Colloquium Calendar
Below is the colloquium calendar for the current semester. All in-person colloquia are held in Malott Hall 1003, beginning at 11:00 a.m. Colloquium refreshments will be available outside room 1003 at 10:30 a.m. unless otherwise announced. Talk titles and abstracts can be found in the accordions below the calendar when available. Please visit the department YouTube Channel (external) for recordings of colloquia when available.
Graduate students in the department can submit their attendance by filling out this form.
| Date | Format | Speaker | Topic | Affiliation | KU Faculty Host | Zoom |
|---|---|---|---|---|---|---|
| August 25th, 2025 | In-Person | Jennifer Lotz | Astro | Space Telescope Inst. | Rudnick | Zoom Link pw: 408508 |
| September 1st, 2025 | No Colloquium | Labor Day Holiday | ||||
| September 8th, 2025 | In-Person | Gabriele Carcassi | Univ Michigan | Tapia Takaki | Zoom Link pw: 408508 | |
| September 15th, 2025 | In-Person | Rachael Farber | KU Chemistry Dept | Zhou | Zoom Link pw: 408508 | |
| September 22nd, 2025 | In-Person | Diana Qiu | Yale Univ | Zhou | Zoom Link pw: 408508 | |
| September 29th, 2025 | In-Person | Hai Fu | Univ Iowa | Rudnick | Zoom Link pw: 408508 | |
| October 6th, 2025 | In-Person | Qimin Yan | Northeastern Univ | Zhou | Zoom Link pw: 408508 | |
| October 13th, 2025 | No Colloquium | Fall Break | ||||
| October 20th, 2025 | In-Person | Xia Hong | CMP | Univ Nebraska-Lincoln | Zhao | Zoom Link pw: 408508 |
| Postponed - date TBD | Bruce Macintosh | Astro | Director, UC Observatories | Crossfield | ||
| November 3rd, 2025 | In-Person | Wennie Wang | Univ Texas Austin | Peelaers | Zoom Link pw: 408508 | |
| November 10th, 2025 | In-Person | Zoya Valairi | Ohio State Univ | Brunetti | Zoom Link pw: 408508 | |
| November 17th, 2025 | In-Person | Stefania Gori | Univ California, Santa Cruz | Lewis | Zoom Link pw: 408508 | |
| November 24th, 2025 | No Colloquium | Thanksgiving Break | ||||
| December 1st, 2025 | In-Person | Andreas Papaefstathiou | Kennesaw State Univ | Lewis | Zoom Link pw: 408508 | |
| March 2nd, 2026 | In-Person | Kristina Nyland | Astro | Computational Physics Inc | Mills | |
| April 20th, 2026 | In-Person | Bruce Macintosh | Astro | Director, UC Obervatories | Crossfield | |
Fall 2025 Colloquia
Title: The Legacies of Hubble, Webb, and future NASA astrophysics flagship missions
Abstract:
For the past four decades, the Space Telescope Science Institute has served as the bridge between NASA's flagship astrophysics missions and the scientific community through its role as the science operations center for Hubble, Webb, and Roman. The Hubble Space Telescope is celebrating its 35th year of operations, and continues to lead innovative new discoveries with its ultraviolet-optical capabilities and decades of high precision data. In its third year of operations, the infrared James Webb Space Telescope is the most powerful telescope ever built and is rapidly transforming a broad range of astronomy fields, including galaxy evolution, cosmology, star-formation, and exoplanet science. In two years, the Nancy Grace Roman Space Telescope will launch and begin to survey the sky at speeds 1000 times that of Hubble. Roman is designed to study cosmological questions about the nature of dark energy, the evolution of the expansion rate, and the growth of large-scale structure over cosmic time, as well as detect tens of thousands of exoplanets and demonstrate cutting-edge technology to directly image exoplanets. Finally, STScI is working to support the next generation NASA astrophysics flagship mission, the Habitable Worlds Observatory. This mission will be a "super-Hubble" capable of detecting earth-like planets around sun-like stars, tracing the cosmic intergalactic medium, and spatially-resolving every known galaxy in the universe. These NASA flagship missions have immeasurable impact on the field of astrophysics and how astronomers around the world do science. They enable STEM workforce development across the U.S. and are clear demonstrations of U.S. and NASA's leadership in science and technology. I will discuss the challenges that cuts to NASA's science budget pose for the future of these missions.
