Abstract

Effective-one-body (EOB) theory was originally proposed based on the post-Newtonian (PN) approximation and plays an important role in the analysis of gravitational wave signals. Recently, the post-Minkowskian (PM) approximation has been applied to the EOB theory. The energy map and the effective metric are the two key building blocks of the EOB theory, and in PN approximation radial action variable correspondence is employed to construct the energy map and the effective metric. In this paper, we employ the PM approximation up to the second order, and use the radial action variable correspondence and the precession angle correspondence to construct the energy map and the effective metric. We find that our results based on the radial action variable correspondence, are exactly the same with those obtained based on the precession angle correspondence. Furthermore, we compare the results obtained in this work to the previous existing ones.

Highlights

  • The EOBNR model is a combination of effectiveone-body (EOB) theory and numerical relativity (NR) [9].The EOB theory, which is inspired by the electromagnetically interacting quantum two-body problem [11], has been applied to compute the gravitational waveform emitted by binary black holes [11,12,13,14]

  • The EOB formalism consists of two main parts: the conservative dynamics part and the radiation reaction part

  • The EOB formalism is a successful theory to investigate the gravitational radiation emitted by binary black holes

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Summary

Introduction

The EOBNR model is a combination of effectiveone-body (EOB) theory and numerical relativity (NR) [9]. The EOB theory, which is inspired by the electromagnetically interacting quantum two-body problem [11], has been applied to compute the gravitational waveform emitted by binary black holes [11,12,13,14]. The original EOB theory is based on post-Newtonian (PN) approximation, and the basic idea is to map the real two-body problem to an effective one body problem. The conservative dynamics of a two-body system is described by an effective Hamiltonian. To build the relations between the real two-body system and the effectiveone-body system, the energy map between the real relativistic energy E (in the center of mass frame) and the effective one. Similar to the Bohr–Sommerfeld quantization conditions of bound states in quantum mechanics, the energy map can be obtained by identifying the real radial action variable

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Radial action variable of a two-body system at 2PM order
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Radial action variable of the EOB system at 2PM order
Action variable in the Schwarzschild gauge
Energy map and effective metric at the 2PM order
Energy map and effective metric based on precession angle
Precession angle of real two-body system at 2PM order
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Precession angle of EOB system at the 2PM order
Effective metric at 2PM order based on precession angle
Comparison with existing results
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Comparison to the existing results
Summary and discussion
Findings
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