 报告题目： |
Modeling the Gravitational wave radiation from neutron star white dwarf binaries |
| 报告人： |
禹升华 |
| 报告人单位： |
中国科学院国家天文台 |
| 报告时间： |
2018年5月22日上午10:30 |
| 报告地点： |
引力中心三楼会议室 |
| 报告摘要： |
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In this talk, I will present a model for the gravitational waves (GW) radiated from neutron star-white dwarf binaries. Using the mili-Hz GW observations made by LISA, we may be able to determine the physical parameters of the binaries with veryshort orbital periods, which have been assumed to be ultracompact X-ray binaries. This model would be useful to understand the entire population of neutron star-white dwarf binaries, and to search for the black hole-white dwarf binaries. |
| 报告人简介： |
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禹升华，2012年7月英国Queen’s University Belfast天体物理博士毕业，2013年1月在中国科学院国家天文台工作至今。主要工作涉及引力波和波源的研究、冷星射电辐射的观测和脉泽不稳定辐射机制等。 |
