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Home Science News Chemistry

The Mathematics That Links Frozen Magnets to Black Hole Chaos

September 22, 2026
in Chemistry
Katie Riggs
By Katie Riggs Scienmag Editorial Profile - Quantum Physics
Reading Time: 5 mins read
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The Mathematics That Links Frozen Magnets to Black Hole Chaos

The Mathematics That Links Frozen Magnets to Black Hole Chaos

The Mathematics That Links Frozen Magnets to Black Hole Chaos

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Physicists at the University at Buffalo have produced a mathematical solution to one of the most striking puzzles in modern quantum physics: how matter can transform from one of the slowest, most inert states imaginable into one of the fastest, most chaotic regimes known to science. Their work, published in Physical Review Letters, shows that a frustrated quantum magnet known as a spin glass can, under the right conditions, shed its frozen character and enter a regime of rapid, highly entangled dynamics described by the Sachdev-Ye-Kitaev model, the same theoretical framework physicists use to probe the information-scrambling behavior of black holes. The result, led by assistant professor Jamir Marino, provides an explicit mathematical bridge between two corners of physics that had long seemed to belong to different universes.

Spin glasses occupy a peculiar place in condensed matter physics. In ordinary magnets, atomic spins tend to align in an orderly pattern, pointing in the same direction and responding to disturbances in predictable ways. In a spin glass, by contrast, the interactions between spins are frustrated: the geometry and disorder of the system make it impossible for all the spins to settle into an arrangement that satisfies every competing influence simultaneously. The result is a state in which the atomic magnets point in disordered directions and become effectively frozen in place, locked into a rigid but random configuration. Because the spins cannot reorganize themselves easily, these systems respond to disturbances extraordinarily slowly, and information that enters the system can remain trapped for very long periods.

That sluggishness is precisely what makes spin glasses interesting beyond fundamental physics. Their capacity to hold information in place has implications for technologies in which stored quantum information must be protected from rapid degradation, and their landscape of competing configurations resembles the rugged cost landscapes that arise in complex optimization problems, including those encountered in artificial intelligence and machine learning. Understanding how spin glasses behave under extreme conditions, particularly at very low temperatures where quantum effects become important, has therefore been a goal with both practical and conceptual significance.

At the opposite end of the dynamical spectrum sits the Sachdev-Ye-Kitaev model, usually abbreviated as SYK. Proposed by Subir Sachdev and Jinwu Ye and later extended by Alexei Kitaev, the model describes a collection of particles whose interactions are so strongly and randomly coupled that the particles become massively entangled with one another. In this regime, any local piece of information is rapidly spread, or scrambled, across the entire system, in much the same way that physicists believe information is scrambled behind the horizons of black holes. The SYK model has become a central tool for studying quantum chaos, fast scrambling, and the strange correspondence between quantum systems and gravitational physics, but its relationship to ordinary, sluggish condensed matter has remained obscure.

Marino and his collaborators, including first author Hossein Hosseinabadi, a former graduate student in Marino’s laboratory who is now an independent distinguished postdoctoral scholar at the Max Planck Institute for the Physics of Complex Systems in Germany, set out to understand what happens to a spin glass as quantum fluctuations grow stronger, especially at extremely low temperatures where the standard mathematical descriptions of these systems have struggled. Their inquiry focused on an infinite-range quantum Heisenberg spin glass, an idealized but well-defined setting in which every spin interacts with every other spin, and quantum mechanical fluctuations compete directly with the glassy tendency of the spins to freeze.

To attack the problem, the team employed quantum field theory techniques based on an unconventional representation of spins, a mathematical reformulation that allowed them to follow the behavior of the system as the temperature drops. Rather than treating the spins as simple arrows pointing in fixed directions, this representation exposes their quantum nature and makes it possible to track how fluctuations grow and interact with the frozen order. The approach enabled the researchers to probe regimes that conventional treatments of spin glasses could not reach reliably, and to characterize the dynamics of the system throughout the crossover.