Title: Assumptions of Physics: a new principled approach to the foundations of physics
Abstract:
We will give an overview and the main results of the Assumptions of Physics project, which aims to find minimal sets of physically meaningful starting points from which the different physical theories can be rederived. It consists of two main strategies. The first, Reverse Physics, starts from the known physical laws and studies principles and assumptions that are equivalent to the mathematical formulation. This allows one to create a clear dictionary between physical concepts and their mathematical representation, showing us, for example, what physical assumptions are equivalent to the principle of least action, or that geometric structures in physics are equivalent to entropic structures. The second approach, Physical Mathematics, aims to rederive all mathematical structures used in physics "from scratch," giving physics a more conceptually solid mathematical foundation. Ultimately, this will lead to a theory of physical theories, which can be used to better understand the current ones and to aid the search for new ones.
Title: Uncovering the Fundamental Interactions Guiding Thin Film Growth and Electronic Metal-Support Interactions
Abstract: There is a central relationship between material structure, composition, and function. For complex surface processes, such as thin film growth and heterogeneously catalyzed chemical transformations, representative systems interrogated with surface science techniques can reveal the atomic-scale mechanisms underpinning observed material activity. Such studies have broadened the understanding of, and are integral to, developing accurate models for many interfacial phenomena. In this presentation, I will discuss recent results investigating the nanoscale chemical, structural, and electronic processes guiding 1) binary and single-component self-assembled monolayer (SAM) formation and 2) the emergence of electronic metal-support interactions in oxide-supported metal nanoparticle catalysts.
Title: From Light to Learning: Predicting Excited-State Dynamics at the Spectroscopic Frontier
Abstract:
Processes ranging from photosynthesis, to photocatalysis, to energy harvesting in photovoltaic cells all begin in the same way: the absorption of light creates an exciton—a correlated electron-hole pair that carries energy rather than charge. Exciton dynamics and coherences determine the efficiency of energy harvesting and transport, while excitonic manipulation enables the optical preparation and transduction of quantum states and offers the potential to integrate the fast speed of photons into electronics. However, quantitative predictions of exciton and other excited-state dynamics remain a significant challenge. The first-principles understanding of exciton dynamics requires a few basic building blocks: 1) The full exciton dispersion to capture the phase space of momentum and energy conserving scattering processes, 2) Interaction of excitons with external perturbations such as electromagnetic fields and lattice vibrations, and 3) An equation of motion describing the dynamical processes. In this talk, I will discuss some of my group’s developments in these directions. Firstly, we have recently measured the exciton dispersion in a 2D materials revealing for the first time the emergence of a massless excitons composed of massive electrons and holes [1]. Secondly, we will show how excitons play a surprising role in nonlinear optics beyond the perturbative regime. Using newly developed first principles techniques, we find that excitons enhance high-harmonic generation in monolayer semiconductors, in ways directly tied to the Berry curvature of the underlying bands. Finally, I will discuss how machine learning is opening new possibilities for simulating excited states far beyond the reach of conventional calculations [3,4].
References:
[1] L. Liu, S.Y. Woo, J. Wu, B. Hou, C. Su, D.Y. Qiu, “Direct Observation of Massless Excitons and Linear Exciton Dispersion,” arXiv:2502.20454v2 (2025).
[2] V. Chang Lee, L. Yue, M.B. Gaarde, Y.-H. Chan, D.Y. Qiu, “Many-body enhancement of high harmonic generation in monolayer MoS2,” Nature Comm. 15, 6228 (2024).
[3] B. Hou, J. Wu, D.Y. Qiu, "Unsupervised representation learning of Kohn–Sham states and consequences for downstream predictions of many-body effects," Nature Comm. 15, 9481 (2024).
[4] B. Hou, X. Xu, J. Wu, D.Y. Qiu, "MBFormer: A General Transformer-based Learning Paradigm for Many-body Interactions in Real Materials," arXiv:2507.05480 (2025).
