Physicist Brings High Energy to UMD With Laser-Made Plasmas

Will Fox credits his early research experiences with introducing him to the power of plasma, a state of matter that could overhaul the energy sector and demystify astrophysical phenomena like cosmic rays and solar flares.

As an undergraduate researcher at Princeton University, Fox joined the Princeton Plasma Physics Laboratory (PPPL), a U.S. Department of Energy lab where he would later work for 11 years, including most recently as a principal research physicist. There, Fox played an integral role in developing experiments that used lasers to produce extremely hot and dense plasmas in the lab—no space telescope needed.Will Fox. Credit: Sarah Jane WhiteWill Fox. Credit: Sarah Jane White

Fox was captivated by the many applications of this research, including the potential to unlock fusion as an alternative energy source and advance the scientific community’s understanding of plasma physics at a fundamental level. 

“Research on laser-produced plasmas has been going on since the ’60s, and what’s exciting about these experiments is that they’ve come up with clever ways to measure what’s happening in the plasma produced,” Fox said. “In doing these experiments, you get to leverage all those developments that have happened over the years.”

In January 2025, Fox joined the University of Maryland as an assistant professor of physics. He’s refurbishing a lab in the Energy Research Facility, which will include a high-powered laser that allows him to produce plasmas on campus without needing to travel to other institutions. The lab will also feature a vacuum chamber and a control room, allowing researchers and collaborators from other institutions to work in a separate area from the laser.

“The physics department has an excellent group of faculty and a lot of expertise to help you set up a lab,” Fox, who holds a joint appointment in UMD’s Institute for Research in Electronics and Applied Physics, said of what attracted him to UMD. 

Magnetically drawn

Despite being the most common state of matter in the universe, plasma is perhaps the least understood. Its free-flowing, negatively charged electrons and positively charged ions make it an efficient conductor of electricity. Its presence on Earth can be seen in lightning strikes, and in space, it contributes to processes such as magnetic reconnection (as seen in solar flares) and collisionless shocks (whose waves propel cosmic rays to nearly the speed of light).

Fox has devoted his career to studying these complex processes and sharing what he’s learned with students. After graduating from Princeton with a bachelor’s degree in physics in 2001, he took a gap year to seize a once-in-a-lifetime opportunity: a math and physics teaching position at a high school in Nepal’s capital through the Princeton in Asia fellowship program. During his year in Kathmandu, Fox spent weekdays in the classroom and weekends in the Himalayas.

“I got into mountain biking and went on hikes,” Fox recalled fondly. “Just being immersed in the culture was exciting, and there was always something new or interesting going on in the city.”

When his fellowship ended, Fox enrolled in MIT’s physics Ph.D. program and focused on magnetic reconnection, a process that occurs in plasma and converts magnetic energy into kinetic energy. This concept is crucial for understanding Earth’s magnetized bubble of plasma, known as a magnetosphere; the aurora phenomena seen near Earth’s poles; and processes related to the sun, including coronal mass ejections and solar flares. 

Magnetic reconnection can also cause problems when it occurs spontaneously in fusion devices used to generate energy. To better understand the phenomenon, Fox contributed to experiments that enabled magnetic reconnection to unfold in a controlled setting.

“Reconnection is one way the plasma can break out of the magnetic field that's trying to hold it in place,” Fox explained. “The idea is that by understanding how reconnection works, you can maybe design a better fusion device or understand what you have to do to keep things contained and in control.”

Finding purpose in plasma

After earning his Ph.D. in 2009, Fox spent two years as a research scientist at the University of New Hampshire’s Space Science Center, where he helped develop a program called the Plasma Simulation Code to see how plasma particles would interact with magnetic and electric fields in a virtual environment. Later, at PPPL, he used this same code to study how laser-produced plasmas might replicate astrophysical phenomena

While Fox enjoyed this modeling work and found that it helps researchers design better experiments, he prefers producing actual plasmas in the lab.

“I still think of myself, ultimately, as an experimental physicist,” Fox said. “At the end of the day, I get excited about seeing a result and real data in a physical experiment.”

After Fox joined the PPPL as a physicist in 2013, he developed experiments with laser-produced plasmas that surpassed temperatures of 30 million degrees Fahrenheit. He also led the first experimental observations of the ion Weibel instability, a process that can spontaneously generate a magnetic field in plasma. Understanding this process can help researchers tackle one of the biggest unanswered questions in his field: how plasmas across the universe generate magnetic fields.

