Formalizing Galaxy Population Evolution: Drift and Mergers as Transport Processes on Manifolds
Tsutomu T. Takeuchi (Nagoya University, Institute of Statistical Mathematics)

TL;DR
This paper introduces a unified mathematical framework modeling galaxy evolution as measure transport on manifolds, linking observational data to underlying physical dynamics and generalizing existing models.
Contribution
It formalizes galaxy evolution as measure dynamics on manifolds, connecting observational statistics with underlying physical processes and unifying various models.
Findings
Reinterprets galaxy evolution as measure transport on manifolds.
Shows observational functions are projections of underlying dynamics.
Connects existing models like continuity equations and coagulation as special cases.
Abstract
Galaxy evolution is commonly described through the time evolution of observational statistics such as luminosity functions and stellar mass functions. However, these quantities are projections of an underlying multivariate galaxy state space rather than fundamental dynamical variables. We develop a unified framework in which galaxy evolution is formulated as the time evolution of a probability measure on the galaxy manifold. Representing galaxy states by latent variables and the population by a density , the evolution is governed by a general equation containing continuous transport and nonlocal jump processes. By reinterpreting manifold learning as the pushforward of measures, we distinguish observational, representation, and physical measures, and emphasize that manifold coordinates themselves need not carry direct physical meaning. In this…
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