A Halo Merger Tree Generation and Evaluation Framework
arXiv:1906.09382
Abstract
Semi-analytic models are best suited to compare galaxy formation and evolution theories with observations. These models rely heavily on halo merger trees, and their realistic features (i.e., no drastic changes on halo mass or jumps on physical locations). Our aim is to provide a new framework for halo merger tree generation that takes advantage of the results of large volume simulations, with a modest computational cost. We treat halo merger tree construction as a matrix generation problem, and propose a Generative Adversarial Network that learns to generate realistic halo merger trees. We evaluate our proposal on merger trees from the EAGLE simulation suite, and show the quality of the generated trees.
11 pages, 7 figures, 2 tables, 3 appendices. Presented at the ICML 2019 Workshop on Theoretical Physics for Deep Learning
References in corpus (18)
- Unsupervised Representation Learning with Deep Convolutional Generative Adversarial Networks
- The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
- The broken hierarchy of galaxy formation
- Hierarchical Galaxy Formation
- The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
- From dwarf spheroidals to cDs: Simulating the galaxy population in a LCDM cosmology
- A Semi-Analytic Model for the Co-evolution of Galaxies, Black Holes, and Active Galactic Nuclei
- Clustering of Galaxies in a Hierarchical Universe: I. Methods and Results at z=0
- A Recipe for Galaxy Formation Shaun Cole
- Chemical enrichment of the intra-cluster and intergalactic medium in a hierarchical galaxy formation model
- A new model of galaxy formation: How sensitive are predicted galaxy luminosities to the choice of SPS model?
- Early supersymmetric cold dark matter substructure
- Resolving Subhaloes' Lives with the Hierarchical Bound-Tracing Algorithm
- Generating Merger Trees for Dark Matter Haloes: A Comparison of Methods
- Galaxy Formation Spanning Cosmic History
- The Accuracy of Subhalo Detection
- Peaks above the Maxwellian Sea: A New Approach to Finding Substructure in N-Body Haloes
- Sussing Merger Trees : The Impact of Halo Merger Trees on Galaxy Properties in a Semi-Analytic Model