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Inspirals of stellar mass compact objects into massive black holes are an important source for future gravitational wave detectors such as Advanced LIGO and LISA.
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Phys. Rev. D 76
P. A. Sundararajan, G. Khanna, and S. A. Hughes, “Towards adiabatic waveforms for inspiral into Kerr black holes: A new model of the source for the time domain perturbation equation”, · 2007
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Phys. Rev. D76
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Phys. Rev. D 77
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Phys. Rev. D77
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S. Drasco and N. Sago, 2008, · 2008
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Phys. Rev. D77
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Phys. Rev. D77
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in preparation (2008)
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in preparation (2008)
E. E. Flanagan and T. Hinderer, “Two timescale analysis of extreme mass ratio inspirals in Kerr. II. Transient Resonances”, · 2008
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in preparation (2008)
E. E. Flanagan and T. Hinderer, “Two timescale analysis of extreme mass ratio inspirals in Kerr. III. Wave generation”, · 2008
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presentation at the 11th Eastern Gravity Meeting, Penn State, May 2008
C. R. Galley, 2008, · 2008
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Phys. Rev. D77
A. Pound and E. Poisson, “Osculating orbits in Schwarzschild spacetime, with an application to extreme mass-ratio inspirals”, · 2008
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