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Department of Physics & Astronomy

Department of Physics & Astronomy

Physics & Astronomy

Learn About the Department

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FRIB Apparatus
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

  • An image of Earth against a backdrop of stars with the text From Earth to the Universe
    A Night at the Planetarium: From Earth to the UniverseOctober 3, 2025
  • Students stand in front of the Nielsen Physics Building on the University of Tennessee, Knoxville, campus
    Open Faculty SearchesOctober 3, 2025
  • A student describes her poster at the Vertex 2025 workshop
    Vertex 2025 Comes to Rocky TopSeptember 30, 2025
See All News
See Our Media Mentions

Colloquium Schedule

Introduction to DAMSA, A Novel Dark Messenger Search Experiment at an Accelerator

October 13, 2025

Speaker: Jaehoon Yu

Host: Tova Holmes

Abstract

Dark matter is thought to make up 25% of the universe. Dark sector particles (DSP) do not interact through the known forces but could be weakly coupled to Standard Model particles through a portal or a mediator (Dark Messenger) that could provide access to the dark matter world. Many searches for these particles at an accelerator thus far seem to face a ceiling that the sensitivity reach is greatly limited, beyond statistical effects. DAMSA (DArk Messenger Searches at an Accelerator) is an extremely short baseline, table-top scale experiment that aims to break through this limit. The experiment plans to take advantage of high beam powers available at various accelerator facilities around the world, including the PIP-II LINAC under construction at Fermilab near Chicago, an essential element in providing the necessary high flux proton beams to the $3.5B U.S. flagship neutrino experiment, DUNE. In this talk, I will describe the DAMSA experiment and discuss the current status and plan for DAMSA, as well as its expected sensitivity reach on the search of the Axion-Like Particle, a dark messenger, as a benchmark physics case.

The Physics of Bacterial Cell Shape and Size

October 20, 2025

Speaker: Sven van Teeffelen, Université de Montréal

Host: Jaan Mannik

Abstract

All living cells are bounded by envelopes that protect them from the environment and confer their sizes and shapes. These shapes help cells to spatially organize their internal biological processes, allowing them to divide and faithfully segregate genetic material to each daughter. Yet, we still know very little about how cells obtain and control cell shape, even in the arguably simplest and best understood organism: the rod-shaped Escherichia coli. To resist a high intracellular osmotic pressure, bacteria and many other single-celled organisms are surrounded by a cell wall, an elastic, covalent meshwork of sugars and peptides. For walled cells to grow, they must enzymatically cut cell-wall bonds while inserting new cell-wall material to prevent envelope rupture. In some bacteria and many fungi and plants, the process of cell-wall remodeling is limited to the tip of the cell, where intracellular pressure and enzymatic cell-wall fluidization drive growth of the rod, akin to glass blowing. However, in E. coli and many other rod-shaped bacteria, cell-wall remodeling happens all along the cylindrical part of the cell, while the poles remain inert (new poles being constructed at mid-cell during division). How do cells control a straight rod-like cell geometry with a well-defined diameter, all the while increasing cell length at a rate that accommodates biomass growth? While the ultimate answers to these questions remain to be found, we have made important progress in the past two decades. For example, i) curved cytoskeletal polymers sense cell-envelope curvature and reenforce cylindrical geometry, ii) mechanical stress affects envelope growth locally, and iii) the ratio between cell-surface area and biomass emerges as a controlled variable, thus coupling the global rate of envelope growth to the rate of biomass growth. I will present these and other findings, illustrate the importance of experiments and theory, and present future directions.

Physics Colloquium: TBA

October 27, 2025

Speaker: TBA

Abstract

TBA

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AAAS, The American Association for the Advancement of Science, Logo
APS, American Physical Society, logo

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

Departmental Honors

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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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