activity
20242026
collaborators

11 papers

astro-ph.CO2026

Optimal and exact wide-angle power spectrum estimation

Noah Sailer, Kendrick Smith, Yurii Kvasiuk +2

What is the optimal power spectrum estimator on ultra-large scales where the plane-parallel approximation breaks down? Conventional estimators, such as the Yamamoto estimator, are…

q-fin.TR2026

MadEvolve: Evolutionary Optimization of Trading Systems with Large Language Models

Yurii Kvasiuk, Tianyi Li, Owen Colegrove +1

We explore the application of LLM-driven algorithm optimization to several common tasks in quantitative finance. MadEvolve, a general-purpose algorithm optimization framework inspi…

astro-ph.CO2026

QML-FAST -- A Fast Code for low- Tomographic Maximum Likelihood Power Spectrum Estimation

Yurii Kvasiuk, Anderson Lai, Moritz Münchmeyer +1

We present a novel implementation for the quadratic maximum likelihood (QML) power spectrum estimator for multiple correlated scalar fields on the sphere. Our estimator supports ar…

cs.LG2026

Fine-Tuning Small Reasoning Models for Quantum Field Theory

Nathaniel S. Woodward, Zhiqi Gao, Yurii Kvasiuk +3

Despite the growing application of Large Language Models (LLMs) to theoretical physics, there is little academic exploration into how domain-specific physics reasoning ability deve…

astro-ph.CO2025

The Simons Observatory: forecasted constraints on primordial gravitational waves with the expanded array of Small Aperture Telescopes

The Simons Observatory Collaboration, I. Abril-Cabezas, S. Adachi +479

We present updated forecasts for the scientific performance of the degree-scale (0.5 deg FWHM at 93 GHz), deep-field survey to be conducted by the Simons Observatory (SO). By 2027,…

astro-ph.CO2025

Reconstruction of Dark Matter and Baryon Density From Galaxies: A Comparison of Linear, Halo Model and Machine Learning-Based Methods

Jordan Krywonos, Yurii Kvasiuk, Matthew C. Johnson +1

For many analyses in cosmology it is necessary to reconstruct the likely distribution of unobserved fields, such as dark matter or non-luminous baryons, from observed luminous trac…