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This document compares different post-Newtonian (PN) template families for modeling gravitational waveforms from extreme mass ratio inspirals (EMRIs) using LISA. The authors derive TaylorT1, TaylorT2, TaylorT3, TaylorT4 and TaylorEt waveform templates up to 22PN order for a test particle orbiting a Schwarzschild black hole. They find that TaylorT1 and TaylorT2 templates have phase differences less than 10−9 radians from numerical waveforms for mass ratios of 10−4 and 10−5, suggesting these templates will pr

Author

anca irina

Language

EN