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博学堂讲座
From numerical relativity to gravitational wave model (第195讲)
浏览量:1300    发布时间:2016-10-16 14:07:03

报告题目:From numerical relativity to gravitational wave model

报告人:曹周键博士

报告时间:下午2:00-3:00

报告地点:理A110

报告题目:From numerical relativity to gravitational wave model
报告人:中国科学院数学与系统科学研究院  曹周键博士
报告地点:浙江工业大学屏峰校区理A110
报告时间:2016年1021日,下午2:00-300

报告摘要:Gravitational wave is among the most important theoretical predictions of general relativity. It has been directly detected very recently by LIGO successfully. Besides the advanced techniques involved in the experiment instruments, the theoretical model also played an important role in such a success. General speaking, a good model may increase the detection ability more than 100 times for a given hardware. In order to treat the real objects in the universe which does not admit any symmetry and includes many complex physics, numerical method is the only practical method currently. For Einstein equation, even the numerical method is highly non-trival. A bundle of tricks are needed to model the gravitational wave sources. Besides the tricks, a huge computer software is needed to treat the massive computational cost problem. Besides general relativity, almost all existing gravity theories predict the existence of gravitational wave. In the near future, it is possible to use gravitational wave detection to test different gravitational theories if proper model is available. This talk will discuss these related problems in general.

报告人简介:曹周键,中国科学院数学与系统科学研究院副研究员。2006年北京师范大学博士毕业后致力于数值相对论和引力波物理的理论研究。在数值相对论方面,与合作者一起发展了Z4c数值相对论计算方程形式,为高自旋双黑洞发展了高精度计算方法,开发出数值相对论软件AMSS-NCKU。在引力波理论方面,发展了BS理论框架到带宇宙学常数的爱因斯坦方程,建立了双黑洞系统的若干引力波理论模型。

欢迎感兴趣的老师同学参加!
博学堂讲座
From numerical relativity to gravitational wave model (第195讲)
浏览量:1300    发布时间:2016-10-16 14:07:03

报告题目:From numerical relativity to gravitational wave model

报告人:曹周键博士

报告时间:下午2:00-3:00

报告地点:理A110

报告题目:From numerical relativity to gravitational wave model
报告人:中国科学院数学与系统科学研究院  曹周键博士
报告地点:浙江工业大学屏峰校区理A110
报告时间:2016年1021日,下午2:00-300

报告摘要:Gravitational wave is among the most important theoretical predictions of general relativity. It has been directly detected very recently by LIGO successfully. Besides the advanced techniques involved in the experiment instruments, the theoretical model also played an important role in such a success. General speaking, a good model may increase the detection ability more than 100 times for a given hardware. In order to treat the real objects in the universe which does not admit any symmetry and includes many complex physics, numerical method is the only practical method currently. For Einstein equation, even the numerical method is highly non-trival. A bundle of tricks are needed to model the gravitational wave sources. Besides the tricks, a huge computer software is needed to treat the massive computational cost problem. Besides general relativity, almost all existing gravity theories predict the existence of gravitational wave. In the near future, it is possible to use gravitational wave detection to test different gravitational theories if proper model is available. This talk will discuss these related problems in general.

报告人简介:曹周键,中国科学院数学与系统科学研究院副研究员。2006年北京师范大学博士毕业后致力于数值相对论和引力波物理的理论研究。在数值相对论方面,与合作者一起发展了Z4c数值相对论计算方程形式,为高自旋双黑洞发展了高精度计算方法,开发出数值相对论软件AMSS-NCKU。在引力波理论方面,发展了BS理论框架到带宇宙学常数的爱因斯坦方程,建立了双黑洞系统的若干引力波理论模型。

欢迎感兴趣的老师同学参加!