On August 27, 2024, scholars, trustees, and friends of UConn gathered at the University of Connecticut School of Law to honor members of the university community elected to the National Academies of Sciences, Engineering, and Medicine. Established by an Act of Congress in 1863, the National Academy of Sciences was followed by the National Academy […]
Dear Friends of UConn Physics, Last year, I wrote to you as a new Interim Head of Physics and only barely a month into my appointment. During the past year, we conducted a search for a permanent head and I was selected. For this, I am very grateful for the trust and support I received […]
Every year, the American Physical Society (APS) sponsors CU*IP – Conference for Undergraduate Women and Gender Minorities in Physics – at several locations around the country. This year, led by Prof. Nora Berrah, UConn Physics applied to host this national conference in Storrs and our proposal was accepted for January 24-26, 2025! The purpose of […]
Lawrence “Larry” Kappers, passed away on Friday, August 2, 2024. Professor Lawrence (Larry) Kappers (aka “Kap”) retired in 2009, having joined the UConn Physics Department in 1973. After receiving his Ph.D. from the University of Missouri-Columbia and completing postdoctoral appointments at the University of Minnesota and Oklahoma State University, he developed an active research program […]
The UConn STARs group visited Hartford Public High School (HPHS) to teach physics for a total of eight class periods from May 6th-9th, 2024. UConn brought 16 undergraduate students from the STARs program to HPHS for our annual outreach program, during which we interacted with about 100 high school students. We collaborated with physics teacher […]
Prof. Anh-Thu Le, Department of Physics, University of Connecticut
Following electron-nuclear dynamics with ultrafast intense lasers
Recent progress in laser technology has led to new coherent light sources that can be used to investigate ultrafast processes in matter. To take advantage of these new light sources, different experimental techniques have been developed to reveal the inner-workings of coupled electron-nuclear dynamics in molecules. Concurrently, theoretical and computational tools have also been developed to understand and decode hidden information from experimental measurements. In this talk, I will present our group’s recent progress in understanding intense laser-atom/molecule interactions by using some of the most promising techniques such as laser-induced electron diffraction, high-harmonic generation spectroscopy, and attosecond transient absorption spectroscopy. I will also address the challenges and opportunities in this field for practical realization of molecular “movies” with atomic resolution in space and time that can provide new insights into fundamental chemical reactions.
I will describe some of the background that led to the award of the Nobel prize to Dr. Adam Riess, who will be our 2024 Katzenstein speaker on November 15.
ASTRA: A Transition-Density-Matrix Approach to Time-Resolved Molecular Ionization
Attosecond science, which investigates the time-resolved correlated motion of electrons in atoms, molecules, and solids, is rapidly advancing toward larger molecular systems and more complex processes, such as multiple ionization and molecular fragmentation. Theoretical methods capable of addressing both multiple excitations and photofragment entanglement are essential to capture these phenomena. Among the most promising theoretical approaches are ab initio wave-function-based close-coupling (CC) methods, increasingly adopted by the AMO community.
Despite significant progress from codes like XCHEM [1,2], tRecX [3], RMT [4], and UKRmol+ [5], scaling remains a major challenge – whether in handling ionic correlation, accounting for many atoms, or for distant fragments. To address these limitations, we developed ASTRA [6] (AttoSecond TRAnsitions), an ab initio CC molecular ionization code based on high-order transition density matrices between correlated ionic states of arbitrary multiplicity [7], and hybrid Gaussian-B-spline integrals [5,9]. ASTRA integrates multiple state-of-the-art codes, such as DALTON [8], a general-purpose quantum chemistry code, LUCIA [7], a large-scale CI code, and GBTOlib [5], a hybrid integral library suited for slow photoelectrons and comparatively small molecules.
ASTRA has successfully reproduced total and partial photoionization cross sections, photoemission asymmetry parameters, and molecular-frame photoelectron angular distributions for molecules such as N 2 , CO, H 2 CO, and Pyrazine, showing excellent agreement with existing benchmarks. Currently, ASTRA is being applied to study attosecond transient absorption spectra of CO and O 2 , as well as sequential XUV-pump IR-probe ionization of C 2 H 4 . Its formalism naturally extends to molecular double ionization and can efficiently model electron exchange between multiple disjoint molecular fragments − relevant for describing ionization in weakly bound clusters like (H 2 O) n .
Looking ahead, continued integration with tools tailored to high-energy photoemission, non-adiabatic nuclear dynamics, and strong fields ionization will be critical for addressing emerging challenges in ultrafast many-body dynamics. Free-electron lasers enable time-resolved studies of core ionization, while table-top attosecond pump-probe experiments are targeting increasingly larger molecules, monitoring both electron dynamics and nuclear rearrangements throughout chemical reactions with intense probe pulses [10]. To reproduce these complex experiments, we are collaborating with NIST to replace GBTOlib with a more efficient hybrid library capable of handling larger molecules and higher orbital angular momenta. We are also pairing ASTRA with surface-hopping methods [11], where multiphoton ionization is typically not available. Additionally, to track the asymptotic evolution of weakly coupled photofragments under strong light fields − without incurring prohibitive computational costs − we are considering integrating separate optimized propagators for each fragment, which will open the door for us to simulate strong-field multichannel molecular-ionization processes.
[1] M. Klinker et al., J. Phys. Chem. Lett. 9, 756 (2018).
[2] V. J. Borràs et al., Science Advances 9, eade3855 (2023).
[3] A. Scrinzi, Comput. Phys. Commun. 270, 108146 (2022).
[4] A. C. Brown et al., Comput. Phys. Commun. 250, 107062 (2020).
