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Bowen-York Type Initial Data for Binaries with Neutron Stars

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arxiv 1606.04881 v1 pith:3LLORT37 submitted 2016-06-15 gr-qc astro-ph.CO

Michael Clark , Pablo Laguna This is my paper · ORCID
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keywords neutronbinaryblackdatainitialmethodstarapproach
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A new approach to construct initial data for binary systems with neutron star components is introduced. The approach is a generalization of the puncture initial data method for binary black holes based on Bowen-York solutions to the momentum constraint. As with binary black holes, the method allows setting orbital configurations with direct input from post-Newtonian approximations and involves solving only the Hamiltonian constraint. The effectiveness of the method is demonstrated with evolutions of double neutron star and black hole -- neutron star binaries in quasi-circular orbits.

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  1. Head-on Collisions of Boson Stars with Bowen-York Type Initial Data

    gr-qc 2026-07 accept novelty 5.5 of 10

    Bowen-York-type initial data for boson stars yields head-on collision results consistent with prior work: BBS radiate more GW energy than BBH, while BHBS radiate less.

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