PETE JOHNSON: An Abundant Source of Energy

Pete Johnson, An Abundant Source of Energy

 


October 8, 2024
Above: Pete Johnson

Pete Johnson, BA’03 physics, is a source of boundless energy. At just 45, the husband and father of four has earned a master’s degree in mechanical engineering at Stanford, founded and built several leading companies, worked as a venture capitalist and investor in Silicon Valley, and is currently the president and CEO of Koloma, Inc., a global leader in geologic hydrogen exploration.

Left to right, Grace, Levi, Pete, Kristin, Josh and Sydney Johnson

What focuses his energy, though, is his family — wife Kristin, daughter Sydney, 16; daughter Grace, 14; son Josh, 10; son Levi, 8.

Johnson is exploring and developing technologies to tap a new source of energy that is powerful, vast, and clean. It’s known as geologic hydrogen. Studies suggest that the earth produces significant amounts of hydrogen through natural geochemical processes and that it may be accumulating in formations below the surface. If sufficiently sized reservoirs can be found, geologic hydrogen could help fuel the U.S. economy for centuries to come while reducing emissions and carbon footprints.

Johnson grew up in The Avenues neighborhood of Salt Lake during the eighties. “I was born the fifth of six sons and had an unbelievably fun, Huck Finn-type of childhood exploring the foothills by foot and bike with my brothers,” he says. “We also spent a lot of time skiing, boating and going to high school sports games for my older brothers.”

At East High School, Pete was inspired by several teachers and classes, including AP Biology and AP Calculus. “I think the most inspiring person for me at East was Keeko Georgelas, the head coach who revitalized the school’s football program and took it from a perennial doormat to one of the top programs in the state. Keeko put into our heads that we could do great things.” Pete took those words to heart, channeling that motivation as he led the East High football team to a state championship in 1997, his senior year. It was the first championship at East since 1974.

Awarded a four-year presidential scholarship, Johnson enrolled at the University of Utah for Fall semester 1997 intending to be an environmental or civil engineering major. “I was interested in biology and math and wanted to be in the environmental remediation and hydrology world, in part thinking that it would give me lots of opportunities to work outside.”

Johnson completed the prerequisite courses before serving a two-year church mission. When he returned, in 2000, he struggled to find passion for the course work. He persisted and took a few more civil engineering classes but wasn’t intrigued with the subject matter.

“I started thinking about what else I could do and was in the middle of a general physics course taught by Sid Rudolph who was just a crazy man and unbelievably passionate about physics,” says Johnson. “I decided to give it a try and was pleasantly surprised with the curriculum and the way I was challenged by the science and the math.”

“I had tough, interesting courses in quantum physics, nuclear physics, electromagnetics and other areas from faculty [not only] Sid Rudolph, [but also] Clayton Williams, Mikhail Raikh and Rich Ingebretsen," says Johnson. "Rich was a longtime family friend who also taught me how to run rivers.” It was the cumulative effect of these courses, and perhaps hitting the rapids, that inspired Johnson to become an entrepreneur in the energy sector.

“My dad was in energy, and it was always something that I was interested in," says Johnson. "So, I applied to the mechanical engineering graduate programs at Stanford and MIT and was accepted into both programs."

Johnson chose Stanford and spent two years there, mostly doing biomechanical research where he found some fascinating topics in stem cell implantation into heart tissue. “At that point, it was time to propose a PhD project, but I struck out on two or three different ideas, being told by my advisor that these ideas sounded more like business plans than research projects. I kept trying to ‘science’-up the proposals but wasn’t getting it, and I realized, probably later than my advisor, that I was more interested in stepping out and pursuing things in Silicon Valley than I was in three-to-five more years in the lab. So, I finished with a master’s degree and never looked back.”

Modern day gold rush

The company name, Koloma, was inspired by the small town of Coloma, California, where gold ore was discovered in 1848 which led to the California Gold Rush that transformed the country and the entire economy. Johnson and company founders Tom Darrah, Paul Harraka and Scott McNally visited the site in 2021 to launch Koloma, Inc. Geologic hydrogen has also been referred to as gold hydrogen, so the team thought the name was appropriate. An appreciation for the history of exploration and the value of learning from the past is embedded in the company.

