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Department of Physics & Astronomy

Department of Physics & Astronomy

Physics & Astronomy

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A physics student work at CERN

Welcome!

Physics and Astronomy at the University of Tennessee, Knoxville, is where fascination meets function. We explore the deep questions of the universe and provide the scientific foundation for discovery that yields the technologies in your pocket, and those of tomorrow.

Our department is driven by an engaged faculty pursuing fundamental research and eager to develop the next generation of scientists.

Our physicists helped put our state on the periodic table, study multi-messenger astronomy and explosive stellar events, and search for new physics at CERN. They describe the properties of nuclei and neutrons and test the limits of superconductivity with new models and novel materials. They merge physics and biology at the cellular level with lab-on-a-chip devices. They’re building an interdisciplinary approach to lead transformative research on quantum materials and devices, information science, and artificial intelligence.

Our students have a breadth of research opportunities on campus, at nearby Oak Ridge National Laboratory, and at facilities all over the world to set them on the path to promising careers.

Learn More About What Sets Us Apart

Department News

  • signal:noise advertisement for February 19 DJ and VJ show at Fly by Night
    Physics After DarkJanuary 30, 2026
  • A photo of Dien Nguyen
    How Spin Shapes the WorldJanuary 15, 2026
  • An etched translucent sign in green reading cosmicrayn, seeing the unseen
    Cosmic Collaboration: Students Join Forces to Bring the Invisible to LifeDecember 16, 2025
See All News
See Our Media Mentions

Colloquium Schedule

Hybrid Magnon–Phonon Excitations in Quantum Magnets

February 16, 2026

Speaker: Xiaojian Bai, Louisiana State University

Host: Haidong Zhou

Abstract

Magnons and phonons are collective excitations in crystals that often behave as independent quasiparticles when their mutual coupling is weak. When magnetoelastic coupling becomes strong, interactions between spin and lattice degrees of freedom can open gaps at band crossings and give rise to hybridized excitations known as magnon-polarons. Because such hybridized modes appear only when energy matching, symmetry compatibility, and microscopic coupling all align, their presence and momentum dependence provide a particularly sensitive probe of the underlying spin–lattice interactions.

In this talk, I will use the olivine-type silicate Co₂SiO₄ to illustrate how this physics plays out in a real material. I will begin by presenting inelastic neutron-scattering measurements that reveal a rich set of hybridized excitations involving magnons, phonons, and spin–orbit excitons. To understand these observations, I will introduce an effective spin Hamiltonian that captures the main features of the magnetic excitations and discuss density functional theory calculations that reproduce the phonon spectrum. Building on these microscopic descriptions, a symmetry analysis of the magnon and phonon modes reveals which excitations can hybridize and where in momentum space such coupling is allowed. This framework naturally leads to a minimal hybridization model that explains the observed avoided crossings and mode mixing, providing a unified picture of the hybridized excitation spectrum in Co₂SiO₄.

More broadly, this work establishes olivine-type oxides as a clean setting for studying magnetoelastic coupling and illustrates how combining dynamical measurements with symmetry-based modeling can reveal microscopic interactions that are difficult to access otherwise.

The Muon Magnetic Moment with Lattice QCD

February 23, 2026

Speaker: Luchang Jin, University of Connecticut

Host: Chien-Yeah Seng

Abstract

The magnetic moment of muon can be characterized by its gyro-magnetic factor $g$, which is numerically close to 2. Fermilab announced a new experimental result for muon $g-2$ on June 3, 2025.
The new result is consistent with the previous BNL measurement, but with about 4 times higher precision. For the Standard Model prediction, the recent theoretical muon $g-2$ white paper was released on May 27, 2025. The new theory result is consistent with the new experimental result, but is about 3 sigma larger than the previous theory white paper result, released on June 8, 2020. Two hadronic contributions, HVP (hadronic vacuum polarization) and HLbL (hadronic light-by-light), are the dominant sources of the theoretical uncertainty. The change in the central value is largely due to the many advances in lattice QCD calculations of these hadronic contributions, particularly the HVP contribution. In this talk, I will describe the theoretical determination of muon $g-2$ with focus on the lattice QCD calculations of the hadronic contributions.

Sowjanya Gollapinni, Los Alamos National Laboratory

March 2, 2026

Speaker: Sowjanya Gollapinni

Host: Stefan Spanier

Abstract

TBA

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Our faculty includes 4 fellows of the American Association for the Advancement of Science and 10 fellows of the American Physical Society.

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Physics & Astronomy

College of Arts and Sciences

401 Nielsen Physics Building
1408 Circle Drive
Knoxville TN 37996-1200
Phone: 865-974-3342
Email: physics@utk.edu

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The University of Tennessee, Knoxville
Knoxville, Tennessee 37996
865-974-1000

The flagship campus of the University of Tennessee System and partner in the Tennessee Transfer Pathway.

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