Analytical effective one-body formalism for extreme-mass-ratio inspirals with eccentric orbits
Chen Zhang,Wen-Biao Han,Shu-Cheng Yang
Figure 7. 2PN and 3PN evolutions for different spins with ν = 0.001. The left and right panels show the evolution of eccentricity and semilatus rectum for five inspirals with various spins using the fluxes truncated at the 2PN and 3PN, respectively.