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Events During the Week of April 27th through May 4th, 2025

Monday, April 28th, 2025

Plasma Physics (Physics/ECE/NE 922) Seminar
A Generative Artificial Intelligence framework for long-time plasma turbulence simulations
Time: 12:00 pm - 1:15 pm
Place: 1227 Engineering Hall
Speaker: Diego Del-Castillo-Negrete, University of Texas at Austin
Abstract: Generative artificial intelligence methods are employed for the first time to construct a surrogate model for plasma turbulence that enables long-time transport simulations [1]. The proposed GAIT (Generative Artificial Intelligence Turbulence) framework is based on the coupling of a convolutional variational autoencoder that encodes precomputed turbulence data into a reduced latent space, and a recurrent neural network and decoder that generate new turbulence states 400 times faster than the direct numerical integration. The model is applied to the Hasegawa-Wakatani (HW) plasma turbulence model, which is closely related to the quasi-geostrophic model used in geophysical fluid dynamics. Very good agreement is found between the GAIT and the HW models in the spatiotemporal Fourier and Proper Orthogonal Decomposition spectra, and the flow topology characterized by the Okubo-Weiss decomposition. The GAIT model also reproduces Lagrangian transport including the probability distribution function of particle displacements and the effective turbulent diffusivity. [1] B. Clavier, D. Zarzoso, D. del-Castillo-Negrete and E. Frenod, Phys. Rev. E Letters 111, L013202 (2025).
Host: Prof. Adelle Wright
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Tuesday, April 29th, 2025

Network in Neutrinos, Nuclear Astrophysics, and Symmetries (N3AS) Seminar
Dark Matter vs Neutrinos
Time: 2:00 pm
Place: Join Zoom Meeting:
Speaker: Aaron Vincent , Queen's University
Abstract: I will discuss the ongoing search for the nature of dark matter, and the possibility of finding it through the most invisible channel: the neutrino. Even though detection is difficult, neutrino telescopes provide observations that span a staggering 14 decades in energy, leading to broad constraints on dark matter models. Other indirect constraints, including cosmological effects on large scale structure and nucleosynthesis, and the relic abundance allow us to hone in on the parameter space. Finally, at high energies, the Glashow resonance allows for a much stronger sensitivity to new dark signals from heavy dark matter than previously thought, and one of the only smoking gun signatures of asymmetric dark matter.

NOTE: All participants and hosts are now required to sign into a Zoom account prior to joining meetings hosted by UC Berkeley.
Host: Baha Balantekin
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Wisconsin Quantum Institute Colloquium
Schroedinger cat in a silicon box: quantum information and quantum foundations
Time: 2:30 pm - 4:00 pm
Place: Discovery Building, DeLuca Forum
Speaker: Andrea Morello, School of Electrical Engineering and Telecommunications, UNSW Sydney, Australia
Abstract:

I will present recent experiments, and exciting new directions, for the use of high-spin nuclei in silicon for quantum information, quantum foundations, and spin-mechanics entanglement. Nuclear spins in silicon are among the most coherent quantum objects to be found in the solid state. They have infinite relaxation time, and second-scale coherence time [1]. By using the I=7/2, 8-dimensional nucleus of antimony [2], we have prepared a nuclear Schroedinger cat within a functional nanoelectronic device [3]. This can be used to encode a cat-qubit similar to the bosonic encodings used in microwave cavities, but with atomic size, and even more extreme noise bias. We then used this and other nonclassical states to perform a curious experiment, where the quanutmness of the state is certified by monitoring its uniform precession, in seeming contradiction with Ehrenfest's theorem [4]. High-spin nuclei possess a quadrupole moment that couples them to lattice strain [5]. I will discuss plans to entangle a single nuclear spin with a MHz-range mechanical oscillator, and perspectives to scale up the mass of the oscillator to test gravitational collapse models. [1] J. Muhonen et al., Nature Nanotechnology 9, 986 (2014) [2] S. Asaad, V. Mourik et al., Nature 579, 205 (2020) [3] X. Yu et al., Nature Physics 21, 362 (2025) [4] A. Vaartjes et al., Newton 1, 100017 (2025) [5] L. O'Neill et al., Applied Physics Letters 119, 174001 (2021)

This event starts at 2:30pm with refreshments, followed at 2:45pm by a short presentation by Brighton Coe (Eriksson group), titled "Light-induced offset charge in Si/SiGe quantum dots as a proxy for radiation impacts". The invited presentation starts at 3pm.

