Analytical effective one-body formalism for extreme-mass-ratio inspirals with eccentric orbits |
Chen Zhang,Wen-Biao Han,Shu-Cheng Yang |
Figure 8. Performances of different PN-order fluxes. The figure shows inspirals with initial parameters of p = 20M, e = 0.6, ν = 0.001, and spin a = 0.99M using fluxes truncated at the 2PN, 2.5PN, 3PN, 3.5PN and 4PN. |