Galaxy Morphology & Topological Representations
Persistent homology and self-supervised learning for robust, interpretable descriptors of galaxy images from surveys such as Galaxy Zoo.
Research
My research aims to connect algebraic topology and machine learning with concrete problems in astrophysics, complex systems, and condensed matter physics.
My PhD focuses on Topological Data Analysis and Topological Deep Learning Applied to Physical Systems Across Scales. The central idea is to use persistent homology, Mapper, and graph neural networks to construct robust, interpretable descriptors of physical fields and time series.
A few representative topics I currently work on. Each card links to publications, talks, or software where you can find more details.
Persistent homology and self-supervised learning for robust, interpretable descriptors of galaxy images from surveys such as Galaxy Zoo.
Topological summaries of time-series data to detect gravitational-wave-like signals in very noisy regimes.
Using topological characteristics of oscillation spectra to study stellar structure and relate mode content to physical parameters.
Applying TDA to magnetohydrodynamic shock-tube simulations to understand the failure modes of convolutional neural network temporal predictors.
Using homology and Mapper to characterize phase-space structure in nonlinear dynamics and networked systems beyond pairwise interactions.
Topological analysis of experimental Barkhausen noise and toy models to connect homological signatures with avalanche statistics and criticality.
At the astronomical scale, I study how topological signatures appear in data such as light curves, power spectra, and images. This includes:
At intermediate scales, my work explores fluid dynamics, magnetohydrodynamics, and dynamical systems. Topological tools are used to quantify structures such as shocks, vortices, and chaotic attractors.
At small scales, I study how topological features emerge in magnetic materials, Barkhausen noise, and quantum systems.