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Physics & Astronomy Colloquium

Dr. Hendrik Schatz, Michigan State University

Title: Rare Isotopes in the Cosmos

Abstract: Atomic nuclei with short lifetimes of fractions of seconds, so called rare isotopes, play an important role in the universe despite their fleeting existence. They serve as stepping stones for the synthesis of chemical elements, they shape the nature of stellar explosions, and they are the major constituents of neutron stars. I will give an overview of the role of rare isotopes in the cosmos and recent efforts to study astrophysical reactions involving rare isotopes at the Facility for Rare Isotope Beams at Michigan State University. As an example, I will discuss accreting neutron stars. These systems are among the brightest X-ray sources in the sky and exhibit an extraordinay range of rare isotope physics. By combining observations, astrophysical modeling, and nuclear physics experiments they can provide new insights into the behavior of matter under extreme temperatures and densities. 

Date:
-
Location:
CP 153
Event Series:

Physics & Astronomy Colloquium

Dr. Ambrose Seo, University of Kentucky

Title: Shaping Light and Charge in Two-Dimensional Materials with Plasmonic Nanostructures

Abstract: Two-dimensional materials such as MoS2 are just one atom thick, which gives them remarkable optical and electronic properties, but also makes them challenging to use efficiently in devices, since their ultrathin nature limits how strongly they interact with light. During my sabbatical in Seoul, I explored new ways to overcome this challenge by combining MoS2 with carefully designed metallic nanostructures that can trap and guide light at the nanoscale. By embedding gold or silver nanowires and nanogrooves beneath or alongside MoS2, we found that we could significantly boost its light emission, collect photo-generated charges more effectively, and improve the efficiency of heterostructures that pair MoS2 with oxide semiconductors. These studies show how "plasmonic" effects, i.e., collective oscillations of electrons in metals, can be harnessed to control light–matter interactions in atomically thin materials. I will present the key outcomes of these projects and discuss how they point toward future opportunities for next-generation devices.

Date:
-
Location:
CP 153
Event Series:

Uncertainty-aware generative models for autonomous discovery in particle theory

Uncertainty quantification (UQ) plays a crucial role in the predictive power of nonperturbative quantum correlation functions at high precision. My research explores novel approaches to UQ in the context of parton distribution functions (PDFs), using uncertainty-aware machine learning techniques to map observables to underlying theoretical models and to navigate the complex parametric landscape of phenomenological scenarios, including the vast ecosystem of beyond-the-Standard-Model (BSM) configurations. By leveraging modern generative AI methods, I investigate how the inherent uncertainties in phenomenological extractions of collinear PDFs impact the landscape of potential New Physics models. My approach integrates explainability methods to trace underlying theory assumptions back to the input feature space - specifically the x-dependence of PDFs - thereby identifying the salient features that shape constraints and model interpretations. Additionally, this work aims to enhance the incorporation of lattice inputs in phenomenological fits and refine the consistency between lattice QCD and collider phenomenology. Together, these components point towards uncertainty-aware autonomous workflows, pushing the frontier of particle physics discovery.
 
Date:
-
Location:
CP 303
Event Series:

Arts and Sciences welcomes new faculty (2025-2026)

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Physics & Astronomy Astro Seminar

Title: How "Little Red Dots" Broke the Universe (and how we're unbreaking it)

Abstract: One of the biggest mysteries of the early era of JWST's operation has been "Little Red Dots," compact sources with strange V shaped spectral energy distributions and broad emission lines. These sources have been incredibly hard to model, and over the course of three years, leading theories have ranged from over-massive galaxies that assembled Milky Way levels of stellar mass in the first Gyr of cosmic time to over-massive active galactic nuclei that defy models of black hole assembly. I will walk through the brief history of discover in this sources, demonstrating how we have slowly been getting closer and closer to understanding them by leveraging JWST, ALMA, and several other observatories to constrain their panchromatic spectral energy distribution. I will discuss our current best understanding of these sources, and how we might move forward to incorporate them into our picture of galaxy and black hole assembly.

Date:
-
Location:
Virtual (https://uky.zoom.us/j/82910452708)
Event Series:

Physics & Astronomy Colloquium

Dr. Daniel Tataru, University of California, Berkeley

Title: Free boundary problems for Euler flows

Abstract: Free boundary problems are very interesting but also very challenging problems in fluid dynamics, where the boundary of the fluid is also freely moving along with the fluid flow. 

I will discuss two such models, governed by the compressible, respectively the incompressible Euler equations, including also MHD flows.  This is joint work with Mihaela Ifrim, and in part with Benjamin Pineau and Mitchell Taylor.

Date:
-
Location:
CP 153
Event Series:

Statistics Seminar

Title: Conformal prediction of future insurance claims in the regression problem

Abstract: In the current insurance literature, prediction of insurance claims in the regression problem is often performed with a statistical model. This model-based approach may potentially suffer from several drawbacks: (i) model misspecification, (ii) selection effect, and (iii) lack of finite-sample validity. This article addresses these three issues simultaneously by employing conformal prediction-a general machine learning strategy for valid predictions. The proposed method is both model-free and tuning-parameter-free. It also guarantees finite-sample validity at a pre-assigned coverage probability level. Examples, based on both simulated and real data, are provided to demonstrate the excellent performance of the proposed method and its applications in insurance, especially regarding meeting the solvency capital requirement of European insurance regulation, Solvency II.

 

Date:
-
Location:
MDS 220
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