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Main Authors: Long, Jiang, Yu, Run-Ze
Format: Preprint
Published: 2024
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Online Access:https://arxiv.org/abs/2403.18627
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author Long, Jiang
Yu, Run-Ze
author_facet Long, Jiang
Yu, Run-Ze
contents The helicity flux density is a novel quantity which characterizes the angle-dependence of the helicity of radiative gravitons and it may be tested by gravitational wave experiments in the future. We derive a quadrupole formula for the helicity flux density due to gravitational radiation in the slow motion and the weak field limit. We apply the formula to the bound and unbound orbits in two-body systems and find that the total radiative helicity fluxes are always zero. However, the radiative helicity flux density, which is $\mathcal{O}(G^3)$ in the Newtonian limit, still has non-trivial dependence on the angle. Furthermore, we also find a formula for the total helicity flux by including all contributions of the higher multipoles.
format Preprint
id arxiv_https___arxiv_org_abs_2403_18627
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Gravitational helicity flux density from two-body systems
Long, Jiang
Yu, Run-Ze
General Relativity and Quantum Cosmology
The helicity flux density is a novel quantity which characterizes the angle-dependence of the helicity of radiative gravitons and it may be tested by gravitational wave experiments in the future. We derive a quadrupole formula for the helicity flux density due to gravitational radiation in the slow motion and the weak field limit. We apply the formula to the bound and unbound orbits in two-body systems and find that the total radiative helicity fluxes are always zero. However, the radiative helicity flux density, which is $\mathcal{O}(G^3)$ in the Newtonian limit, still has non-trivial dependence on the angle. Furthermore, we also find a formula for the total helicity flux by including all contributions of the higher multipoles.
title Gravitational helicity flux density from two-body systems
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2403.18627