Testing and Emulating Modified Gravity on Cosmological Scales
Andrius Tamosiunas

TL;DR
This thesis develops methods for testing modified gravity models using galaxy clusters and introduces machine learning-based emulators for cosmological simulations, enabling faster and more efficient analysis of various cosmological scenarios.
Contribution
It presents novel techniques for constraining modified gravity models with galaxy clusters and introduces GAN-based emulators for cosmological simulation data.
Findings
Galaxy clusters provide powerful constraints on cosmological scales.
GAN emulators can produce accurate simulation data with 1-20% differences.
Emulators significantly speed up the generation of diverse cosmological scenarios.
Abstract
This thesis introduces a set of methods for testing models of modified gravity using galaxy clusters. In particular, a technique for constraining models with a chameleon screening is introduced. In addition, the outlined technique is expanded to test a wider class of models, such as the theory of emergent gravity. Finally, the first part of the thesis is concluded by adapting the mentioned tests for model independent constraints. The obtained results indicate that galaxy clusters can be used to obtain some of the most powerful constraints on cosmological scales. The second part of the thesis is dedicated to the topic of cosmological emulators. More specifically, a technique of emulating cosmological N-body simulation output data based on machine learning is introduced. Generative adversarial networks (GANs) are used to emulate dark matter-only as well as hydrodynamical simulation…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Cosmology and Gravitation Theories · Computational Physics and Python Applications