“The unique thing about Koloma is that we have 20 years of data advantage and a big head start in the field, and that data advantage has led to a large number of tools and techniques we can build and validate through our exploration work,” says Johnson.

Koloma has already developed the technology to identify the most promising regions for geologic hydrogen potential. The company continues to conduct geophysical studies and some preliminary drilling projects around the world. Johnson anticipates large-scale hydrogen production to begin by 2030 if they are successful in their exploration efforts.

As a new primary energy source, naturally occurring geologic hydrogen could be a powerful tool to help move towards lower carbon energy forms in the U.S. and around the world.

The Science

Geologic hydrogen is generated naturally in the Earth’s iron-rich mantel by an oxidation-reduction reaction known as serpentinization. Through this water-rock reaction, considerable quantities of hydrogen are continuously produced and stored in geological formations below the surface. In fact, geologic hydrogen can be produced with low-carbon intensity, resulting in a low-carbon footprint on par with electrolysis. In addition, the process does not require external water inputs or external energy inputs such as heat or electricity.

For these reasons, geologic hydrogen presents a highly efficient, low-cost and low-greenhouse-gas energy source.

Even with all that potential energy in development, Johnson’s internal energy source is rooted in Mountain View, California, near Stanford where he and his family reside.

“We’ve always got plenty going on,” says Johnson of his family which spends weekends at soccer games, hiking in the redwoods or hanging out on the Northern California coast.

He met his wife Kristin in September 2003, the first weekend he was in Palo Alto for graduate school. “Kristin had just taken a job with Pfizer in sales. I was smitten early on, but she was dating guys who didn’t have years of grad work in front of them and were already going places, so it took me about a year of building trust as a friend before she really started to see me as a viable option!”

“Once we started dating it was clear we had something great going on, and I think my mom would have killed me if I messed it up so I was careful,” says Johnson who proposed at sunrise on top of Half Dome in Yosemite National Park. They were married in October 2005 in Salt Lake City.

Pete Johnson’s advice to others is simple and, not surprisingly, family-centric: “Avoid thinking that being passionate about your work means you won’t be able to be a great spouse and parent. Find a way to make it all work.”

APS Fellowship awarded to Tino Nyawelo

APS Fellowship awarded to Tino Nyawelo


October 4, 2024
Above: Tino Nyawelo

The American Physical Society has elected the Society's 2024 Fellows, one of whom is University of Utah's Tino Nyawelo. 

 

The APS Fellowship Program recognizes members who have made exceptional contributions in physics research, important applications of physics, significant contributions to physics education, or leadership in or service to APS.

This year,149 Fellows were selected and recognized for their contributions to science. Nyawelo's honor was by recommendation of the American Physical Society Forum on Diversity and Inclusion at its September council meeting. The citation reads that the award is being made “[f]or significant contributions to creating and sustaining physics and STEM education opportunities for students from marginalized groups, particularly refugees.”

"I am incredibly grateful and humbled by this award," says Nyawelo. "It feels great to be recognized and rewarded for the hard work that one does. I am grateful to everyone who has always been a part of my journey, from my family to my colleagues who supported me and showed me how to give back to my community. In particular, I would like to thank my former Dean — Pierre Sokolsky who enthusiastically encouraged me from the very beginning and strongly supported my work to provide opportunities for students from marginalized groups in STEM."

Earlier this year, under the auspices of Nyawelo's INSPIRE program, a community of refugee students and their families, scientists, educators and policymakers celebrated an event three years in the making. As reported in @The U, Nyawelo and his team installed five cosmic ray detectors atop the Department of Workforce Services Utah Refugee Center in downtown Salt Lake City. The detectors, which measure echoes of cosmic particles bombarding Earth’s atmosphere, were built by nearly 60 participants in the program formally called Investigating the Development of STEM-Positive Identities of Refugee Teens in a Physics Out of School Time Experience. INSPIRE brings science research — in this case particle physics — to teenagers and contributes to a worldwide effort to measure cosmic ray activity on Earth. Data from these detectors are added in real-time to a widely available database that has also recently been relocated to U.