“When we look out at the cosmos, almost all of the plasma that's out there has a magnetic field,” Fox said. “You can look at the polarization of light that’s coming from a galaxy and see that there must be some large magnetic field embedded in the plasma. So overall, it's a question of, ‘Where did this magnetic field come from in the first place?’”

In later studies, Fox used plasma and a static magnetic field to generate collisionless shocks, which are comparable in some ways to the shockwaves that ripple off airplanes flying faster than the speed of sound. He also developed an improved method of measuring magnetic fields in plasma, resulting in a higher degree of accuracy.

In recognition of these discoveries, Fox received two awards from the American Physical Society: a 2019 Thomas H. Stix Award for Outstanding Early Career Contributions to Plasma Physics and a 2020 John Dawson Award for Excellence in Plasma Physics Research. 

Fox has published more than 80 research papers throughout his career and is gearing up for many more at UMD. Currently, he is using laser-produced plasmas to take a closer look at magnetic reconnection. 

“We are colliding two plasmas with magnetic fields together and then using these techniques to measure how the plasma is behaving, where they're interacting and where the reconnection is happening,” Fox said.

Going forward, Fox plans to collaborate on experiments with Distinguished University Professor of Physics Howard Milchberg, whose lab is also located in the Energy Research Facility and is equipped with a short pulse laser. 

“Our vision is that we'll have these cooperative experiments where the laser in my lab will produce the plasma state, and then we can take different types of probe measurements using the short pulse laser,” Fox said. “I’m looking forward to running more experiments and collaborating with the faculty and students here.”


Written by Emily Nunez

Summer at Summit Station

For most graduate students, research trips primarily mean conferences. For Aishwarya Vijai, it meant a month at Summit Station, Greenland, deep inside the Arctic Circle. Summit Station is located near the apex of the Greenland ice sheet at an elevation of ~10,000 feet above sea level. The station hosts scientists from collaborations around the world to conduct experiments on and with the Greenland ice sheet. One such collaboration is the Radio Neutrino Observatory in Greenland (RNO-G), a next-generation, ultra-high energy (UHE) neutrino detector. RNO-G sends teams of 4-5 people to help build the detector, and this year, these teams included a student from UMD: Aishwarya, a fourth-year graduate student in the physics department. Aishwarya works with Assistant Professor Brian Clark. The team flew to Summit Station via miltary aircrafts called LC-130s from Kangerlussuaq, a small town in Western Greenland. They stayed at Summit Station for a month to do maintenance work and collect data for calibration purposes. 

From Summit Station, the RNO-G detector, which is spread out over multiple locations (“stations”) on the ice sheet, is accessed via snow machines. Primary work done by this year included raising structures like solar panels and wind turbines which are used to power the detector. This involved a lot of shoveling to remove the drifting snow and attaching extensions to the bases of these structures to raise their heights. In addition, the team collected critical data to better understand the detector’s performance. This was achieved by campaigns where antennas were lowered hundreds of feet into the ice sheet. 

Summit Station has a maximum capacity of 40 people and operates 6 days a week with Sundays off. The biggest building on station is the aptly named Big House, a common area for meals, bathrooms, showers and entertainment in the form of books and board games. Food is prepared on station by a chef 6 days a week with leftovers on Sundays. Additional amenities include a gym, a recreational tent with a projector for watching movies, and a sauna. Sleeping accommodations are in the form of fish huts (small hard-sided structures for 1 person), the Flarm and the Caboose (hard-sided structures for 6-8 people). 

Temperatures at Summit Station typically fluctuate around -10 degrees Fahrenheit with wind chill, with occasional storms generating wind gusts of up to 50 mph. All people on Summit Station are equipped with winter gear to handle extreme weather. The station is located within the Arctic Circle so the sun doesn’t set in the summer until the beginning of August. The constant sunlight reflecting off the ice sheet leads to a high albedo. Sunglasses are worn outside at almost all times. 

Summit Station and the surrounding ice sheet was an incredible place to visit. The ice sheet is extremely beautiful and vast, appearing almost infinite in size. There are also several cool phenomena that can be observed on the ice sheet, like sun dogs and halos, which are produced when sunlight refracts through the ice crystals in the atmosphere. Sunsets at Summit Station saturate the sky in shades of red and yellow that appear even brighter in contrast to the white surroundings. The community at Summit Station also made the experience incredible, turning a nearly inhospitable place into the place to be for an experience of a lifetime. 

The Greenland ice sheet is one of the only places in the world where a UHE neutrino observatory like RNO-G can be built. The collaboration as a whole looks forward to returning next year and continuing work building the detector and hopefully using it to elevate our understanding of the universe at the highest of energies. 

