Simulation of the White Dwarf Binary Background for LISA

Details Simulation of the White Dwarf Binary Background for LISA Simulation of the White Dwarf Binary Background for LISA

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aps..apr.k9012b&link_type=abstract

American Physical Society, April Meeting, 2003, April 5-8, 2003 Philadelphia, Pennsylvania, MEETING ID: APR03, abstract #K9.012

Physics

Scientific paper

Gravitational radiation from the galactic population of white dwarf binaries is expected to produce a background signal in the LISA frequency band. At low frequencies (f < 1 mHz) the number of sources will be so large that the background can be treated as gaussian noise, while at high frequencies (f > 10 mHz) the signal consists of separable individual sources. We present a time-domain simulation of the sigal in the intermediate range (1 mHz < f < 10 mHz) from a synthesized population of 9 × 10^4 binaries in the galactic disk. We compare this signal with the simulated signal from binaries in selected globular clusters.

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