Astrophysics At z 10 With Gravitational Waves

Details Astrophysics At z 10 With Gravitational Waves Astrophysics At z 10 With Gravitational Waves

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008head...10.0602s&link_type=abstract

American Astronomical Society, HEAD meeting #10, #6.02

Astronomy and Astrophysics

Astrophysics

Scientific paper

What astrophysics can be done at redshifts beyond 5 using gravitational waves? Historically, gravitational wave antennas have been characterized by their detection capability. This is measured in terms of signal-noise ratio, and implies a rate of false positives and false negatives. But to do useful astrophysics, one would like to measure - or more properly, estimate - astrophysical parameters of the gravitational wave sources. In the interest of strengthening the connection between science objectives and a specific instrument performance, the LISA community has reformulated the LISA science requirements around the anticipated uncertainty in astrophysical parameter estimation. The rationale for this characterization of LISA and a summary of the astrophysics that LISA can do will be given.

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