Advocating for Quantum Simulation of Extreme Physics

The Big Bang, supernovae, collisions of nuclei at breakneck speeds—our universe is filled with extreme phenomena, both natural and human-made. But the surprising thing is that all of these seemingly distinct processes are governed by the same underlying physics: a combination of quantum mechanics and Einstein’s theory of special relativity known as quantum field theory.

Theoretical nuclear and particle physicists wield quantum field theory in their efforts to understand interactions between many particles or the behavior of particles with extremely large energies. This is no easy feat: At least theoretically, quantum field theory plays out in an infinite universe with particles constantly popping in and out of existence. Even the world’s biggest supercomputer would never be able to model it exactly. Fortunately, there are many computational tricks that can make the problem more tractable—like cutting up the infinite universe into a finite grid and taking judicious statistical samples instead of tracking every parameter of every particle—but they can only help so much. 

Over the past few years, a growing group of scientists has become wise to the potential of quantum computers to approach these calculations in a completely new way. With a fully functioning quantum computer, a lot of the approximations could be avoided, and the quantum nature of the universe could be modeled with true quantum hardware. However, quantum computers are not yet big and reliable enough to really tackle these problems, and the algorithms nuclear and particle physicists would need to run on them are not yet fully developed.

“Even if we have large-scale, fully capable quantum computers tomorrow,” said Zohreh Davoudi, associate professor of physics at UMD, “we don’t actually have all the theoretical tools and techniques to use them to solve our grand-challenge problems.”Zohreh Davoudi

Classical computers require exponential resources to simulate quantum physics. To simulate one extra tick of the clock or include one extra particle, the amount of computing power must grow significantly. So, the classical methods resort to approximations that fall short because they leave out details and lose the ability to address certain kinds of questions. For one, they can’t keep up with the real-time quantum evolution of the early universe. Additionally, they can’t track what happens during collisions of heavy nuclei. And finally, they are forced to ignore the quantum interactions between the myriad particles in high-energy settings, like those that are emitted from an exploding star. A quantum computer, however, could tackle these problems on their own quantum turf, without needing as many resources or resorting to as many approximations.

Now, researchers want to make sure the nascent effort to use quantum computers to simulate the extreme events of the universe continues to thrive. Davoudi, along with JQI Adjunct Fellow and College Park Professor of Physics Chris Monroe and other researchers, penned a whitepaper laying out the case for funding quantum simulation research in particle physics, published in the journal PRX Quantum in May 2023. Davoudi also co-authored a similar whitepaper in the field of nuclear physics, available on the arXiv preprint server.  

“It's a responsibility of researchers to also think at a larger scale,” said Davoudi, who is also a Fellow of the Joint Center for Quantum Information and Computer Science (QuICS) and the associate director of education at the National Science Foundation Quantum Leap Challenge Institute for Robust Quantum Simulation (RQS). “If we think this field is intellectually promising, interesting, and worth investing in as a scientist, we have to make sure that it stays healthy and lively for generations to come.”

Some sub-fields of physics, including the nuclear and particle physics communities, engage in long-term planning for the future of their field. Nuclear physicists in the U.S. plan seven years ahead, and particle physicists plan a full decade ahead. Researchers from many universities and national laboratories come together in meetings, seminars, and panel discussions over the course of a year to decide what the highest priorities in the field should be. Funding agencies in the U.S. and worldwide have historically taken these conclusions seriously. The whitepapers developed by Davoudi and her co-authors are a part of those efforts. In them, they argue for the importance of studying quantum simulation for nuclear and particle physics and make specific recommendations for further development. 

“These new research directions in both nuclear physics and high-energy physics were not part of the last U.S. long-range planning processes, because the idea had simply not been introduced at the time,” Davoudi said.

Indeed, the ideas weren’t even on Davoudi’s radar six years ago when she came to UMD to join the physics faculty as a theoretical nuclear physicist. While she was busy searching for an apartment, Davoudi saw an announcement for a workshop hosted by QuICS exploring the intersection of her field with quantum computing. Instead of looking for a place to live, she spent several days at the workshop, talking to theorists and experimentalists alike. 

Davoudi was enticed by the promise of quantum simulations to solve the kinds of problems she was unable to address with classical computational tools, and it changed the course of her career. In the years since, she has developed new theoretical techniques and collaborated with experimentalists to push the boundaries of what quantum simulators can do to help uncover the basic physics of the universe.

Davoudi wants to ensure that this burgeoning field continues to thrive into the future. In the whitepapers, she and her co-authors identified specific problems where quantum computing holds the most promise. Then, they made three main recommendations to ensure the success of the field for the next seven to 10 years. 

First, they recommended funding for theoretical efforts to develop algorithms that run on quantum hardware. Even though the potential of quantum computing is clear, detailed algorithms for simulating quantum field theory on a quantum computer are still in their infancy. Developing these will require a dedicated effort by the nuclear and particle physics communities. 

Second, they advocated for greater interdisciplinary communication between the nuclear, particle and quantum physics communities. Different quantum computer architectures will have different quirks and advantages, and the field theory folks will need to have access to them to figure out how to make the best use of each one. Certain implementations may, in turn, become motivated to engineer specific capabilities for the kinds of problems nuclear and particle physicists want to study. This can only be accomplished through close interdisciplinary collaboration, the authors claim. 

“As a community, we cannot isolate ourselves from the quantum information and quantum technology communities,” Davoudi said.

Third, Davoudi and her co-authors believe it is key to bring in junior researchers, train them with a diverse set of skills, and give them opportunities to contribute to this growing effort. As with the QuICS workshop that inspired Davoudi, the community should invest in education and training for the relevant skills through partnerships between universities, national labs and the private sector. 

