Relativistic Corrections to the Formation Rate of Extreme Mass-Ratio Inspirals
Chen Feng, Yong Tang

TL;DR
This paper develops a relativistic analytic model for estimating EMRI event rates, revealing that relativistic effects significantly increase predicted rates, especially for shallow stellar profiles, which is crucial for gravitational-wave detection planning.
Contribution
It introduces a relativistically self-consistent framework for EMRI rate estimation, extending the loss-cone theory to include general relativistic effects in Schwarzschild spacetime.
Findings
Relativistic effects increase EMRI rate predictions by about a factor of 8.
The rate enhancement is more significant for shallower stellar density profiles.
The predicted rates are insensitive to the mass of the central black hole.
Abstract
Extreme mass-ratio inspirals (EMRIs) are long-duration gravitational-wave sources in which a compact object gradually spirals into a massive black hole. Their formation is governed by the interplay between stochastic angular-momentum diffusion driven by two-body relaxation and the dissipative evolution caused by gravitational-wave emission, with the loss-cone boundary deciding whether an object undergoes an inspiral or a direct plunge. Building on this physical picture, we construct a relativistically self-consistent analytic framework for estimating EMRI event rates. In Schwarzschild spacetime, we generalize the standard loss-cone angular momentum to an energy-dependent quantity and revise the plunge pericenter by using the minimum stable radius derived from general relativity. Relative to the Newtonian treatment, we show that incorporating these relativistic effects increases the…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Relativity and Gravitational Theory
