Analytical effective one-body formalism for extreme-mass-ratio inspirals with eccentric orbits
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Analytical effective one-body formalism for extreme-mass-ratio inspirals with eccentric orbits |
| Chen Zhang,Wen-Biao Han,Shu-Cheng Yang |
| Figure 4. The frequency shifts Δωrνωr0 and Δωϕνωϕ0 versus the Kerr parameter a for various p, e with ν = 10−4. When a becomes smaller, the frequency shift can become larger, since the orbit approaches the ISBO. |
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