A closed-form solution φ(r,θ) for Hill's surfaces in the CR3BP is obtained by solving a cubic equation that reproduces tadpole, horseshoe, Roche lobe, and quasi-spherical shapes.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
UNVERDICTED 2representative citing papers
Introduces a target redshift z_t to isolate metal-poor black hole progenitors and a statistical framework to test merger-rate variations against forecasts from Einstein Telescope and Cosmic Explorer.
citing papers explorer
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Hill's level surfaces in the circular restricted three-body problem solved
A closed-form solution φ(r,θ) for Hill's surfaces in the CR3BP is obtained by solving a cubic equation that reproduces tadpole, horseshoe, Roche lobe, and quasi-spherical shapes.
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Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors
Introduces a target redshift z_t to isolate metal-poor black hole progenitors and a statistical framework to test merger-rate variations against forecasts from Einstein Telescope and Cosmic Explorer.