Improved modelling of gravitational waves from LMXBs

Details Improved modelling of gravitational waves from LMXBs Improved modelling of gravitational waves from LMXBs

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004head....8.1903w&link_type=abstract

American Astronomical Society, HEAD meeting #8, #19.03; Bulletin of the American Astronomical Society, Vol. 36, p.944

Astronomy and Astrophysics

Astronomy

Scientific paper

Accreting neutron stars in LMXBs are potentially promising sources of gravitational radiation. We discuss the modelling of these systems, including key issues concerning variability of the accretion spin-up torque. The associated variability in the signal from various gravitational-wave mechanisms (accretion induced asymmetries, toroidal magnetic fields or unstable r-modes) is considered, and we assess the detectability of these sources.

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