Neural Infalling Cloud Equations (NICE): Increasing the Efficacy of Subgrid Models and Scientific Equation Discovery using Neural ODEs and Symbolic Regression
arXiv:2408.10387 · doi:10.1093/mnras/staf217
Abstract
Galactic systems are inherently multiphase, and understanding the roles and interactions of the various phases is key towards a more complete picture of galaxy formation and evolution. For instance, these interactions play a pivotal role in the cycling of baryons which fuels star formation. The transport and dynamics of cold clouds in their surrounding hot environment are governed by complex small scale processes (such as the interplay of turbulence and radiative cooling) that determine how the phases exchange mass, momentum and energy. Large scale models thus require subgrid prescriptions in the form of models validated on small scale simulations, which often take the form of coupled differential equations. In this work, we explore using neural ordinary differential equations which embed neural networks as terms in the model to capture an uncertain physical process. We then apply Symbolic Regression to potentially discover new insights into the physics of cloud-environment interactions. We test this on both generated mock data and actual simulation data. We also extend the neural ODE to include a secondary neural term. We show that neural ODEs in tandem with Symbolic Regression can be used to enhance the accuracy and efficiency of subgrid models, and/or discover the underlying equations to improve generality and scientific understanding. We highlight the potential of this scientific machine learning approach as a natural extension to the traditional modelling paradigm, both for the development of semi-analytic models and for physically interpretable equation discovery in complex non-linear systems.
13 Pages, 8 Figures, Accepted for publication in MNRAS
References in corpus (56)
- The NumPy array: a structure for efficient numerical computation
- Machine Learning for Fluid Mechanics
- How Do Galaxies Get Their Gas?
- Galaxy Bimodality due to Cold Flows and Shock Heating
- Galactic Winds
- The Structure and Kinematics of the Circum-Galactic Medium from Far-UV Spectra of z~2-3 Galaxies
- The Athena++ Adaptive Mesh Refinement Framework: Design and Magnetohydrodynamic Solvers
- Gaseous Galaxy Halos
- Multi-Phase Galaxy Formation: High Velocity Clouds and the Missing Baryon Problem
- Evidence for Ubiquitous Collimated Galactic-Scale Outflows along the Star-Forming Sequence at z~0.5
- Time-Dependent Ionization in Radiatively Cooling Gas
- Toward a Unification of Star Formation Rate Determinations in the Milky Way and Other Galaxies
- The growth and entrainment of cold gas in a hot wind
- Accretion of gas onto nearby spiral galaxies
- Magnetized Gas Clouds can Survive Acceleration by a Hot Wind
- The Launching of Cold Clouds by Galaxy Outflows I: Hydrodynamic Interactions with Radiative Cooling
- Interpretable Machine Learning for Science with PySR and SymbolicRegression.jl
- Resolving small-scale cold circumgalactic gas in TNG50
- Starburst-Driven Galactic Winds: Filament Formation and Emission Processes
- A Model for Star Formation, Gas Flows and Chemical Evolution in Galaxies at High Redshifts
- How cold gas continuously entrains mass and momentum from a hot wind
- Multiphase Gas and the Fractal Nature of Radiative Turbulent Mixing Layers
- The Physical Nature of Starburst-Driven Galactic Outflows
- The Fate of High-Velocity Clouds: Warm or Cold Cosmic Rain?
- The Disruption and Fueling of M33
- Interaction of a cold cloud with a hot wind: the regimes of cloud growth and destruction and the impact of magnetic fields
- An Exact Integration Scheme for Radiative Cooling in Hydrodynamical Simulations
- On Neural Differential Equations
- On the Survival of Cool Clouds in the Circum-Galactic Medium
- Entrainment in Trouble: Cool Cloud Acceleration and Destruction in Hot Supernova-Driven Galactic Winds
- Radiative Mixing Layers: Insights from Turbulent Combustion
- High Velocity Rain: The Terminal Velocity of Model of Galactic Infall
- Universal Differential Equations for Scientific Machine Learning
- The impact of magnetic fields on thermal instability
- The origin of the high-velocity cloud complex C
- Is Multiphase Gas Cloudy or Misty?
- Linked evolution of gas and star formation in galaxies over cosmic history
- A simple model for mixing and cooling in cloud-wind interactions
- The Mass Inflow and Outflow Rates of the Milky Way
- Cloudy with A Chance of Rain: Accretion Braking of Cold Clouds
- Cosmic-Ray Transport in Varying Galactic Environments
- The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- II: Cold, Dense Gas Clouds and High-Velocity Cloud Analogs
- Arkenstone I: A Novel Method for Robustly Capturing High Specific Energy Outflows In Cosmological Simulations
- The in situ formation of molecular and warm ionised gas triggered by hot outflows
- Radiative turbulent mixing layers at high Mach numbers
- Boosting galactic outflows with enhanced resolution
- CR Driven Multi-phase Gas Formed via Thermal Instability
- Cooling driven coagulation
- Mass, Morphing, Metallicities: The Evolution of Infalling High Velocity Clouds
- Physical effects on compact high-velocity clouds in the circumgalactic medium
- Using physics-informed neural networks to compute quasinormal modes
- Neural networks: solving the chemistry of the interstellar medium
- The role of the halo magnetic field on accretion through High-Velocity Clouds
- Climate Modeling with Neural Diffusion Equations
- Neural Astrophysical Wind Models
- Neural ODEs as a discovery tool to characterize the structure of the hot galactic wind of M82