More About RNO-G

The Radio Neutrino Observatory in Greenland (RNO-G) is a UHE neutrino telescope located at Summit Station, Greenland. The detector aims to find UHE neutrinos potentially emitted from energetic phenomena in the universe like black hole mergers and supernovas (explosions of stars). The detector is currently under construction and the University of Maryland (UMD) is a major construction site. Currently, the RNO-G group at UMD has built nearly 250 antennas. These antennas are the primary detection unit of RNO-G and aim to find the broadband radio pulse that is produced when UHE neutrinos interact with ice.

The fully completed detector will have 35 stations spaced 1 km apart to create an array. Each station will be equipped with 24 antennas buried in the Greenland Ice Sheet in drilled holes ~100 meters in depth. 8 stations have been built so far.

 

Jacob "Bob" Dorfman, 1937-2025

Professor Emeritus Jacob Robert Dorfman died on August 27, 2025. A native of Pittsburgh, Dorfman grew up in Baltimore and received his bachelor’s degree and doctorate at Johns Hopkins University. After three years of post-doctoral research at the Rockefeller University, he was appointed a UMD assistant professor in physics. During his time in College Park, he served as the Director of the Institute for Physical Science and Technology, Dean of the College of Computer, Mathematical and Physical Sciences, and Vice President for Academic Affairs and Provost, returning to teaching and research in 1992. He retired as an emeritus professor in 2005.

"The entire University of Maryland community extends its deepest condolences to Dr. Dorfman's family, friends and colleagues,” said UMD President Darryll J. Pines. "Dr. Dorfman's contributions to the university were substantial and wide-ranging, from serving as a dean and as provost to chairing a committee focused on improving student academic outcomes. He played a critical role in laying the foundation for our institution to achieve excellence, and we are grateful for all he did to advance the university.”

Dorfman enjoyed visiting professor appointments at the University of Utrecht, Rockefeller University and The Technion in Haifa, Israel.  He is the author of over one hundred scientific papers and books on statistical thermodynamic and chaos theory. His most recent book, Contemporary Kinetic Theory of Matter, written with Henk van Beijeren and T. R. Kirkpatrick, was published in 2021.

In addition to his scientific work, Dorfman studied art history, specializing in 17th century Dutch art, and continued to serve on thesis committees in recent years.

A memorial service is planned for Sunday, Aug. 31 at 10 a.m. at Temple Micah, 2829 Wisconsin Ave. NW

 

Faculty, Staff, Student and Alumni Awards & Notes

Follow us on LinkedIn: https://www.linkedin.com/company/umdphysics 

 

Faculty and Staff 
Students
  • Dhruv Agarwal and Hannah McCright received CMNS Alumni Network Endowed undergraduate awards.
  • Isabella Giovannelli was quoted in Physics.
  • Rodrigo Andrade e Silva and Saketh Muddu received the Charles W. Misner Award in Gravitational Physics.
  • Rajrupa Mondal and Zhaohui Xu received the Joseph and Dorothy Sucher Graduate Prize in Physics.
  • Iman Ahmadabadi and Jeffery Yu received the Thomas Mason Interdisciplinary Physics Award.
  • Sagnik Mondal, Kushan Panchal, Alexandra Behne and Greeshma Oruganti received the Charles T. Husar Fellowship in Physics.
  • Shuzhe Zeng received the Leon A. Herreid Science Fellowship.
  • Aishwarya Vijai spent the summer at Summit Station in Greenland.
Alumni
  • Susan Holcomb (B.S., '10) won the 2023 Cupboard Pamphlet Contest for her book Wolfbaby.

In Memoriam

It is with much sadness that the Department of Physics announces the passing of members of our community.

  • Roger Dean Bengtson (Ph.D., 1968) died in May, 2023. He researched plasma physics at the University of Texas for 46 years.
  • Bob Dorfman, a Professor Emeritus and former Dean and Provost, died August 27, 2025.
  • John Gonano, a former tutor in the Slawsky Clinic, died this spring. During his career, he worked for NIST and for the Army Research Lab.
  • Gary Wilson Phillips (Ph.D., 1967), died on July 7, 2025. After a career at the Naval Research lab, he held an adjunct position at Georgetown University.
  • Andrew C. Victor, who worked as a physicist in rocket propulsion after receiving his master's degree at UMD, died on July 18, 2025.
  • Frank C. Young (Ph.D., 1962), died on August 1, 2025. After receiving his doctorate, he worked for 10 years in the UMD Cyclotron before joining the Naval Research Lab.