Analytical effective one-body formalism for extreme-mass-ratio inspirals with eccentric orbits |
Chen Zhang,Wen-Biao Han,Shu-Cheng Yang |
Figure 6. Illustration of orbital evolution with different mass ratios and orbital parameters with 2PN fluxes. The solid line represents evolution with initial parameters of p = 20M, e = 0.6 and the dashed line represents evolution with initial parameters of p = 10M, e = 0.6. The different colors denote different mass ratios. |