LISA sensitivity below 0.1 mHz

Details LISA sensitivity below 0.1 mHz LISA sensitivity below 0.1 mHz

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cqgra..20s.301b&link_type=abstract

Classical and Quantum Gravity, Volume 20, Issue 10, pp. S301-S310 (2003).

Physics

19

Scientific paper

It has been clear for some time that the LISA mission can provide valuable new information concerning galaxy formation and evolution. If galaxies or pre-galactic structures contain massive black holes before their mergers, then these black holes may sink towards the centre of the newly formed structure and form a binary. The conditions under which the black holes will form a close binary that radiates gravitational waves strongly in less than a Hubble time have been discussed in a number of articles. Here, the gravitational wave sensitivity that LISA can achieve in order to look for such signals at frequencies below 0.1 mHz is discussed, and a specific sensitivity goal at frequencies down to 3 μHz is suggested.

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