[5] Z. Masin et al., Comp. Phys. Commun. 249, 107092 (2020).
[6] J. M. Randazzo et al., Phys. Rev. Res. 5, 043115 (2023).
[7] J. Olsen et al., J. Chem. Phys. 89, 2185 (1988); ibid. 104, 8007 (1996).
[8] K. Aidas et al., Comp. Mol. Sci. 4, 269 (2014).
[9] H. Gharibnejad et al., Comp. Phys. Commun. 263, 107889 (2021).
[10] F. Vismarra et al., Nature Chemistry (2024).
[11] L. Fransén et al., J. Phys. Chem. A 128, 1457 (2024).
A New Era for Connecticut’s Oldest Planetarium: Historic Roots to Modern Revival
The UConn Planetarium, built in 1954, has long been a central resource for astronomy education and outreach at the University of Connecticut. In this talk, I will present an overview of the planetarium’s historical roots at UConn, its significance in the community, and the extensive renovations we have completed to bring this important facility back to life. After years of disuse, the planetarium has been fully upgraded with modern technology and will officially reopen on November 1st, immediately following this colloquium.
Our efforts to restore the planetarium are guided by the legacy of Dr. Cynthia Peterson, UConn’s first woman physics faculty member and a pioneer in science education. The planetarium now officially bears her name as the Cynthia Wyeth Peterson Memorial Planetarium, in honor of her decades of dedication to astronomy outreach. Following my presentation, Nora Berrah and Celeste Peterson will speak about Dr. Peterson’s life and achievements - how her contributions to UConn and the wider scientific community continue to resonate today.
Prof. Moshe Gai, Department of Physics, University of Connecticut
Concepts of Stellar Evolution
Star are born, they evolve to a mature midlife and sooner or later die, some in an amazing last display. We will discuss how star reveal the stages of Stellar Evolution and what makes them tick. We will also seek feedback on the need for such a graduate class at UConn.
The search for anyons, quasiparticles with fractional charge and exotic exchange statistics, has inspired decades of condensed matter research. Moreover, it has been predicted that exchange braiding of these particles, especially non-abelian anyons, can produce topologically protected logic operations that can serve as building blocks for fault-tolerant quantum computing. In this talk, I will discuss the progress of research on two quantum materials platforms to realize these exotic particles. In the first example, we will discuss anyons arising in fractional quantum Hall (FQH) effects, using quantum Hall interferometers for direct observation of the anyon braiding phase around a confined cavity. In the second example, we will discuss our recent experimental efforts to realize non-abelian anyons in proximitized topological insulator surfaces by controlled manipulation of magnetic vortices containing non-abelian anyons.
Jacob Heeren is a data analyst at Collins Aerospace, where he supports both commercial and military operations. His responsibilities span the entire data pipeline, encompassing data engineering, visualization, analytics, and governance across diverse projects. He holds degrees in psychology and applied mathematics from Iowa State University, with additional studies in astrophysics at the University of Iowa. Outside of his professional role, Jacob enjoys rock climbing and creating music, reflecting his passion for both physical and creative pursuits. Jacob will discuss his career path, current role, and useful skill sets for data science positions
Profs. Xian Wu and Erin Scanlon and Matt Guthrie, Department of Physics, University of Connecticut
An Introduction to Physics Education Research
Physics education research (PER) is a subfield of physics that focuses on investigating questions such as: 1) how can we teach physics better?; 2) how do students learn physics?; and 3) how can we make the physics community more inclusive, equitable, and diverse? In this talk, we will give an introduction to PER, including common misconceptions, methods, and the PER happening at UConn.
Román Fernández Aranda, Department of Physics, University of Crete and FORTH Institute of Astrophysics, Greece
A Burning Hot DOG: The extreme ISM conditions of the most luminous obscured galaxy in The Universe
Hot dust-obscured galaxies (or Hot DOGs) are a remarkable population of high-redshift galaxies. Hot DOGs harbor hyper-luminous supermassive black holes (SMBHs), which are believed to provide strong feedback, creating extreme conditions in the interstellar medium (ISM) of their host galaxies in recurrent episodes of strong accretion and heavy obscuration. W2246-0526 is a Hot DOG at redshift 4.6 and the most luminous obscured galaxy known to date. I will present ALMA observations of both the brightest far-IR fine-structure emission lines and their underlying dust continuum, combined with ISM modeling of the gas and the dust. This work sheds light on the extreme conditions galaxies can experience during the early stages of the Universe, which is critical to our understanding of how distant and young galaxies evolve.
Prof. Shohini Bhattacharya, Department of Physics, University of Connecticut
Exploring the Cosmic Core of Nucleons with the Electron-Ion Collider
Have you ever wondered what holds the universe together at its most fundamental level? The answer lies in Quantum Chromodynamics (QCD), the theory that describes how quarks and gluons—collectively known as partons—interact to form nucleons, the protons and neutrons that make up all visible matter. Despite our understanding of QCD, the inner workings of partons remain one of the most profound mysteries in physics. How do they move? How do they contribute to a nucleon’s spin and structure? The Electron-Ion Collider (EIC), a cutting-edge facility soon to be operational, is poised to address these profound questions. In this talk, I will take you on a journey into the “cosmic core” of nucleons and explain how the EIC, like a super-powered microscope, will enable us to peer deep inside protons and neutrons, unveiling the dynamics of partons. I will focus on one of my key research projects aimed at unraveling the nucleon spin puzzle using the capabilities of the EIC. But the excitement doesn’t end there. Advancing our understanding of QCD not only helps us probe nucleons but also allows us to test the Standard Model of particle physics, our most comprehensive theory of the universe. Together, we will explore the far-reaching implications of this research field.