2022
DOI: 10.1093/mnras/stac3494
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Performance of different correction maps in the extended phase-space method for spinning compact binaries

Abstract: Since the first detection of gravitational waves by the LIGO/VIRGO team, the related research field has attracted more attention. The spinning compact binaries system, as one of the gravitational-wave sources for broadband laser interferometers, has been widely studied by related researchers. In order to analyze the gravitational wave signals using matched filtering techniques, reliable numerical algorithms are needed. Spinning compact binaries systems in Post-Newtonian (PN) celestial mechanics have an insepar… Show more

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Cited by 4 publications
(10 citation statements)
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“…These applications were successful in several examples, but not in chaotic orbits. However, our previous work [Luo et al(2021), Luo et al(2022)] proposed the manifold corrections map, which effectively overcame the challenge. Unlike that in the original paper [Luo et al(2021), Luo et al(2022)], the correction map for the 1PN Hamiltonian is…”
Section: Phase-space Expansion Methods With a Multi-factors Correctio...mentioning
confidence: 99%
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“…These applications were successful in several examples, but not in chaotic orbits. However, our previous work [Luo et al(2021), Luo et al(2022)] proposed the manifold corrections map, which effectively overcame the challenge. Unlike that in the original paper [Luo et al(2021), Luo et al(2022)], the correction map for the 1PN Hamiltonian is…”
Section: Phase-space Expansion Methods With a Multi-factors Correctio...mentioning
confidence: 99%
“…Midpoint and correction maps [Luo et al(2017), Luo et al(2021)] have been proposed to ensure the equivalence of the original variables and the copy one. Recently, we proposed a multi-factor correction map that yields a higher accuracy of the phase-space expansion method without significant computational resource increases [Luo et al(2022)]. This paper aims to design a multi-factor correction map for post-Newton Hamiltonian and examine its performance.…”
Section: Introductionmentioning
confidence: 99%
“…Now we list all the numerical methods used in the numerical experiments for comparison. 2ndKSYM-mp: the second order K-symplectic-like method with the midpoint permutation which is the method S 2 ˜defined in equation (32) or (37). 2ndKSYM-perm: the second order K-symplectic-like method with another permutation which is the method S 2 ˆdefined in equation (39) or (41).…”
Section: Methodsmentioning
confidence: 99%
“…These could be the reasons for the method's good performance in astrophysical applications [30]. Recently, the permutations of the extended phase space explicit symplectic-like methods have been further explored [31,32]. Numerical experiments demonstrate that for the cases of circular restricted three-body system or chaotic orbits of spinning compact binary, the midpoint permutation causes the secular energy drift [31].…”
Section: Introductionmentioning
confidence: 99%
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