Blades of light: A tabletop method for generating megatesla magnetic fields

Osaka, Japan - Researchers at The University of Osaka have developed a novel method for generating ultrahigh magnetic fields via laser-driven implosions of blade-structured microtubes. This method achieves field strengths approaching one megatesla—a breakthrough in compact, high-field plasma science.

Ultrastrong magnetic fields approaching the megatesla regime—comparable to those found near strongly magnetized neutron stars or astrophysical jets—have now been demonstrated in theory using a compact, laser-driven setup. A team led by Professor Masakatsu Murakami at The University of Osaka has proposed and simulated a unique scheme that uses micron-sized hollow cylinders with internal blades to achieve these field levels.

The technique—called bladed microtube implosion (BMI)—relies on directing ultra-intense, femtosecond laser pulses at a cylindrical target with sawtooth-like inner blades. These blades cause the imploding plasma to swirl asymmetrically, generating circulating currents near the center. The resulting loop current self-consistently produces an intense axial magnetic field exceeding 500 kilotesla, approaching the megatesla regime. No externally applied seed field is required.

This mechanism stands in stark contrast to traditional magnetic compression, which relies on amplifying an initial magnetic field. In BMI, the field is generated from scratch—driven purely by laser-plasma interactions. Moreover, as long as the target incorporates structures that break cylindrical symmetry, high magnetic fields can still be robustly generated. The process forms a feedback loop in which flows of charged particles—composed of ions and electrons—strengthen the magnetic field, which in turn confines those flows more tightly, further amplifying the field.

“This approach offers a powerful new way to create and study extreme magnetic fields in a compact format,” says Prof. Murakami. “It provides an experimental bridge between laboratory plasmas and the astrophysical universe.”

Potential applications include:

•            - Laboratory astrophysics: mimicking magnetized jets and stellar interiors

•            - Laser fusion: advancing proton-beam fast ignition schemes

•            - High-field QED: probing non-linear quantum phenomena

Simulations were conducted using the fully relativistic EPOCH code on the SQUID supercomputer at The University of Osaka. A supporting analytic model was also constructed to reveal the fundamental scaling laws and target optimization strategies.

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The article, “Gigagauss magnetic field generation by bladed microtube implosion” was published in Physics of Plasmas at DOI: https://doi.org/10.1063/5.0275006.

Publication Details

Title: Gigagauss magnetic field generation by bladed microtube implosion

Authors: D. Pan, M. Murakami

Journal: Physics of Plasmas (American Institute of Physics)

https://doi.org/10.1063/5.0275006 (Online publication: July 14, 2025)

Funding: Japan Society for the Promotion of Science (JSPS), Kansai Electric Power Company (KEPCO)

Simulations: Performed using the SQUID supercomputer at The University of Osaka

About The University of Osaka

The University of Osaka was founded in 1931 as one of the seven imperial universities of Japan and is now one of Japan's leading comprehensive universities with a broad disciplinary spectrum. This strength is coupled with a singular drive for innovation that extends throughout the scientific process, from fundamental research to the creation of applied technology with positive economic impacts. Its commitment to innovation has been recognized in Japan and around the world. Now, The University of Osaka is leveraging its role as a Designated National University Corporation selected by the Ministry of Education, Culture, Sports, Science and Technology to contribute to innovation for human welfare, sustainable development of society, and social transformation.

Website: https://resou.osaka-u.ac.jp/en