Generalized linear matrix method computes normal modes in stellar disks with sharp L=0 edges via boundary integrals, validated to ~0.003 accuracy on Kuzmin-Toomre models against an independent nonlinear method.
year = 1963, month = aug, volume =
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2026 2representative citing papers
Bayesian comparison of Gaia DR3 rotation curves favors the Einasto dark matter profile over NFW, prefers cored over cuspy profiles, and finds MOND variants provide poorer fits than the best dark matter models.
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A generalized linear matrix method for normal modes in collisionless stellar disks
Generalized linear matrix method computes normal modes in stellar disks with sharp L=0 edges via boundary integrals, validated to ~0.003 accuracy on Kuzmin-Toomre models against an independent nonlinear method.
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Determination of the best dark matter profile for the Milky Way with Gaia DR3 using Bayesian Model Comparison
Bayesian comparison of Gaia DR3 rotation curves favors the Einasto dark matter profile over NFW, prefers cored over cuspy profiles, and finds MOND variants provide poorer fits than the best dark matter models.