"The APS Fellow distinction is given to less than 0.5% of the non-student APS members and is an incredible honor for our department," says Carsten Rott, chair of the Department of Physics and Astronomy. "I am just excited about all the ways that Tino has and continues to enrich our department and give deeper meaning to the importance of STEM education, in many cases making life changing differences for so many students."

A presentation of certificates is done at the annual meeting of the APS forum on Diversity and Inclusion.

By David Pace

Read about Nyawelo's winning last year's international Spirit of Salam Award here.

ACCESS Scholar: Kate Anderson

ACCESS Scholar, Kate Anderson


October 1, 2024
Above: Kate Anderson

Undergraduate Kate Anderson has her sights set far, another planet to be exact. After a year of research in the ACCESS Scholars program, she is one step closer to her dream of becoming a NASA astronaut. 

Anderson grew up in Las Vegas, Nevada, and had a passion for science, astronomy specifically, from a young age. She says that ACCESS was what initially drew her to the U, and ultimately what made her decide to major in physics and chemistry. The ACCESS scholarship is designed to advance belonging in STEM by engaging first-year students with research and helping them develop a community within the college.

Like many alumni of the program, ACCESS strongly shaped Anderson’s first year experience. She contributed to a project in Assistant Professor Yao-Yuan Mao’s astrophysics lab. Anderson gathered data with code to locate isolated, low-mass galaxies near the Milky Way that might provide clues to the origin of our universe. 

“Some of these galaxies are so isolated from the Milky Way that they have had little to no interaction with other galaxies since their creation. Because of that, they still have a lot of the properties of the very early universe. I was just trying to find the precursor to the bigger question” explains Anderson. 

This hands-on research experience through ACCESS helped Anderson earn a NASA Space Grant Consortium Scholarship, an additional boost on her path to becoming an astronaut. 

Anderson’s dream of voyaging to another planet to do true astrophysics “fieldwork” is supported by a plan that has been in the works since well before she stepped foot on campus. “I decided I wanted to be an astronaut and worked backwards,” she says. 

NASA astronauts either have a science or military background. Anderson thought “why not both?”. This motivated her to join the Air Force ROTC in addition to her academic obligations with the hope of becoming a pilot. This way, she can command the spaceship as well as handle the science. 

“NASA actually posted applications for astronauts a couple months ago. I was devastated that I couldn't apply now,” says Anderson. Though the journey ahead is long, this budding scientist and future space traveler has a lot to look forward to in her next few years at the U. Anderson is excited about starting  new research projects, taking observational astronomy, and spending time with her friends, many of whom she met through ACCESS. 

By Lauren Wigod

How special is the Milky Way Galaxy?  

How special is the Milky Way Galaxy?


September 25, 2024

Above: A mosaic of the satellite galaxies across the Milky Way-like systems that the SAGA team has surveyed. The mages are sorted by their luminosity from left to right. Credit: Yao-Yuan Mao (Utah), with images from the DESI Legacy Surveys Sky Viewer

A “saga” about 101 galaxies like the Milky Way and their companions

Is our home galaxy, the Milky Way Galaxy, a special place? A team of scientists started a journey to answer this question more than a decade ago. Commenced in 2013, the Satellites Around Galactic Analogs (SAGA) Survey studies galaxy systems like the Milky Way. Now, the SAGA Survey just published three new research articles that provide us with new insights into the uniqueness of our own Milky Way Galaxy after completing the census of 101 satellite systems similar to the Milky Way’s.   

These “satellites” are smaller galaxies in both mass and size which orbit a larger galaxy, usually called the host galaxy. Just as with smaller satellites that orbit the Earth, these satellite galaxies are captured by the gravitational pull of the massive host galaxy and its surrounding dark matter. The Milky Way Galaxy is the host galaxy of several satellite galaxies, of which the two largest are the Large and Small Magellanic Clouds (LMC and SMC). While LMC and SMC are visible to the naked eye from the Southern Hemisphere, there are many other fainter satellite galaxies orbiting around the Milky Way Galaxy that can only be observed with a large telescope.  