Title: Resolving the Hubble Constant Discrepancy: Mitigating Biases in Cosmic Distance Ladders
Abstract:
The Hubble constant (H0), representing the present-day expansion rate of the universe, exhibits an approximately 8% discrepancy between direct measurements in the late universe and indirect measurements from the early universe. Accurate direct measurements are challenging because they require measuring cosmic distances far beyond our galaxy, necessitating the use of a distance ladder with multi-step calibrations of different distance indicators. While propagated measurement errors contribute only about 1% to the uncertainty in H0, biases in inference and priors may be at the same level as the observed discrepancy. I will discuss two important biases: Malmquist bias, stemming from observational selection and luminosity dispersion, and Eddington bias, resulting from the scatter and non-uniform distribution of the luminosity indicator. With simulated data, I will show that these biases can be mitigated by constructing the data likelihood function to account for their contributing factors. By applying these methods, future direct measurements of H0 can achieve unbiased precision, potentially resolving the current discrepancy.
Title: From simple to complex: learning pathways for solid-state quantum systems
Abstract:
Complex properties of solid-state quantum systems are entangled with a set of physical quantities and constraints, such as orbital interactions, Hamiltonian, and global/local atomic environment and symmetries. In recent years, artificial intelligence (AI) and machine learning (ML) have been widely applied to many aspects of physical sciences, while the use of ML for either complex solid-state systems or complex properties of solids remains challenging. In this talk, I will introduce recent developments of ML frameworks that enable the prediction of complex properties in solid-state quantum systems from simple graph representations and physical principles. The talk will focus on model developments for two types of complex properties that are associated with (i) electronic structures and (ii) configurations.
Two routes for electronic structure learning will be discussed: end-to-end predictions and Hamiltonian learning. I will introduce a universal and end-to-end graph-Transformer-based model predicting the electronic band structure of any crystalline system based on atomic structure input only. The mean absolute error is ~0.3 eV for band energy predictions, which is believed to be essential for ML-accelerated discovery/design of functional quantum materials. In terms of Hamiltonian learning, I will discuss how existing ML force field models can be reused and combined with physical-principle-informed embeddings to build an efficient model for predicting electronic structures of large-scale twisted two-dimensional materials. Beyond basic electronic structures, I will introduce a model built on top of equivariant neural network to predict one of the most complicated electronic-structure-derived properties in solids: tensorial spectra.
In the field of applying ML for material systems with tremendous numbers of configurations, I will introduce a general ML framework for modeling ensemble properties of atomically disordered materials such as multi-compositional alloys. I will discuss how equivariant neural network models can be combined with first-principles computational approaches for atomistic systems and statistical methods to enable fast and reliable predictions for both disorder-related properties (such as order-disorder phase transitions) and ensemble properties of these systems, which are not accessible by traditional computational approaches.
At the conclusion of the talk, I will highlight ongoing progress in modeling complex properties of solids, with particular attention to data challenges and the need for collective community efforts to address them.
Title: Emergent Phenomena in Ferroelectric Oxide/van der Waals Heterostructures
Abstract:
The heterointerfaces between ferroelectric oxides and two-dimensional (2D) van der Waals materials present a versatile platform for achieving novel interfacial coupling, nonvolatile field effect control, and nanoscale programmable functionalities. In this talk, I will discuss a range of emergent phenomena in ferroelectric oxide/vdW heterostructures mediated by interfacial coupling of charge, lattice, and polar symmetry. By combining polarization doping with nanoscale domain patterning in a ferroelectric Pb(Zr,Ti)O3 (PZT) gate, we create one-dimensional graphene superlattice in the high Kronig-Penney potential limit [1]. Negative capacitance (NC) transistors are developed based on polycrystalline PZT gated MoS2, which exhibits ultralow subthreshold swing of 9.7 mV/decade at 300 K. Theoretical modeling and PFM studies suggest that the NC mode is enabled by the metastable polar states within the domain walls [2]. We observe enhanced polar alignment, piezoelectricity, and Curie temperature in thin CuInP2S6 flakes prepared on PZT, which can be attributed to the tilt of the free-energy quadruple well via interfacial strain coupling [3]. An unconventional tuning effect of second harmonic generation signal is enabled by the polar coupling of monolayer MoS2 with either the polar domain or the chiral dipole rotation at the domain wall surface in PZT thin films and free-standing membranes [4]. Our study showcases the rich research opportunities offered by integrating ferroelectric oxides with 2D materials.
