The universal acceleration scale from stellar feedback
Michael Y. Grudi\'c, Michael Boylan-Kolchin, Claude-Andr\'e, Faucher-Gigu\`ere, and Philip F. Hopkins

TL;DR
This paper proposes that the universal acceleration scale observed in galaxy rotation curves arises from stellar feedback processes, linking it to fundamental constants and explaining the transition to baryon dominance.
Contribution
It introduces a model where the characteristic acceleration scale is derived from stellar feedback, connecting galaxy dynamics to fundamental physical constants.
Findings
The observed acceleration scale $g_\dagger$ matches the feedback-regulated star formation threshold.
The model explains the flat rotation curves and the $g_{\rm obs} \sim (g_{\rm baryon} g_{\dagger})^{1/2}$ scaling.
The acceleration scale can be expressed as $g_{\dagger} \sim 0.1 G m_p / \sigma_T$, linking it to fundamental constants.
Abstract
It has been established for decades that rotation curves deviate from the Newtonian gravity expectation given baryons alone below a characteristic acceleration scale , a scale promoted to a new fundamental constant in MOND. In recent years, theoretical and observational studies have shown that the star formation efficiency (SFE) of dense gas scales with surface density, SFE with (where is the momentum flux output by stellar feedback per unit stellar mass in a young stellar population). We argue that the SFE, more generally, should scale with the local gravitational acceleration, i.e. that SFE $\sim g_{\rm tot}g_\mathrm{crit} \equiv (G\,M_{\rm tot}/R^{2}) /…
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