Dark Sage: Next-generation semi-analytic galaxy evolution with multidimensional structure and minimal free parameters
Adam R. H. Stevens, Manodeep Sinha, Alexander Rohl, Mawson W. Sammons,, Boryana Hadzhiyska, C\'esar Hern\'andez-Aguayo, Lars Hernquist

TL;DR
Dark Sage is an advanced semi-analytic galaxy formation model that incorporates detailed structural and evolutionary features of galaxies with minimal free parameters, calibrated against key observational data.
Contribution
It introduces a new stellar feedback treatment, detailed disc heating and age distribution tracking, and achieves high complexity with only three free parameters.
Findings
Predicts radial and vertical disc structures.
Tracks stellar age, metallicity, and velocity dispersion per annulus.
Calibrated with cosmic star formation history and mass functions.
Abstract
After more than five years of development, we present a new version of Dark Sage, a semi-analytic model (SAM) of galaxy formation that breaks the mould for models of its kind. Included among the major changes is an overhauled treatment of stellar feedback that is derived from energy conservation, operates on local scales, affects gas gradually over time rather than instantaneously, and predicts a mass-loading factor for every galaxy. Building on the model's resolved angular-momentum structure of galaxies, we now consider the heating of stellar discs, delivering predictions for disc structure both radially and vertically. We add a further dimension to stellar discs by tracking the distribution of stellar ages in each annulus. Each annulus--age bin has its own velocity dispersion and metallicity evolved in the model. This allows Dark Sage to make structural predictions for galaxies that…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies
