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Parameter matching between horizon quasi-local and point-particle definitions at 1PN for quasi-circular and non spinning BBH systems in harmonic gauge

Dongze Sun, Leo C. Stein

TL;DR

This work addresses how PN and NR define BBH masses differently at finite separations by constructing a gauge-consistent mapping in harmonic gauge between PN point-particle masses and NR AH-based quasi-local masses. Using matched asymptotic expansions, the authors build a global harmonic BBH metric and derive a harmonic-coordinate transformation that aligns the inner-zone BH metric with the PN near-zone to leading $1\text{PN}$ order. They locate the AH on horizon-penetrating slices to show the AH mass equals the PN mass at $1\text{PN}$, and they quantify how generic harmonic slicings introduce a $1\text{PN}$-level correction, $m_1^{\text{AH}}=m_1\left(1-\tfrac{1}{4}\delta v^2\right)$. The results provide a practical bridge for PN–NR waveform hybrids and NR initial-data construction, with clear paths to include spins, eccentricity, and other NR gauges in future work.

Abstract

We investigate how commonly used parameter definitions in Post-Newtonian (PN) theory compare with those from Numerical Relativity (NR) for binary black hole (BBH) systems. In NR, masses and spins of each companion are measured quasi-locally from apparent horizon geometry, whereas in PN they are attributes of point particles defined via asymptotic matching in body zones. Although these definitions coincide in the infinite-separation limit, they could differ by finite-separation corrections that matter for precision modeling. Working entirely in harmonic gauge, we perform asymptotic matching between each companion's inner zone metric -- obtained from black hole perturbation theory -- and the PN two-body metric, and construct the coordinate transformation that preserves the gauge in the strong field region. We solve perturbatively for the apparent horizon (AH) on a group of harmonic inertial time slice and compute its quasi-local areal mass from the horizon geometry. Then we establish the leading order matching between quasi-local (AH based) and PN (point-particle) parameter definitions in harmonic gauge. We find that on a horizon penetrating harmonic slicing, the AH quasi-local mass agrees with the PN point-particle mass at 1PN order. For generic harmonic slicings that deviate from the horizon penetrating condition by a 1PN order perturbation, the AH mass differs from the PN mass also by a 1PN correction. This parameter matching is crucial for hybridizing PN and NR waveforms and for providing better initial conditions in NR and Cauchy-Characteristic Evolution (CCE) simulations. The framework provides a bridge between different descriptions of BBH systems, and it can be extended to spinning and eccentric cases and more general NR gauges.

Parameter matching between horizon quasi-local and point-particle definitions at 1PN for quasi-circular and non spinning BBH systems in harmonic gauge

TL;DR

This work addresses how PN and NR define BBH masses differently at finite separations by constructing a gauge-consistent mapping in harmonic gauge between PN point-particle masses and NR AH-based quasi-local masses. Using matched asymptotic expansions, the authors build a global harmonic BBH metric and derive a harmonic-coordinate transformation that aligns the inner-zone BH metric with the PN near-zone to leading order. They locate the AH on horizon-penetrating slices to show the AH mass equals the PN mass at , and they quantify how generic harmonic slicings introduce a -level correction, . The results provide a practical bridge for PN–NR waveform hybrids and NR initial-data construction, with clear paths to include spins, eccentricity, and other NR gauges in future work.

Abstract

We investigate how commonly used parameter definitions in Post-Newtonian (PN) theory compare with those from Numerical Relativity (NR) for binary black hole (BBH) systems. In NR, masses and spins of each companion are measured quasi-locally from apparent horizon geometry, whereas in PN they are attributes of point particles defined via asymptotic matching in body zones. Although these definitions coincide in the infinite-separation limit, they could differ by finite-separation corrections that matter for precision modeling. Working entirely in harmonic gauge, we perform asymptotic matching between each companion's inner zone metric -- obtained from black hole perturbation theory -- and the PN two-body metric, and construct the coordinate transformation that preserves the gauge in the strong field region. We solve perturbatively for the apparent horizon (AH) on a group of harmonic inertial time slice and compute its quasi-local areal mass from the horizon geometry. Then we establish the leading order matching between quasi-local (AH based) and PN (point-particle) parameter definitions in harmonic gauge. We find that on a horizon penetrating harmonic slicing, the AH quasi-local mass agrees with the PN point-particle mass at 1PN order. For generic harmonic slicings that deviate from the horizon penetrating condition by a 1PN order perturbation, the AH mass differs from the PN mass also by a 1PN correction. This parameter matching is crucial for hybridizing PN and NR waveforms and for providing better initial conditions in NR and Cauchy-Characteristic Evolution (CCE) simulations. The framework provides a bridge between different descriptions of BBH systems, and it can be extended to spinning and eccentric cases and more general NR gauges.

Paper Structure

This paper contains 15 sections, 59 equations, 1 figure.

Figures (1)

  • Figure 1: A schematic diagram showing the domain setup and symbols.