Subject Area

Physics

Abstract

In both cosmology and small-x quantum chromodynamics, the relevant theoretical predictions are well-defined but expensive to evaluate repeatedly over broad parameter spaces or large ensembles of simulated data. The central question of this thesis is when machine learning can accelerate those calculations without weakening the reliability of the final physics conclusions. The thesis develops and tests this idea in three settings. First, it studies the Derivative Approximation for Likelihoods (DALI) as a means of diagnosing when Fisher-matrix forecasts cease to be trustworthy in cosmological parameter inference. Second, it investigates graph-based spherical neural networks for estimating primordial non-Gaussianity directly from simulated cosmic microwave background maps and benchmarks their performance against Fisher and Komatsu-Spergel-Wandelt estimator targets. Third, it constructs neutral-network surrogates for the Balitsky-Kovchegov equation in order to accelerate diploe-model calculations relevant to deep-inelastic scattering as small Bjorken-x. Across these projects, the main conclusion is methodological rather than a novel discovery. Machine learning is most useful here when it functions as a calibrated surrogate within a theory-first workflow. In that setting, the exact calculation remains the standard of truth; the learned model is trained against controlled numerical data, and performance is judged by physics-level validation rather than by generic machine-learning metrics alone. The results show that surrogate models can provide substantial computational gains in controlled regimes, but they must be paired with explicit validity tests and final cross-checks against higher-fidelity calculations before they are used to support scientific claims.

Degree Date

Spring 2026

Document Type

Dissertation

Degree Name

Ph.D.

Department

Physics

Advisor

Fred Olness

Second Advisor

Difeng Cai

Third Advisor

Thomas Coan

Fourth Advisor

Joel Meyers

Number of Pages

177

Format

.pdf

Creative Commons License

Creative Commons Attribution-Noncommercial 4.0 License
This work is licensed under a Creative Commons Attribution-Noncommercial 4.0 License

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