Approach to the separatrix with eccentric orbits
Guillaume Lhost, Geoffrey Compère
SciPost Phys. Core 8, 059 (2025) · published 29 August 2025
- doi: 10.21468/SciPostPhysCore.8.3.059
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Abstract
Eccentric binary compact mergers are prime targets of current and future gravitational wave observatories. In the small mass ratio expansion, post-adiabatic inspirals have been modeled up to the separatrix, where first-principle modeling currently ends. In this paper, we derive the analytic late time solution to the adiabatic inspiral in terms of self-force coefficients at the separatrix. We identify the role of the Lambert $W_{-1}$ function as a key mathematical ingredient in the approach to the separatrix.
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Cited by 1
Authors / Affiliations: mappings to Contributors and Organizations
See all Organizations.- 1 Guillaume Lhost,
- 2 3 Geoffrey Compère