“This is a new field, and you have to build the workforce,” Davoudi said. “I think it's important for our field to bring in diverse talent that would allow the field to continue to intellectually grow, and be able to solve the problems that we would like to eventually solve.”

 

Written by Dina Genkina

Sasha Philippov Investigates Plasma Around Black Holes and Neutron Stars

Curiosity about the cosmos has attracted many young astrophysicists to their careers, but that was not the case for Alexander “Sasha” Philippov. While growing up in Russia, he was a natural at science and even competed in the national Physics Olympiad for high school students. However, his interests at the time were more down-to-earth.Sasha PhilippovSasha Philippov

“I was not into astrophysics whatsoever,” said Philippov, who joined the University of Maryland’s Department of Physics as an assistant professor in May 2022. “When I went to college, I was hoping to do theoretical particle physics, but my advisor and mentor, Professor Vasily Beskin, showed me that you can do very interesting, detailed modeling in astrophysics. It looked like real physics to me—not just looking into a telescope and watching the stars.”
 
Philippov has been starstruck ever since, using a combination of theory and computer modeling to tackle big questions in high-energy astrophysics and publish over 60 papers. 

After completing his undergraduate studies at the Moscow Institute of Physics and Technology, he earned a Ph.D. in astrophysical sciences from Princeton University in 2017. It was during his graduate studies that he started specializing in the physics of plasmas—a state of matter comprising hot, ionized gas that surrounds “some of the most mysterious and exotic objects in the universe,” including black holes and neutron stars, Philippov said. 

He was then named a NASA Einstein and Theoretical Astrophysics Center Fellow and completed his postdoc at UC Berkeley, where he co-developed computer code to model the behavior of charged particles around rotating black holes.

“This sort of thing had never been modeled before, because you need to take into account the effects of general relativity, how the electromagnetic fields are modified by the spinning black hole and how they react to the dynamics of charged particles,” Philippov explained. “Ours was the first code that could do it.” 

His code enabled a flurry of studies—including five publications in the journal Physical Review Letters—which offered new insights into the extraction of energy from rotating black holes, the production of electron-positron plasmas and electromagnetic flares near the event horizons of black holes, and the accretion of collisionless plasma.

After his postdoc, Philippov worked as an associate research scientist at the Simons Foundation’s Flatiron Institute in New York City, where he continued to study the emission mechanisms of pulsars—magnetized neutron stars that rapidly rotate. During this time, he constructed the first models capable of explaining the mysterious coherent emission of pulsars, which were found to produce relativistic lightning strong enough to shoot beams of radio waves out into space. Although this cosmic phenomenon was discovered more than 50 years ago, its cause was not fully understood until Philippov’s study.

Recently, he was named deputy director of a multi-institutional Simons Foundation project called the Simons Collaboration on Extreme Electrodynamics of Compact Sources (SCEECS). The team will model electrodynamic processes related to neutron stars and black holes, which have magnetic fields that are 10 billion times stronger than those associated with the Large Hadron Collider in Switzerland.

The group will use kinetic plasma simulations and large-scale fluid-type modeling to study the underlying emission mechanisms of magnetars—neutron stars with the strongest magnetic fields—and spinning black holes. Advances in high-performance computing and telescope technologies help make this work possible.

“It’s a big investment for research that is completely theoretical,” Philippov said of the grant. “We will be looking at a collection of both completely new and very old problems—the latter having been revitalized by the power of computer simulations and new observations. It’s a great time to do this.”

Philippov also recently received a $600,000 grant from the National Science Foundation to support the modeling of phenomena in extreme plasmas around black holes and neutron stars. In addition, he continues to study the radiation of neutron stars (including enigmatic fast radio bursts), flares from accreting supermassive black holes and merging neutron stars, and particle acceleration in jets produced by black holes. 

As a Fellow in the Joint Space-Science Institute (JSI), a collaboration between the NASA’s Goddard Space Flight Center and UMD’s astronomy and physics departments, Philippov is helping to organize a workshop in October 2023 that will share the latest expertise on “winds throughout the universe,” including everything from the sun’s powerful wind to the gusts produced by merging neutron stars.

In his day-to-day work, Philippov works closely with students and postdoctoral fellows and said he “tremendously enjoys mentoring and interacting with early career researchers.” 

Though he was not instantly smitten with astrophysics as a high school student, he is happy he pursued this career path. For him, having the chance to ponder big questions in astrophysics—and better yet, to answer them—is what continues to drive his research.

“The time that you get to study something completely new is why we are in this business,” Philippov said. “The joy of getting to finally understand something after a long time is remarkable.”

 

Written by Emily Nunez.

In Memoriam

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

  • Donald Robert Benton (Ph.D., '85) died on May 5, 2023.
  • Larry Lambert Burton (Ph.D., '77) died on March 23, 2023.
  • Richard Durkin (M.S., '72) died on April 22, 2023. 
  • Lewis Fulcher, a former postdoctoral associate, died on May 9, 2023.
  • Professor Emeritus Charles William Misner died on July 24, 2023. A memorial service is planned for November 10 & 11More
  • Sherman Poultney, a faculty member who worked on the Lunar Laser Ranging Reflector for Apollo 11, died on February 9, 2023.
  • Bruce Rowley, a talented machinist in the Department of Physics from 2004 until his retirement in 2022,, died on July 19.
  • Arthur W. Ruff (Ph.D., '64), died on April 24, 2023.
  • Philip DiLavore III, a who served as an Assistant Professsor before moving to Indiana State University in 1971, on died July 16, 2023.
  • Jonathan San Miguel (B.S., '17), died on April 16, 2023, in Stanford, CA.

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