Host: Mark Eriksson
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Graduate Program Event
Mental Health for Graduate Students - Part 3 (of 3)
Conflict Resolution
Time: 4:00 pm - 5:00 pm
Place: B343 Sterling
Speaker: Neeti Shenoy, MA, and felix savino, Staff Psychologist, Mental Health Services/University Health Services
Abstract: Join Neeti Shenoy, MA, and felix savino, Staff Psychologist, Associate Director and Training Director at MHS, for a discussion of strategies for resolving conflicts.
Host: Sharon Kahn
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Outreach
Badgers on Tap
Time: 7:00 pm - 8:00 pm
Place: Working Draft Beer Company, 1133 E Wilson St, Madison, WI 53703
Speaker: Noah Hurst and Juliana Pacheco Duarte, UW–Madison Physics and NEEP
Abstract: Join plasma physics scientist Noah Hurst and NEEP professor Juliana Pacheco Duarte in a popular science talk on nuclear energy: fission and fusion as part of the Badgers on Tap series. More info coming soon!
Host: Badger Talks
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Wednesday, April 30th, 2025

Department Meeting
Time: 12:15 pm - 1:00 pm
Place: B343 Sterling Hall
Speaker: Kevin Black, UW - Madison
Host: Kevin Black
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Physics Department Colloquium
Wisconsin Union Directorate / Donald Kerst Distinguished Lecture Series
Adam Riess: The Surprising Expansion History of the Universe
Time: 7:00 pm - 8:30 pm
Place: Memorial Union, Shannon Hall
Speaker: Adam Riess, Space Telescope Science Institute
Abstract: Adam Riess is a distinguished astronomer at the Space Telescope Science Institute and a member of the National Academy of Sciences. In 2011, he was named a co-winner of the Nobel Prize in Physics and was awarded the Albert Einstein Medal for his leadership in the High-z Supernova Search Team’s discovery that the expansion rate of the universe is accelerating, a phenomenon widely attributed to a mysterious, unexplained "dark energy" filling the universe. The discovery was named by Science magazine in 1998 as "the Breakthrough Discovery of the Year." Free tickets are required, visit the website below to learn more. They will be available beginning April 23.
Host: WUD, L&S
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Thursday, May 1st, 2025

R. G. Herb Condensed Matter Seminar
Superconductivity with Anyons
Time: 10:00 am - 6:00 pm
Place: 5310 Chamberlin
Speaker: Hart Goldman, UMN
Abstract: I will discuss the phenomenology of superconductors hosting both order parameter vortices and fractionally charged anyon excitations. I will demonstrate that in such systems superconductivity and topological order are intertwined under applied magnetic fields, leading to surprising observable consequences departing from traditional superconductivity from electronic pairing. In particular, I will show that vortices nucleated by perpendicular magnetic fields must trap anyons in their cores. However, because only some vortices can trap an integer number of anyons, this places a constraint on the vortex phase winding. In general, rather than the expected hc/2e quantization of superconducting vortices, we find instead the enhanced flux quantum of hc/e, which I will argue should affect a wide range of observables. I will further develop a general Landau-Ginzburg theory describing vortex fluctuations and discuss the phase diagram as perpendicular magnetic field is increased, showing that condensation of the intertwined vortices leads to exotic insulating phases hosting neutral anyons and a nonvanishing thermal Hall effect.
Host: Elio König
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NPAC (Nuclear/Particle/Astro/Cosmo) Forum
The BayesLIM Project to map the high-redshift universe
Time: 2:30 pm - 3:30 pm
Place: Chamberlin 5280
Speaker: Nick Kern, MIT
Abstract: I will discuss using next-generation radio telescopes to map the high-redshift universe with unprecedented statistical precision, enabling us to tap into a trove of currently unharnessed cosmological information.

The Bayesian Line Intensity Mapping (BayesLIM) project leverages advances in machine learning software and hardware to deliver a comprehensive Bayesian forward model for cosmological intensity mapping experiments. Its goal is to enable the first robust detection of the high redshift 21 cm signal, while faithfully accounting for covariant uncertainties between the signal and contaminants.
Host: Peter Timbie
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Astronomy Colloquium
What JWST Reveals about the Hubble Tension
Time: 3:30 pm - 4:30 pm
Place: 4421 Sterling Hall
Speaker: Adam Riess, Johns Hopkins University
Abstract: The Hubble tension—the persistent discrepancy between local and early-Universe measurements of the Hubble constant—remains one of the most intriguing puzzles in cosmology. The James Webb Space Telescope (JWST) now offers a fresh perspective on this issue by allowing an independent look at the same type of stars, Cepheids, used in the Hubble Space Telescope (HST) measurements that help define our best local estimate of cosmic expansion. I’ll show how early JWST data, although still limited in size, serves as a powerful crosscheck of the HST-based distance ladder. When comparing results across multiple techniques and research groups, we find strong consistency with the HST measurements, lending confidence to their accuracy. These comparisons suggest that the observed tension is unlikely to stem from systematic errors in HST’s Cepheid distances. Though JWST’s smaller sample size limits its precision for now, it already provides valuable validation of the HST approach. As more data accumulates, JWST will play an increasingly important role in testing and refining our understanding of the expanding Universe—and perhaps help us get to the bottom of the Hubble tension.
Host: Melinda-Soares Furtado
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Friday, May 2nd, 2025

