University of Birmingham > Talks@bham > Astrophysics Seminars > Accurate gravitational-wave measurements with inaccurate waveform models?

Accurate gravitational-wave measurements with inaccurate waveform models?

Add to your list(s) Download to your calendar using vCal

If you have a question about this talk, please contact Ilya Mandel.

Theoretical models of the gravitational-wave (GW) signals emitted by coalescing compact binaries are a fundamental part of the search strategy employed in the analysis of detector data. Consequently, drawing reliable conclusions from such GW searches highly relies on the existence of accurate waveform predictions.

In this talk I will briefly present how to obtain the GW signal of the inspiral of two black holes, which in turn can be complemented by large-scale numerical simulations of the merger and ringdown phase. Even though these waveforms are the best and most complete description of the expected signal we have today, various studies show that they fail to satisfy desirable (but most stringent) accuracy requirements. Nevertheless, there is potential benefit in combining inspiral and merger waveforms, and the remaining uncertainty can be expressed in terms of physically meaningful quantities such as the detection efficiency and the systematic bias in measuring the source parameters.

This talk is part of the Astrophysics Seminars series.

Tell a friend about this talk:

This talk is included in these lists:

Note that ex-directory lists are not shown.

 

Talks@bham, University of Birmingham. Contact Us | Help and Documentation | Privacy and Publicity.
talks@bham is based on talks.cam from the University of Cambridge.