Constraint-satisfying binary boson star initial data via XCFC
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arXiv
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| Main Authors: | , , , , , , |
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| Format: | Preprint |
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2026
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| _version_ | 1866914582400860160 |
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| author | Palloni, Gabriele Sanchis-Gual, Nicolas Font, José A. Santos-Pérez, Samuel Cordero-Carrión, Isabel Cerdá-Durán, Pablo Lazarte, Claudio |
| author_facet | Palloni, Gabriele Sanchis-Gual, Nicolas Font, José A. Santos-Pérez, Samuel Cordero-Carrión, Isabel Cerdá-Durán, Pablo Lazarte, Claudio |
| contents | Numerical-relativity simulations with non-trivial matter configurations require initial data that satisfy the Hamiltonian and momentum constraints of the Einstein equations. We construct constraint-satisfying scalar-field initial data using the eXtended Conformally Flat Condition (XCFC) formalism, in which the matter variables are conformally rescaled and an auxiliary vector field is introduced. In doing so, we overcome the issues of local uniqueness and convergence of the solutions that arise in the second-order elliptic equations associated with the constraints. Using an iterative solver method, we demonstrate the convergence of the XCFC approach to a solution for several scalar-field matter systems. Those include Gaussian-like profiles, topological torus configurations, and equal-mass boson star binaries. In particular, for the latter case, it is common to employ the superposition of two isolated boson star solutions in order to build the initial data. We show that our formalism significantly improves upon a superposition approach by generating genuinely constraint-satisfying initial data for boson star binaries. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2605_20888 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Constraint-satisfying binary boson star initial data via XCFC Palloni, Gabriele Sanchis-Gual, Nicolas Font, José A. Santos-Pérez, Samuel Cordero-Carrión, Isabel Cerdá-Durán, Pablo Lazarte, Claudio General Relativity and Quantum Cosmology Numerical-relativity simulations with non-trivial matter configurations require initial data that satisfy the Hamiltonian and momentum constraints of the Einstein equations. We construct constraint-satisfying scalar-field initial data using the eXtended Conformally Flat Condition (XCFC) formalism, in which the matter variables are conformally rescaled and an auxiliary vector field is introduced. In doing so, we overcome the issues of local uniqueness and convergence of the solutions that arise in the second-order elliptic equations associated with the constraints. Using an iterative solver method, we demonstrate the convergence of the XCFC approach to a solution for several scalar-field matter systems. Those include Gaussian-like profiles, topological torus configurations, and equal-mass boson star binaries. In particular, for the latter case, it is common to employ the superposition of two isolated boson star solutions in order to build the initial data. We show that our formalism significantly improves upon a superposition approach by generating genuinely constraint-satisfying initial data for boson star binaries. |
| title | Constraint-satisfying binary boson star initial data via XCFC |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2605.20888 |