The goal of the SAGA Survey is to characterize satellite systems around other host galaxies that have similar stellar masses as the Milky Way Galaxy. Yao-Yuan Mao, a University of Utah faculty member in the Department of Physics and Astronomy, is co-leading the SAGA Survey with Marla Geha at Yale University and Risa Wechsler at Stanford University. Mao is the lead author of the first article in the series of three that have all been accepted by the Astrophysical Journal. This series of articles reports on the SAGA Survey’s latest findings and makes the survey data available to other researchers worldwide.  

 An outlier galaxy? 

An image of a Milky Way-like galaxy and its system of satellite galaxies. The SAGA survey identified six small satellite galaxies in orbit around this Milky Way analog. Credit: Yasmeen Asali (Yale), with images from the DESI Legacy Surveys Sky Viewer https://www.legacysurvey.org/acknowledgment/

 In the first study led by Mao, the researchers highlighted 378 satellite galaxies identified across 101 Milky Way-mass systems. The number of confirmed satellites per system ranged from zero to 13 — compared to four satellites for the Milky Way. While the number of satellite galaxies in the Milky Way system is on par with the other Milky Way-mass systems, “the Milky Way appears to host fewer satellites if you consider the existence of the LMC,” Mao said. The SAGA Survey has found that systems with a massive satellite like the LMC tend to have a higher total number of satellites, and our Milky Way seems to be an outlier in this regard. 

An explanation for this apparent difference between the Milky Way and the SAGA systems is the fact that the Milky Way has only acquired the LMC and SMC quite recently, compared with the age of the universe). The SAGA article explains that if the Milky Way Galaxy is an older, slightly less massive host with the recently added LMC and SMC, one would then expect a lower number of satellites in the Milky Way system not counting other smaller satellites that LMC/SMC might have brought in.  

This result demonstrates the importance of understanding the interaction between the host galaxy and the satellite galaxies, especially when interpreting what we learn from observing the Milky Way. Ekta Patel, a NASA Hubble Postdoctoral Fellow at the U but not part of the SAGA team, studies the orbital histories of Milky Way satellites. After learning about the SAGA results, Patel said, “Though we cannot yet study the orbital histories of satellites around SAGA hosts, the latest SAGA data release includes a factor of ten more Milky Way-like systems that host an LMC-like companion than previously known. This huge advancement provides more than 30 galaxy ecosystems to compare with our own, and will be especially useful in understanding the impact of a massive satellite analogous to the LMC on the systems they reside in.”  

Why do galaxies stop forming stars? 

The second SAGA study of the series is led by Geha, and it explores whether these satellite galaxies are still forming stars. Understanding the mechanisms that would stop the star formation in these small galaxies is an important question in the field

Yao-Yuan Mao

of galaxy evolution. The researchers found, for example, that satellite galaxies located closer to their host galaxy were more likely to have their star formation “quenched,” or suppressed. This suggests that environmental factors help shape the life cycle of small satellite galaxies.  

The third new study is led by Yunchong (Richie) Wang, who obtained his PhD with Wechsler. This study uses the SAGA Survey results to improve existing theoretical models of galaxy formation. Based on the number of quenched satellites in these Milky Way-mass systems, this model predicts quenched galaxies should also exist in more isolated environments — a prediction that should be possible to test in the coming years with other astronomical surveys such as the Dark Energy Spectroscopic Instrument Survey.  

Gift to the astronomy community 

In addition to these exciting results that will enhance our understanding of galaxy evolution, the SAGA Survey team also brings a gift to the astronomy community. As part of this series of studies, the SAGA Survey team published new distance measurements, or redshifts, for about 46,000 galaxies. “Finding these satellite galaxies is like finding needles in a haystack. We had to measure the redshifts for hundreds of galaxies to just identify one satellite galaxy,” Mao said. “These new galaxy redshifts will enable the astronomy community to study a wide range of topics beyond the satellite galaxies.”  

The SAGA Survey was supported in part by the National Science Foundation and the Heising-Simons Foundation. Other authors of these three SAGA studies include Yasmeen Asali, Erin Kado-Fong, Nitya Kallivayalil, Ethan Nadler, Erik Tollerud, Benjamin Weiner, Mia de los Reyes, John F. Wu, Tom Abel, and Peter Behroozi. 

