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Physical scales We make use of the empirical relation between the massMof a SMBH, the velocity dispersionσof the stars around it, known asM–σrelation

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astro-ph.GA 1

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2026 1

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Self-acceleration of Hardening Binaries

astro-ph.GA · 2026-05-01 · unverdicted · novelty 7.0

Hardening binaries experience deterministic self-acceleration of their center of mass, induced precession, and plane rotation in uniform isotropic media, driving outward spiraling and eccentricity growth in all cases rather than circularization.

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  • Self-acceleration of Hardening Binaries astro-ph.GA · 2026-05-01 · unverdicted · none · ref 1

    Hardening binaries experience deterministic self-acceleration of their center of mass, induced precession, and plane rotation in uniform isotropic media, driving outward spiraling and eccentricity growth in all cases rather than circularization.