Low Frequency Astrophysical Gravitational Wave Background

Details Low Frequency Astrophysical Gravitational Wave Background Low Frequency Astrophysical Gravitational Wave Background

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..686..231p&link_type=abstract

THE ASTROPHYSICS OF GRAVITATIONAL WAVE SOURCES. AIP Conference Proceedings, Volume 686, pp. 231-234 (2003).

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Gravitational Radiation, Magnetic Fields, And Other Observations, Radiation Mechanisms, Polarization, Galaxy Mergers, Collisions, And Tidal Interactions, Gravitational Radiation Detectors, Mass Spectrometers, And Other Instrumentation And Techniques

Scientific paper

Three simplified merger tree models for galaxy formation have been explored by Menou and collaborators [1, 2]. We have used these merger trees for a very preliminary investigation of what range of gravitational wave background levels at low frequencies might be expected from massive black hole binary coalescences after mergers of galaxies or pre-galactic structures. We find that the background produced probably does not substantially affect the LISA sensitivity at low frequencies, provided that mergers at z > 5 do not have a strong effect.

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