By David Pace

The Art and Science of Innovation: Catmull’s Story

The Art and Science of Innovation: Catmull’s Story


Sep 16, 2024
Above : Edwin Catmull, co-founder of Pixar. | Pixar

Ed Catmull doesn’t have the intense presence one might expect from a man with his resume.

Not only has Catmull [BS’69, physics] won five Academy Awards, he’s also received an ACM A.M. Turing Award — considered the Nobel Prize of computing — has rubbed shoulders with George Lucas and Steve Jobs, co-founded Pixar and co-created the first computer-animated film (and the technology that made it possible).

Catmull is the 2024 winner of The Leonardo Award, an award that seeks to honor individuals who have made “contributions (that) exemplify the blend of art and science,” per The Leonardo.

To receive his Leonardo Award, Catmull returned to Salt Lake City — the very place his impressive career started.

“(Catmull) credits the atmosphere and the work that he did at the University of Utah with some of his early success,” Virginia Pearce, director of the Utah Film Commission, said during Thursday night’s ceremony. “We are so proud about your start in Utah and the deeply grateful for the mark that you’ve made on (the film industry) industry and beyond.”

‘It was amazing’: How the University of Utah shaped Catmull’s career

As a kid, Catmull balanced his interests in both art and science. He never saw the subjects as being inharmonious.

“Growing up, I didn’t know that (science and art) were considered to be not compatible with each other. Nobody told me that,” Catmull said Thursday night at The Leonardo Museum. Animation fascinated him, but there was no college for it. So when he started his Bachelor’s degree at University of Utah, he fell back on science.

“There were no tools for it, for animation, so I switched over into physics when I went to college,” Catmull said. This revelation prompted laughter from the audience — how can the man who co-founded Pixar be a physicist?

Read the full article by Margaret Darby in DeseretNews.

U Physics Alumna Heads to Paris Olympics

PHysics of Olympic Pistol Shooting


July 29, 2024
Above: Alexis Lauren Lagan, BS'17

With a pistol program desperate for success, Alexis (Lexi) Lauren Lagan BS'17 physics represents the next generation of athletes ready to take her sport to a new level. This month she heads to Paris. Her second Olympics.

Despite a degree in physics and a law degree in the works, Lexi can’t shake an Olympic dream so enticing she’s put her career on hold to represent her country in Paris this summer.

Lexi started shooting with her dad at a young age and enjoyed going to the range with her family as a bonding activity. While pursuing her bachelor’s degree in Pre-Law Physics, she began shooting international pistol at the University of Utah. At the collegiate level, she won a handful of national titles in women’s, mixed team events, and earned her spot on several All-American Teams.

Lexi participated in pistol for fun and to make friends in college, but as the Rio Games approached, she realized she wanted to pursue her interest in international shooting sports. She won the Olympic Alternate seat in Women’s Air Pistol in 2016, narrowly missing the opportunity to join Team USA in Rio. This only fueled her passion into the Tokyo 2020 Games and now Paris 2024.

In addition to visiting the range with her family, Lexi grew up dancing and singing. At 14, She received a medal and certificate from the White House for singing the National Anthem at more than 150 performances. She enjoys camping and hiking, and has a corgi named Guinevere who is frequently featured on her Instagram.

Read more about the sport.

Read more about U-affiliated athletes at the Games.

The Hidden Space Race and Vardeny’s Spintronic Revolution

The Hidden Space Race and Vardeny's Spintronic Revolution


July 19, 2024
Above: Valy Vardeny, Distinguished Professor of Physics & Astronomy, Photo Credit: Dung Hoang

Vardeny was a pioneer of organic spin waves known as “Spintronics.” Spin waves transfer information much faster with far less heat.

When Neil Armstrong and Buzz Aldrin landed on the moon fifty years ago, Zeev Valentine Vardeny was a young man living in Israel. The “space race” was palpable at the time. The “race” for ever-increasing technological innovation is profoundly felt in Israel. Putting brain power to work to maintain Israel’s safety is nothing short of a national mission.

