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Physics & Astronomy String Theory Seminar

NB: non-standard time!


Title: Symmetry-weighted ensemble averaging from TQFT gravity

Abstract: In a recently proposed framework of TQFT gravity (2310.13044, 2405.20366) -- a toy model of AdS3 gravity -- a bulk 3d TQFT summed over all topologies is shown to be dual to a unitary ensemble of boundary 2d CFTs. I will show that the CFTs in this ensemble are weighted by the inverse of the order of their symmetry group (relative to the categorical symmetry provided by the bulk TQFT as a SymTFT). Mathematically, this is the natural measure over the groupoid of the TQFT Lagrangian algebras that construct the CFTs, and the holographic duality then provides a generalization of the Siegel-Weil formula beyond averaging over bosonic lattice-CFTs. I will also discuss some examples for rational CFTs as well as implications to noncompact TQFTs and pure gravity.

Date:
-
Location:
CP 303
Event Series:

Physics & Astronomy Colloquium

Dr. Matthew Bayliss, University of Cincinnati

Title: Taking Galaxies Apart and Putting Them Back Together Again

Abstract: Understanding the growth and evolution of stars and galaxies across cosmic time is a cornerstone of modern observational cosmology. After Cosmic Dawn, the first generation of galaxies powered much of cosmic re-ionization. Later, the global star-formation density accelerated toward its peak at Cosmic Noon, when most of the stellar mass in the Universe was formed. The industry standard is to use individual galaxies as the de facto measurement unit. There are practical reasons for counting galaxy-by-galaxy: galaxies grow and reside in dark matter haloes that map back to primordial mass over-densities, and even space-based observatories can only marginally resolve galaxies in the distant universe. However, the physical processes that drive galaxy growth and evolution -- cloud collapse, star formation, feedback, etc. -- operate on scales much smaller than a galaxy. I will present ongoing work using bright, strongly lensed galaxies to zoom in on the scales of individual star clusters to resolve the physics of what's happening inside distant galaxies. 

Date:
-
Location:
CP 153
Event Series:

Physics & Astronomy Nuclear Science Seminar

Title: From chiral effective field theory to perturbative QCD: A Bayesian model mixing approach to neutron star matter

Abstract: Constraining the equation of state (EOS) of strongly interacting, dense matter is the focus of significant experimental, observational, and theoretical effort. While chiral effective field theory (EFT) can describe the EOS between the typical densities of nuclei and those in the outer cores of neutron stars, perturbative QCD (pQCD) can be applied to properties of deconfined quark matter, both with quantified theoretical uncertainties.

However, describing the full range of densities in between with a single EOS that has well-quantified uncertainties is a challenging problem. Bayesian model mixing (BMM) can help bridge the gap between the two theories.

In this talk, I will present a BMM framework that can combine EOS constraints from different density regions in a principled way to construct a globally predictive, composite EOS model based on Gaussian processes (GPs). I will discuss applications of this BMM framework to the EOS and structure of neutron stars, as well as the statistical uncertainty quantification of the underlying microscopic EOS calculations.

Date:
-
Location:
CP 179
Event Series:

Statistics Seminar

Title: Doubly robust estimation and inference for a log-concave counterfactual density

Abstract: We consider the problem of causal inference based on observational data (or the related missing data problem) with a binary or discrete treatment variable. In that context, we study inference for the counterfactual density functions and contrasts thereof, which can provide more nuanced information than counterfactual means and the average treatment effect. We impose the shape-constraint of log-concavity, a type of unimodality constraint, on the counterfactual densities, and then develop doubly robust estimators of the log-concave counterfactual density based on augmented inverse-probability weighted pseudo-outcomes. We provide conditions under which the estimator is consistent in various global metrics. We also develop asymptotically valid pointwise confidence intervals for the counterfactual density functions and differences and ratios thereof, which serve as a building block for more comprehensive analyses of distributional differences.

Date:
-
Location:
MDS 220

Statistics Seminar

Title: Scalable distributional regression for wearable devices, adjusting for informative non-wear bias (plus hybrid statistical-AI generative models for complex structured data)

Abstract: Many modern instruments (wearables, imaging, geospatial sensors) generate subject-level data streams with thousands to millions or more measurements. Collapsing these to simple summaries (e.g., means) can obscure important structure. We present a general distributional regression framework for distribution-on-scalar and distribution-on-function settings. Distributions are modeled via subject specific empirical quantile functions and represented with quantlet basis functions that provide a compact and near-lossless representation for the subject-specific distributions, enabling joint inference on entire distributions and flexible post hoc computation of any distributional summary to characterize the differences.

Our approach is built on the Bayesian Functional Mixed Model (BayesFMM) framework, accommodating arbitrary mixes of discrete/continuous predictors with smooth (nonlinear) effects, multiple random-effects levels for multilevel designs, nonstationary spatial/temporal dependence, and Gaussian or heavier-tailed errors for robustness. A basis-projection strategy makes the method computationally scalable in both the number of subjects and the number of repeated measurements per subject. Simulation studies show greater efficiency than fitting separate models over a grid of quantiles.

To address informative missingness, we incorporate functional predictors that encode time-of-day non-wear patterns, effectively calibrating each subject’s distribution to a common non-wear profile. Simulations demonstrate that non-wear biases both full-distribution inference and scalar summaries, and we show that our proposed regression calibration approach mitigates this bias more effectively and much more computationally efficiently than imputation.

Applied to the TEAN adolescent accelerometer study, we confirm and refine associations of adolescent activity levels with age, BMI, and walkability, characterizing nuanced effects for these continuous predictors, and identifying which parts of the activity distribution shift without predefining summaries. 

Time permitting, I will briefly preview ongoing work using statistical generative AI to build inferential frameworks for complex object data while preserving key internal structure, with application to handwritten digits data, and show how both the distributional regression for wearable devices and generative AI model for digits data are encompassed by one general methodological framework.

 

Date:
-
Location:
MDS 220
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