Redshift factor and the first law of binary black hole mechanics in numerical simulations

TL;DR

This paper introduces a new method to extract the redshift factor from numerical simulations of binary black holes, confirming its relation to surface gravity and validating the first law of binary black hole mechanics.

Contribution

A novel technique for measuring the redshift factor on apparent horizons in numerical simulations, linking it to surface gravity and the first law of binary black hole mechanics.

Findings

Confirmed the relation between redshift factor and surface gravity.

Validated the first law of binary black hole mechanics in simulations.

Enabled tests of analytic predictions for redshift in approximate circular orbits.

Abstract

The redshift factor $z$ is an invariant quantity of fundamental interest in post-Newtonian and self-force descriptions of compact binaries. It connects different approximation schemes, and plays a central role in the first law of binary black hole mechanics, which links local quantities to asymptotic measures of energy and angular momentum in these systems. Through this law, the redshift factor is conjectured to have a close relation to the surface gravity of the event horizons of black holes in circular orbits. We propose and implement a novel method for extracting the redshift factor on apparent horizons in numerical simulations of quasicircular binary inspirals. Our results confirm the conjectured relationship between $z$ and the surface gravity of the holes and that the first law holds to a remarkable degree for binary inspirals. The redshift factor enables tests of analytic predictions for $z$ in spacetimes where the binary is only approximately circular, giving a new connection between analytic approximations and numerical simulations.