Physicists Achieve Unmatched Precision in Measuring Magnetic Anomalies in Mines

Researchers from the Muon G-2 Experiment have unveiled their third measurement of the Muon magnetic anomaly. The conclusive results align with findings published in 2021 and 2023 but boast significantly improved precision at 127 parts per billion, surpassing the experimental goal for 140 people.

Muon particles traveling through lead in the cloud chamber. Image credit: Jino John 1996 / cc by-sa 4.0.

The Muon G-2 experiment investigates the wobble of a fundamental particle known as the Muon.

Muons resemble electrons but are roughly 200 times more massive. Like electrons, they exhibit quantum mechanical properties called spins, which can be interpreted as tiny internal magnets.

When subjected to an external magnetic field, these internal magnets wobble akin to the axis of a spinning top.

The precession speed of a magnetic field is influenced by the muon’s characteristics, captured numerically as the G-factor.

Theoretical physicists derive G-factors based on our current understanding of the universe’s fundamental mechanics, as outlined in the standard model of particle physics.

Nearly a century ago, G was anticipated to be 2; however, experimental measurements revealed minor deviations from this value, quantified as the Muon magnetic anomaly, Aμ, based on the formula (G-2)/2, giving the Muon G-2 experiment its name.

Muon magnetic anomalies encapsulate the effects of all standard model particles, enabling theoretical physicists to compute these contributions with remarkable precision.

Earlier measurements conducted at the Brookhaven National Laboratory during the 1990s and 2000s indicated potential discrepancies with the theoretical calculations of that era.

Disparities between experimental results and theoretical predictions could signal the existence of new physics.

In particular, physicists contemplated whether these discrepancies could stem from an undetected particle influencing the muon’s precession.

Consequently, physicists opted to enhance the Muon G-2 experiments to obtain more accurate measurements.

In 2013, Brookhaven’s magnetic storage ring was relocated from Long Island, New York, to Fermilab in Batavia, Illinois.

Following extensive upgrades and enhancements, the Fermilab Muon G-2 experiment launched on May 31, 2017.

Simultaneously, an international collaboration among theorists established the Muon G-2 theory initiative aimed at refining theoretical calculations.

In 2020, the Theoretical Initiative released updated and more precise standard model values informed by data from other experiments.

The differences between the experimental results continued to widen in 2021 as Fermilab announced the initial experimental results, corroborating Brookhaven’s findings with improved accuracy.

Simultaneously, new theoretical predictions emerged, relying significantly on computational capabilities.

This information closely aligned with experimental measurements and narrowed the existing discrepancies.

Recently, the Theoretical Initiative published a new set of predictions integrating results from various groups using novel calculation techniques.

This result remains in close agreement with experimental findings and diminishes the likelihood of new physics.

Nevertheless, theoretical endeavors will persist in addressing the disparities between data-driven and computational approaches.

The latest experimental values for the muon magnetic moment from Fermilab’s experiments are:

aμ =(g-2)/2 (Muon experiment) = 0.001 165 920 705

This final measurement is based on an analysis of data collected over the past three years, spanning 2021 to 2023, and is integrated with previously published datasets.

This has more than tripled the dataset size utilized in the second results from 2023, achieving the precision target set in 2012.

Moreover, it signifies the analysis of the highest quality data from the experiment.

As the second data collection run concluded, the Muon G-2 collaboration finalized adjustments and enhancements to the experiment, boosting muon beam quality and minimizing uncertainties.

“The extraordinary magnetic moment of the muon (G-2) is pivotal as it provides a sensitive test of the standard model of particle physics,” remarked Regina Lameika, associate director of high energy physics at the U.S. Department of Energy.

“This is an exhilarating result, and it’s fantastic to witness the experiment reach a definitive conclusion with precise measurements.”

“This highly anticipated outcome represents a remarkable achievement in accuracy and will hold the title of the most precise measurement of muon magnetic anomalies for the foreseeable future.”

“Despite recent theoretical challenges that have lessened the evidence for new physics in Muon G-2, this finding presents a robust benchmark for proposed extensions to the standard model of particle physics.”

“This is an incredibly exciting moment; not only did we meet our objectives, but we surpassed them, indicating that such precision measurements are challenging.”

“Thanks to Fermilab, the funding agencies, and the host lab, we accomplished our goals successfully.”

“For over a century, the G-2 has imparted crucial insights into the nature of reality,” stated Lawrence Gibbons, a professor at Cornell University.

“It’s thrilling to contribute accurate measurements that are likely to endure for a long time.”

