Hybrid analytic and machine-learned baryonic property insertion into
galactic dark matter haloes
- URL: http://arxiv.org/abs/2012.05820v1
- Date: Thu, 10 Dec 2020 16:50:33 GMT
- Title: Hybrid analytic and machine-learned baryonic property insertion into
galactic dark matter haloes
- Authors: Ben Moews, Romeel Dav\'e, Sourav Mitra, Sultan Hassan, Weiguang Cui
- Abstract summary: Baryonic properties require complex hydrodynamic simulations that are computationally costly to run.
We merge an extended version of the equilibrium model, an analytic formalism describing the evolution of the stellar, gas, and metal content of galaxies, into a machine learning framework.
We create a high-speed hydrodynamic simulation emulator that populates galactic dark matter haloes in N-body simulations with baryonic properties.
- Score: 1.2599533416395767
- License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
- Abstract: While cosmological dark matter-only simulations relying solely on
gravitational effects are comparably fast to compute, baryonic properties in
simulated galaxies require complex hydrodynamic simulations that are
computationally costly to run. We explore the merging of an extended version of
the equilibrium model, an analytic formalism describing the evolution of the
stellar, gas, and metal content of galaxies, into a machine learning framework.
In doing so, we are able to recover more properties than the analytic formalism
alone can provide, creating a high-speed hydrodynamic simulation emulator that
populates galactic dark matter haloes in N-body simulations with baryonic
properties. While there exists a trade-off between the reached accuracy and the
speed advantage this approach offers, our results outperform an approach using
only machine learning for a subset of baryonic properties. We demonstrate that
this novel hybrid system enables the fast completion of dark matter-only
information by mimicking the properties of a full hydrodynamic suite to a
reasonable degree, and discuss the advantages and disadvantages of hybrid
versus machine learning-only frameworks. In doing so, we offer an acceleration
of commonly deployed simulations in cosmology.
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