Distinguished Professor of Physics & Astronomy Zeev Valentine Vardeny at the University of Utah in is certainly an All-Star of physics. While most Utahns have never heard of him, Vardeny opened up an entirely new branch of physics. He has helped innovate significant advances leading to OLED (organic LEDs), organic spin-wave and technology. If these aren’t familiar then next time you look at your organic LED flat-screen TVs or put your 96 gig flash memory card in your computer, just know that Vardeny and his work are a key part of that technology.

His field of Solid State Physics refers to how electrons behave when traveling through materials. Electrons flow through all of our electrical devices to provide them power. Computers transmit information and energy, but they also produce heat.

Vardeny says, " Using spintronic technology will help pave the way for vast changes in computer abilities that are known as quantum computers. First off. In regular computers the bits of regular computers are either a one or a zero. But if you have a quantum computer the bits can have infinite possibilities. There is an infinite number of numbers between zero and one.”

The Department of Defense is spending a lot of money is in using quantum computers and spin waves to create an entirely new form of communication.

You can read more about Vardeny and his research at the U in Utah Stories , Science Direct and Mirage News.

A once-in-a-career discovery: the black hole at Omega Centauri’s core

A once-in-a-career discovery: the black hole at Omega Centauri’s core


July 11, 2024
Above: The likely position of Omega Centauri star cluster’s intermediate black hole. Closest panel zooms to the system.
PHOTO CREDIT: ESA/HUBBLE & NASA, M. HÄBERLE (MPIA)

Omega Centauri is a spectacular collection of 10 million stars, visible as a smudge in the night sky from Southern latitudes.

Through a small telescope, it looks no different from other so-called globular clusters; a spherical stellar collection so dense towards the center that it becomes impossible to distinguish individual stars. But a new study, led by researchers from the University of Utah and the Max Planck Institute for Astronomy, confirms what astronomers had argued about for over a decade: Omega Centauri contains a central black hole.The black hole appears to be the missing link between its stellar and supermassive kin—stuck in an intermediate stage of evolution, it is considerably less massive than typical black holes in the centers of galaxies. Omega Centauri seems to be the core of a small, separate galaxy whose evolution was cut short when it was swallowed by the Milky Way.

“This is a once-in-a-career kind of finding. I’ve been excited about it for nine straight months. Every time I think about it, I have a hard time sleeping,” said Anil Seth, associate professor of astronomy at the U and co-principal investigator (PI) of the study. “I think that extraordinary claims require extraordinary evidence. This is really, truly extraordinary evidence.” A clear detection of this black hole had eluded astronomers until now. The overall motions of the stars in the cluster showed that there was likely some unseen mass near its center, but it was unclear if this was an intermediate-mass black hole or just a collection of the stellar black holes. Maybe there was no central black hole at all.

A medium Level panel zoom of the Omega Centauri star cluster’s intermediate black hole likely position. PHOTO CREDIT: ESA/HUBBLE & NASA, M. HÄBERLE (MPIA)

“Previous studies had prompted critical questions of ‘So where are the high-speed stars?’ We now have an answer to that, and the confirmation that Omega Centauri contains an intermediate-mass black hole. At about 18,000 light-years, this is the closest known example for a massive black hole,” said Nadine Neumayer, a group leader at the Max Planck Institute and PI of the study. For comparison, the supermassive black hole in the center of the Milky Way is about 27,000 light-years away.

A range of black hole masses

In astronomy, black holes come in different mass ranges. Stellar black holes, between one and a few dozen solar masses, are well known, as are the supermassive black holes with masses of millions or even billions of suns. Our current picture of galaxy evolution suggests that the earliest galaxies should have had intermediate-sized central black holes that would have grown over time, gobbling up smaller galaxies done or merging with larger galaxies.

Such medium-sized black holes are notoriously hard to find. Although there are promising candidates, there has been no definite detection of such an intermediate-mass black hole—until now.

“There are black holes a little heavier than our sun that are like ants or spiders—they’re hard to spot, but kind of everywhere throughout the universe. Then you’ve got supermassive black holes that are like Godzilla in the centers of galaxies tearing things up, and we can see them easily,” said Matthew Whittaker, an undergraduate student at the U and co-author of the study. “Then these intermediate-mass black holes are kind of on the level of Bigfoot. Spotting them is like finding the first evidence for Bigfoot—people are going to freak out.”

