Stochastic Evolution of Galactic Star Formation with Halo Coupling, AGN Quenching and Hopf Bifurcation Dynamics
Sanjeev Kumar, A.K. Awasthi, Mahesh Kumar

TL;DR
This paper introduces a stochastic nonlinear oscillator model for galactic evolution, capturing star formation bursts, AGN quenching, and morphological features through bifurcation dynamics and noise effects.
Contribution
It develops a novel computational framework using stochastic bifurcation theory and noise modeling to simulate complex galactic behaviors and morphologies.
Findings
Noise broadens bifurcation regimes, inducing starburst bursts.
Galactic Heartbeat as a deterministic limit cycle observed in star formation spectra.
Model reproduces spiral structures and quenching phenomena through spatially varying bifurcation fields.
Abstract
We present a computational framework for galactic evolution based on a coupled stochastic nonlinear oscillator, implemented with the \textbf{Stochastic Hopf Engine}. Gas density () and star formation rate () co-evolve through a supercritical Hopf bifurcation, capturing the transition from quiescent stability to merger-driven starbursts. Scatter in dark matter halo properties, modeled as multiplicative noise via the \textbf{Euler--Maruyama method}, broadens the bifurcation into a regime where noise-induced bursts occur below the deterministic threshold. Simulations reveal a periodic signature, the \textbf{Galactic Heartbeat}, emerging as a deterministic limit cycle validated by the \textbf{data3} resonance peak in the star-formation spectrum. A radial reduction yields an effective \textbf{Fokker--Planck equation} for burst amplitude; its stationary solution matches numerical…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Statistical Mechanics and Entropy