“For decades, muon magnetic moments have served as a significant benchmark for the standard models,” noted Dr. Simon Kolody, a physicist at Argonne National Laboratory.

“The new experimental results illuminate this fundamental theory and establish a benchmark to guide new theoretical calculations.”

These new results will be featured in the journal Physical Review Letters.

Source: www.sci.news

Anomalies in the Universe: Massive spiral galaxies expel enormous pairs of relativistic jets

2MASX J23453268-0449256 (J2345-0449 for short), a very huge, rapidly spinning, jet lag spiral galaxy with approximately 947 million light years in the Aquarius constellation, a mass of billions of people billions that are billions of times the sun’s, and mounted on a massive radio jet spanning six million light years. This is one of the largest known in any spiral galaxy, and such powerful jets are almost exclusively found in elliptical galaxies rather than spiral, thus covering the conventional wisdom of galaxies’ evolution. It also means that the Milky Way can potentially create similar energetic jets in the future.



This image shows the Spiral Galaxy 2Masx J23453268-0449256 and its huge radio jet. Image credit: Bagchi et al. /Giant Metrure Lave Radio Telescope.

“This discovery is more than just weird. It forces us to rethink the evolution of galaxies and how super-large black holes grow and shape the environment within them,” said Professor Joydeep Baguch of Christ University.

“If spiral galaxies can not only survive, but also thrive under such extreme conditions, what does this mean for the future of our own Milky Way galaxies?”

“Can our Galaxy experience similar high-energy phenomena that have serious consequences for the survival of precious lives within it?”

In a new study, astronomers have unraveled the structure and evolution of the Spiral Galaxy J2345-0449, three times the size of the Milky Way.

Using observations from NASA/ESA Hubble Space Telescope, Giant Metruh Rave Radio Telescope, Atacama’s Large Millimeter/Sub-Millimeter Array (ALMA), and multi-wavelength analysis, we detected the giant ultrafine black holes of its mind and radio jets in the largest radio jets by creating rare galaxies.

Traditionally, scientists believed that such huge, superimpression violent activities would destroy the delicate structures of spiral galaxies.

But for all possibilities, J2345-0449 retains its quiet nature with a well-defined spiral arm, bright nuclear bars and an uninterrupted ring of stars.

In addition to enigma, the galaxy is surrounded by vast halos of hot x-ray exhaust, providing important insights into its history.

This halo cools slowly over time, but the black hole jets act like space furnaces, preventing new star formation despite the abundant star-building materials present.

The authors also found that J2345-0449 contains 10 times the dark matter as the Milky Way.

“Understanding these rare galaxies could provide important clues about the invisible forces that govern the universe, such as the nature of dark matter, the long-term fate of the galaxy, and the origin of life,” says Ph.D. A student at the University of Christ.

“In the end, this research brings us one step closer to solving the mystery of the Cosmos and reminds us that the universe holds surprise beyond our imagination.”

Survey results It was published in Monthly Notices from the Royal Astronomical Society.

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Joydeep Bagchi et al. 2025. Announcing bulge disk structures, AGN feedback and baryon landscapes in a large helical galaxy with MPC-scale radio jets. mnras 538(3): 1628-1652; doi: 10.1093/mnras/staf229

Source: www.sci.news

Galactic anomalies suggesting dark matter presence are more puzzling than anticipated

A dark matter halo (yellow) forms around the galaxy

Ralph Koehler/SLAC National Accelerator Laboratory

When you think of the Milky Way, “delicate” may not be the first word that comes to mind.But when Mariangela Lisanti She started tinkering with the Our Galaxy recipe, but found it surprisingly fragile.

Lisanti, a particle physicist at Princeton University, wonders what would happen if dark matter, a mysterious substance thought to make up more than 80 percent of all matter in the universe, was more exotic than researchers usually assume. I was simulating something. She replaced a small portion of standard dark matter with something more complex. “We thought we could just add 5% and everything would be fine,” she says. “And we destroyed the galaxy.”

There are good reasons for such interference. Since the 1980s, astronomical signs have shown that dark matter is a single type of slow-moving particle that does not interact with itself. Particle physicists have spent a great deal of effort searching for that particle. But decades later, it remains a no-show. Perhaps because dark matter is not what we tend to imagine.

Recently, a series of galactic anomalies have sparked a scramble to find alternatives. This “complex” dark matter can be as simple as subatomic particles bouncing off each other, or as complex as dark particles forming dark atoms, stars, and even galaxies. There are a number of mind-boggling possibilities.

But now observations of anomalies in our galaxy promise to finally help narrow down the options. and…

Source: www.newscientist.com