Academic Calendar
Last Spring Semester class day
Abstract: *Note: actual end time may vary.*
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Climate & Diversity
Diversity Forum Fridays! Addressing the Mental Health Needs of Underrepresented Collegiate Students
Time: 9:00 am - 10:30 am
Place: Chamberlin 5310 & Zoom
Speaker: Rachel Zizmann, UW-Madison Physics
Abstract: On college campuses, BIPOC, first-generation and low-income students are disproportionately underrepresented in seeking mental health services, highlighting systemic disparities in access to support. In this session, the panelists plan to discuss the role of the Community Support Specialists (CSS), who work exclusively with DDEEA students. This position was created by the Counseling Psychology Training Clinic (CPTC) in partnership with UW-Madison’s Mental Health Services (MHS) to increase counseling access among underrepresented students at UW-Madison using a social justice framework. The speakers will present an overview of the program’s history, including data and testimonials from past DDEEA students. During the session, panelists will share their experiences in the CSS roles, including their positionalities as BIPOC graduate students responsible for supporting the mental health needs of other underrepresented students. They will address questions about various interventions for supporting students, such as individual therapy, the role of outreach, and creative methods for disseminating interventions.
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Theory Seminar (High Energy/Cosmology)
Electroweak Symmetry Restoration at High Energies
Time: 1:30 pm - 3:00 pm
Place: Chamberlin 5280
Speaker: Tao Han, University of Pittsburgh
Abstract: With the milestone discovery of the Higgs boson at the LHC, detailed study of its properties becomes a high priority for collider physics. After a brief overview of the properties of the longitudinal gauge bosons and the Higgs boson, we revisit the Goldstone boson equivalence theorem and define the “electroweak symmetry restoration” (EWSR) quantitatively. We present some examples to examine the EWSR via the processes with "radiation amplitude zeros” by separating out the gauge sector and the scalar sector. Finally, we comment on what we learn from testing the EWSR and make some remarks on the SM at high energies in light of the UV completion.
Host: Lisa L Everett
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Thesis Defense
Superconducting diode effect
Time: 2:15 pm - 3:45 pm
Place: 2104 CH
Speaker: Jaglul Hasan, Physics PhD student
Abstract: In this thesis, we explore the generalities of the supercurrent diode effect. As an illustrative example, we examine a model of a two-dimensional superconductor with Rashba-type spin-orbit coupling under an in-plane magnetic field and in the clean limit, which realizes a helical phase. First, we utilize Ginzburg-Landau phenomenology to derive a general formula for the diode efficiency. This is achieved by incorporating higher gradient terms in the Lifshitz invariants, which are responsible for the nonreciprocal superflow. Subsequently, we validate these results through microscopic diagrammatic computation and further estimate correction terms arising from interband pairing correlations. We provide a detailed comparison to prior investigations of this problem conducted within the framework of the quasiclassical approximation based on the Eilenberger equation.

Even though superconducting diode effect (SDE) has garnered significant attention due to its potential applications in superconducting electronics, the role of disorder scattering in SDE has rarely been considered, despite its potential qualitative impact, as we demonstrate. We investigate SDE in a disordered Rashba superconductor under an in-plane magnetic field, employing a self-consistent Born approximation to derive the corresponding Ginzburg-Landau theory. Our analysis reveals two surprising effects. First, in the strong Rashba SOC regime, disorder becomes the driving mechanism of SDE, which vanishes in its absence. In this case, we show that disorder-induced mixing of singlet and triplet superconducting orders underlies the effect. Second, in the weak Rashba spin-orbit coupling (SOC) regime, disorder can reverse the direction of the diode effect, indicated by a sign change in the superconducting diode efficiency coefficient.
Host: Alex Levchenko
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Physics Department Colloquium
TBD
Time: 3:30 pm - 4:30 pm
Place: Chamberlin 2241
Speaker: Erika Marin-Spiotta, University of Wisconsin-Madison
Host: Kevin Black
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Awards
Physics Student & Alumni Awards Banquet
Time: 5:30 pm - 8:30 pm
Place: Discovery Building
Speaker: Kevin Black
Host: Department
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Saturday, May 3rd, 2025

Academic Calendar
Study Day
Abstract: *Note: actual end time may vary.*
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Sunday, May 4th, 2025

Academic Calendar
Exams
Abstract: *Note: actual end time may vary.*
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