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. 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.
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.
Last year’s Nobel Prize in Physics was awarded to Pierre Agostini, Anne l’Huillier, and Ferenc Krausz, for discoveries that launched attosecond science and technology at the turn of the century, before there were any x-ray free electron lasers. Subsequent advances at SLAC as well as other labs around the world helped to establish the breadth and importance of research at the attosecond frontier, making the case for Nobel recognition of the foundational work. This illustrates how technological advances and fundamental discoveries feed on each other: advances in ultrafast lasers are quickly followed by fundamental discoveries in physics, which then motivate further advances in laser technology. This colloquium is an eyewitness account of that story from its beginnings four decades ago to the present. I’ll describe the science behind the Prize, and I’ll explain how x-ray lasers have become a central focus for the next chapter of the saga.
Reception preceding at 3pm in the Gant Light Court
Prof. Lea Ferreira dos Santos, Department of Physics, University of Connecticut
Nonequilibrium Quantum Dynamics
Santos’s group uses numerical and analytical methods to understand, predict, and control the dynamics of quantum systems taken far from equilibrium. This talk will present two lines of research of the group. (i) The characterization of quantum systems with many interacting particles, the timescales for their relaxation process, and the conditions for reaching thermal equilibrium. (ii) The use of the quantum-classical correspondence to better understand and make use of static and dynamical properties of transmon qubits, which are the predominant element in circuit-based quantum information processing.
How to Make a Faster Trapped-Ion Quantum Computer?
Trapped ions offer a pristine platform for quantum computation, but enhancing the interactions without compromising the qubits remains a crucial challenge. In this talk, I will present a strategy to enhance the interaction strengths in trapped-ion systems via parametric amplification of the ions’ motion, thereby suppressing the relative importance of decoherence. We illustrate the power of this approach by showing how it can improve the speed and fidelity of two-qubit gates in multi-ion systems and how it can enhance collective spin states useful for quantum metrology. Our proposal has been further demonstrated in the experiment, confirming the enhancement. Our results open a new avenue of phonon modulation in trapped ions and are directly relevant to numerous other physical platforms in which spin interactions are mediated by bosons.
Prof. Peter Schweitzer, Department of Physics, University of Connecticut
Internal Structure of Hadrons
Hadrons are composed particles and exhibit a rich internal structure which is probed experimentally in high energy experiments and described in the theory of Quantum Chromodynamics. Recent advances in the theory of hadron structure with focus on gravitational form factors are discussed.
Dr. Eric Koch, Harvard Smithsonian Center for Astrophysics
Revealing the multi-phase neutral interstellar medium’s role in the star formation lifecycle: a sharpened view of nearby galaxies from LGLBS and PHANGS-JWST
The neutral interstellar medium (ISM) fuels the star formation lifecycle, yet we still lack vital constraints on the formation and destruction of molecular clouds because of challenges in observing the cold neutral ISM phases with high resolution and sensitivity. With dedicated surveys, the combination of VLA, ALMA, and JWST can now make significant advances in the coming years. In this talk, I will present multiple observational approaches that are making progress in this area: detailed 21-cm HI VLA mapping across the Local Group from the Local Group L-band Survey (lglbs.org), resolved molecular cloud studies with ALMA and JWST in M33 and PAH imaging from PHANGS-JWST as a highly sensitive resolved view of the total neutral gas tracer (phangs.org). These surveys bridge Galactic with extragalactic star formation studies and provide new constraints to guide the next generation of numerical simulations.
Prof. Simone Colombo, Department of Physics, University of Connecticut
Observing our Universe with Quantum Sensors
In this seminar, we will introduce the application of atomic, molecular, and optical (known as AMO) physics to the field of quantum metrology. We will show how atoms are used as probes of our universe and how to harness quantum effects to enhance their sensing capabilities.
We will then focus on a specific type of atomic sensor and one of our research interests: optical atomic clocks. Building upon recent results, we will illustrate how optical clocks’ performances can be pushed beyond current limitations and how they can be/are deployed to get a better glimpse of the inner workings of our universes. In this framework, we will highlight the research activities that we are currently pursuing in our lab. Crucially, we will attempt to give a perspective on the life of an AMO physicist.
Bi-polaron superconductivity in the low density limit
It has been assumed for decades that high values of Tc from the electron-phonon coupling are impossible. At weak-to-intermediate coupling strength this result follows from the Migdal-Eliashberg theory, while at strong coupling, when bipolarons form, the transition temperatures are low because of the exponential effective mass enhancement. However, the latter conclusion was based on numerical solutions of the Holstein model. I will discuss a different model with coupling based on the displacement modulated hopping of electrons and argue that much larger values of the bipolaron Tc can be achieved in this setup. Non-locality of the problem gives rise to small-size, yet relatively light bipolarons, which can be studied by an exact sign-problem-free quantum Monte Carlo approach even in the presence of strong Hubbard and Coulomb potentials. We find that Tc in this model generically and significantly exceeds typical upper bounds based on Migdal-Eliashberg theory or superfluidity of Holstein bipolarons, and, thus, offers a route towards the design of high-Tc superconductors via functional material engineering. Finally, there are indications for even better prospects in systems with non-linear electron-phonon coupling.