Read more about the Discovery @TheU.

Read more about the story at NASA, Deseret News, ABC4 Utah and ESA/Hubble releases.

Neutrino Oscillation Research Advances

Neutrino Oscillation Research Advances


July 9, 2024
Above: A Layout of IceCube Lab depth compared to the height of the Eiffel Tower.

In the world of particle physics, electrical charges define the terms. While electrons have a negative charge, the appropriately named “positron" has a positive charge. But then there are neutrinos which have no charge at all.

Neutrinos are also incredibly small and light. They have some mass, but not much and they rarely interact with other matter. They come in three types or "flavors": electron, muon, and tau.

Cosmic rays travel through space then crash into the earth's atmosphere and produce  air showers that Include neutrinos and many other types of particles. When neutrinos are produced and start traveling, they can change from one flavor to another. The atmospheric neutrinos are then detected by DeepCore, a denser array of sensors in the center of the IceCube detector at the South Pole.This process is called neutrino oscillation and the IceCube Detector, a massive neutrino detector buried deep in the ice at the South Pole, has a special area called DeepCore that can detect lower-energy neutrinos.

Scientists at the IceCube Neutrino Observatory in Antarctica have made a breakthrough in measuring neutrinos. Using advanced computer techniques, they've achieved the most precise measurements to date of how these particles change as they travel through space, helping us understand fundamental properties of the universe that could lead to new discoveries in physics.

Shiqi Yu

Shiqi Yu, a research assistant professor in the Department of Physics & Astronomy at the University of Utah and others who published their findings recently in Physical Review Letters analyzed data from over 150,000 neutrino events collected over nine years (2012-2021). They used advanced computer programs called convolutional neural networks (CNNs) to process this data. The team made the most precise measurements ever of two important properties related to neutrino oscillation: Delta m²₃₂ and sin²(θ₂₃). These numbers help describe how neutrinos change as they travel.

“We also carefully studied the systematic uncertainties that arise from our imperfect knowledge of our models and chose some to use as free nuisance parameters that fit together with the physics parameters for our data,” says Yu.

Using CNNs, which use three-dimensional data for image classification, Yu and co-lead of the study Jessie Micallef first developed use cases for the CNNs to focus on the DeepCore region and trained them to reconstruct different properties of particle interactions in the detector. They then used the CNN reconstructions to select qualified neutrino interactions that happened in or near the DeepCore region to produce a neutrino-dominated dataset with well-reconstructed energies and zenith angles.

Jessie Micallef

Yu notes that the CNN-reconstructed analysis-level dataset is already being used for other neutrino oscillation analyses, such as determining the neutrino mass ordering and non-standard neutrino interactions and for atmospheric tau neutrino appearance analyses.

“The atmospheric neutrino dataset from DeepCore exhibits relatively high energies in the oscillation analyses, which is unique compared to existing accelerator-based experiments,” says Yu. “Given our dataset and independent analysis, it is interesting to see agreement and consistency in physics parameter measurements.”

This research helps confirm and refine our understanding of how neutrinos — fundamental particles that can tell us a lot about the universe — behave. The techniques developed here, animated by machine learning, can be used in future studies to learn even more about neutrinos and the universe. Those future studies will be informed by IceCube which is planning an upgrade in 2025-2026 that will allow for even more detailed measurements of neutrinos.

By studying neutrino detection and the phenomenon of neutrino oscillation, scientists like Shiqi Yu hope to answer big questions about the nature of matter, energy and the cosmos.

Read the May 2024

Tony Hawk : The Intuitive Physicist of Vert Skating

The Intuitive Physicist of Vert Skating


June 13, 2024
Above: Tony Hawk executing an impressive aerial maneuver on his skateboard.

'Would you consider Tony Hawk a physicist?'

'I would consider Tony Hawk a physicist. If nothing else, he’s an intuitive scientist, right?'

Before you go, watch Kevin Davenport, assistant lecture professor in the Department of Physics & Astronomy at the U, break down the physics that allows vert skaters to huck themselves into the stratosphere—learn why he calls Tony Hawk an intuitive scientist.

Read the rest of the story by Lisa Potter at @The U.