[1] T. Li et al., Phys. Rev. Lett.132, 056204 (2024).
[2] Song et al.,npj 2D Mater. Appl.6, 77 (2022).
[3] K. Wang et al., ACS Nano17, 15787 (2023).
[4] D. Li et al., Nat. Commun.11, 1422 (2020); D. Li et al., Adv. Mater.35, 2208825 (2023).
Title: Leveraging defects and interfaces in low-dimensional materials for memristors
Abstract: Two-dimensional materials have recently been shown to demonstrate non-volatile resistive switching, offering significant advantages such as high-density integration and low energy consumption due to their atomic-scale thinness. Previous experimental work indicates that vertical heterojunctions based on transition metal dichalcogenides (TMDs) exhibit resistive switching and I-V hysteresis. Using first-principles calculations, we develop material-based relationships for resistive switching mechanisms based on the formation and dissolution defects and study the interfacial interactions that give rise to memory effects. Understanding the separate electronic, ionic, and coupled contributions in resistive switching mechanisms using first-principles methods is an overarching goal.
In this presentation, I will describe our work in the computational characterization of defects in 2D materials in the monolayer and at the interface, understanding materials trends relating to switching energy, and elucidating the impact of an applied electric field on interfacial transport. Our results reveal that defect energetics of transition metals are connected to resistive switching processes and exhibit consistent materials trends across different TMDs (MoS2, MoSe2, WS2, WSe2). I will describe several models that explain this trend. Finally, I will discuss the effects of electric field in the hysteresis cycle and how structural asymmetry of the heterostructure and point defects impact the interfacial characteristics of the system on several I-V characteristics, such as the coercive voltage, remnant polarization and dissipation ratio.
Title: A 𝝂 Perspective on Particle Physics
Abstract:
Once an unlikely hypothesis not foreseen by the Standard Model, the existence of nonzero neutrino mass is now an experimentally verified fact. Neutrino oscillation experiments remain the first and sole evidence of this scientific breakthrough. The extraordinarily smallness of neutrino mass and the weakness of neutrino interactions determine the scale of observable phenomena, making these experiments particularly challenging.
In this talk, I will outline how neutrino oscillation experiments continue to provide a rich environment for exploring fundamental physics, specifically for determining the neutrino mass ordering, searching for potential charge-parity violation in the lepton sector, and making precision measurements to probe the unitarity and completeness of the three-flavor neutrino paradigm. I will review the current landscape of the results from the long-baseline neutrino oscillation experiments, and present the results from the currently operational NOvA and the T2K experiments. Additionally, I will highlight and contrast how next-generation experiments are designed to achieve the target sensitivities needed to answer these fundamental physics questions.
Title: The origin of neutrino masses
Abstract:
Neutrinos are among the most mysterious particles in the Standard Model. We know they have mass, but we do not yet understand how these masses arise or whether neutrinos are their own antiparticles. This talk will explore current theoretical and experimental efforts to uncover the origin of neutrino masses, focusing on the distinction between Dirac and Majorana neutrinos and the role of lepton-number violation. I will present new theoretical results demonstrating the existence of additional observables, beyond neutrinoless double beta decay, that could shed light on the origin of neutrino masses, and discuss the experimental prospects for probing them in upcoming searches.
Title: Exploring Scalar Sectors at the LHC and Beyond
Abstract:
The Standard Model of particle physics provides remarkably precise predictions that have been tested and confirmed across decades of collider experiments. Yet its scalar sector, which contains the Higgs field, remains the least understood part of the theory. This talk explores how the scalar sector of the SM can be "deformed" through anomalous interactions, or extended by new scalar fields, motivated by open questions. I will present recent progress in constraining these possibilities, and highlight how multi-scalar production processes at the LHC and future colliders offer uniquely sensitive probes of the underlying structure of the scalar sector.
Please follow this link for an archive of previous colloquia.