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Alumni Day

 

Join us for Annual Graduate Alumni Day, where three UK Mathematics alumni from the University of South Florida, Georgia Tech, and Microsoft return to share the career paths and insights from life in and beyond academia. Come ready to listen, ask and leave with a clearer picture of what's possible.

Schedule:

  • 2:00 PM — Mathematicians in the Age of Technology | Tefjol Pllaha, University of South Florida
  • 3:00 PM — An Academic Professional Does What? | Hunter Lehmann, Georgia Institute of Technology
  • 4:30 PM — Life After the Ph.D.: Research Beyond Academia | Vasily Zadorozhnyy, Microsoft

 

Visitor Parking

Visitor parking is available nearby. Rates are $2/hour unless noted.

Garage: Cornerstone Garage (PS #5) has entrances on South Limestone and Upper Street. Cost is $2/hour with a $30/exit maximum.

Surface Lots (pay at the meter):

  • W.T. Young Library Visitor Lot — off Hilltop Avenue
  • Prall Street Lot — off South Limestone/Upper Street (note: pay at the meter in front of your space only)

For more visitor parking information, visit transportation.uky.edu/visitoroptions.

 

Event poster for the University of Kentucky Department of Mathematics Annual Graduate Alumni Day, Friday, March 27, 2026, 2:00–5:30 PM, Chemistry Physics Building 287. Features three talks: 'Mathematicians in the Age of Technology' by Tefjol Pllaha (University of South Florida) at 2:00 PM; 'An Academic Professional Does What?' by Hunter Lehmann (Georgia Institute of Technology) at 3:00 PM; and 'Life After the Ph.D.: Research Beyond Academia' by Vasily Zadorozhnyy (Microsoft) at 4:30 PM. Sponsored by the UK Department of Mathematics, College of Arts and Sciences.

Date:
-
Location:
ChemPhys 287, Room 287
Event Series:

Physics & Astronomy Colloquium

Dr. Sang Mo Yang, Sogang University, South Korea

Title: Ferroelectricity at the Nanoscale: Emerging Materials and Local Probes

Abstract: Ferroelectricity on the nanoscale has been the subject of considerable interest in condensed matter physics for over half a century. Beyond its fundamental importance, ferroelectricity provides essential functionality for advanced electronic devices, including nonvolatile memories, field-effect transistors and tunnel junctions. 

However, conventional perovskite-based ferroelectric oxides (e.g., Pb(Zr,Ti)O3) face significant challenges in achieving device performance that can compete with current dynamic random-access memories and flash memories. Over the past decade, novel ferroelectricity has been discovered in new material systems, including fluorite-structured HfO2-based thin films, two-dimensional (2D) van der Waals (vdW) materials and 2D perovskite halides. These discoveries have brought about a renaissance in the ferroelectric research community. 

In this colloquium, I will present our group’s recent efforts to investigate and understand ferroelectricity across these emerging material platforms [1] using various scanning probe microscopy techniques.
[1] T. H. Jung et al., “Spatially Resolved Observation of Ferroelectric-to-Paraelectric Phase Transition in a Two-Dimensional Halide Perovskite,” Advanced Materials 37, 2506270 (2025)

Date:
-
Location:
CP 153

Physics & Astronomy Colloquium

Dr. Joel Leja, Penn State University

Title
Again but faster, better and with more physics: ML-accelerated inference of galaxy properties in deep and wide surveys of the universe
 
Abstract
The inference of the physical properties of galaxies at cosmological distance requires modeling a wide range of physics, including e.g. stellar evolution and atmospheres; dust attenuation and re-emission; nebular physics;  and AGN emission. Bayesian inference is often used to map the inevitable degeneracies, and the large amount of physics and wide parameter space means these codes are typically not fast. Yet current and near-future surveys of the universe will yield spectra for millions of galaxies and imaging for billions. 
 
I will introduce new tactics employed to speed up these codes, ranging from neural net emulators of key physics (photoionization modeling; stellar spectra) to efficient gradient-enhanced GPU-accelerated high-dimensional sampling to rapid simulation-based inference. These tactics yield speed-ups of somewhere between 100x and 100,000x with different trade-offs in flexibility and accuracy. In addition to unlocking industrial-scale modeling of galaxy surveys, I will discuss qualitatively new science directions enabled by these breakthroughs, such as modeling entire galaxy populations rather than one-at-a-time approaches and extremely high dimensional modeling of individual systems, e.g. spatially resolved modeling.
Date:
-
Location:
CP 153
Event Series:

More than 2,100 students achieve inclusion in Fall 2025 Dean's List for UK College of Arts and Sciences

More than 2,100 students have been named to the University of Kentucky College of Arts and Science's Dean's List for Fall 2025<. To earn Dean's List honors, students must earn:

  • A semester GPA of 3.6 or greater.
  • A least 12 earned credit hours in graded coursework. Earned credit hours taken as Pass/Fail are excluded.

A list of Dean's List students may be found here


 

Physics & Astronomy Astro Seminar

Title: Alien oceans: hot springs, phosphorus, and the search for life in the solar system

Abstract: The discovery of liquid water oceans on Saturn’s moon Enceladus in 2006 and as many as a dozen other moons in the solar system (most notably Jupiter’s moon Europa) has greatly changed our understanding of our solar system’s "habitable zone." Rather than simply searching for liquid water, planetary scientists now need a framework to assess the relative likelihood of different planetary targets to host the physical and chemical ingredients required to support detectable biology. 

In this talk, I will discuss the planetary (hydrothermal) and exogenous (meteoritic sedimentation) processes leading to nutrients and bioavailable energy on ocean moons. I show how even a relatively tectonically quiescent seafloor can lead to hydrothermal circulation. I will then focus on a specific bioessential nutrient produced by this circulation: phosphorus that was recently discovered on Enceladus. Our published results anticipated those observations to within analytical error of the satellite. I show how models integrating stellar stoichiometry and an understanding of thermodynamics and fluid dynamics can lead to testable predictions of icy moon ocean chemistry. Finally, I discuss the implications for exoplanet and future planetary science missions. 

Date:
-
Location:
CP 303

Physics & Astronomy String Seminar

Title: Exact Transition Amplitudes in Liouville CFT and the Cigar

Abstract: We study exact transition amplitudes in certain 2D CFTs — Liouville theory and the SL(2,R)/U(1) coset model describing Witten's 2D black hole. Using bootstrapped conserved currents and a generating functional approach based on canonical transformations, we compute these transitions both recursively and via functional integral representations. The tree-level evaluation of the generating functional reproduces exact results, while providing a diagrammatic framework for loop corrections. We also find that the statistics of Liouville transition elements at higher oscillator levels exhibit level repulsion.

Date:
-
Location:
CP 303
Event Series:

Fall Commencement 2025

Gallery of Photos from Fall Commencement 2025 - Photos by Nathan Parker

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