What they discovered came as a surprise. Intuition suggests that lowering the temperature should make a spin glass freeze even more thoroughly, locking its spins into ever more rigid disorder. Instead, the calculations revealed that as the temperature falls and quantum fluctuations intensify, those fluctuations can disrupt and eventually dismantle the locked arrangement of spins. Rather than becoming more firmly frozen, the system passes through a crossover in which the spins become so strongly entangled that they lose their individual identities altogether, and the slow glassy dynamics gives way to the fast, collective, scrambling behavior of the SYK model. The spin glass, in effect, melts from within, not because of heat but because of quantum mechanics.

You normally think that lowering the temperature will freeze something even more, Marino notes, but here the quantum effects can essentially melt the spin glass and carry the system from extremely slow dynamics to extremely fast dynamics. The team’s solution does not merely assert that this transition occurs; it provides the mathematical machinery that describes how matter moves from among the slowest states in quantum dynamics to among the fastest, tracing the entire trajectory and characterizing the intermediate states that lie between the two extremes. In doing so, it supplies a controlled, solvable example of a phenomenon that touches some of the deepest questions about the flow of quantum information.

The broader implications extend in several directions. Because spin glasses are natural candidates for architectures in which quantum information must be stored and protected, while SYK-like dynamics represents the rapid spreading of information that quantum technologies often try to avoid or exploit deliberately, understanding the pathway between these regimes could help engineers control when information stays put and when it disperses. The work also offers a concrete laboratory-scale connection to black hole physics: the same mathematical description that governs information scrambling in gravitational systems now emerges from an ordinary, if exotic, quantum magnet, reinforcing the idea that the principles of quantum chaos transcend the specific systems in which they were first discovered.

The study, titled Crossover to Sachdev-Ye-Kitaev Criticality in an Infinite-Range Quantum Heisenberg Spin Glass, appeared in Physical Review Letters, a journal of the American Physical Society, on September 17, and represents a collaboration between the University at Buffalo and Harvard University, where Marino worked alongside Subir Sachdev, the Herchel Smith Professor of Physics who first proposed the SYK model with Jinwu Ye. The research was performed using computational modeling and simulation grounded in quantum field theory, and its mathematical solution demonstrates that the boundary between ultraslow glassy order and ultrafast entangled chaos is not a wall but a traversable landscape, one that physicists can now explore with quantitative precision.

Subject of Research: A mathematical solution describing the transition of an infinite-range quantum Heisenberg spin glass from slow glassy dynamics to fast Sachdev-Ye-Kitaev quantum critical behavior.

Article Title: Physicists crack the math connecting ultraslow quantum magnetism to ultrafast black-hole physics

Article References: Physicists crack the math connecting ultraslow quantum magnetism to ultrafast black-hole physics. (n.d.). Original publication

Image Credits: AI Generated

DOI: Not provided

Keywords: spin glass, SYK model, quantum magnetism, black hole physics, quantum chaos, quantum entanglement, information scrambling, quantum field theory, condensed matter physics, quantum dynamics, Physical Review Letters, quantum technologies

Cite Scienmag News

Katie Riggs. (September 22, 2026). The Mathematics That Links Frozen Magnets to Black Hole Chaos. Scienmag. https://scienmag.com/the-mathematics-that-links-frozen-magnets-to-black-hole-chaos/

Katie Riggs. "The Mathematics That Links Frozen Magnets to Black Hole Chaos." Scienmag, 22 September 2026, https://scienmag.com/the-mathematics-that-links-frozen-magnets-to-black-hole-chaos/. Accessed 22 September 2026.

Katie Riggs. "The Mathematics That Links Frozen Magnets to Black Hole Chaos." Scienmag. September 22, 2026. https://scienmag.com/the-mathematics-that-links-frozen-magnets-to-black-hole-chaos/

Tags: black hole analogies in condensed matterblack hole information scramblingblack hole physicsCondensed matter physicsdisordered spin systemsfrustrated quantum magnetsinformation scramblingmathematical solutions in quantum physicsPhysical Review Lettersquantum chaosquantum dynamicsQuantum Entanglementquantum field theoryquantum information theoryquantum magnetismquantum technologiesSachdev-Ye-Kitaev modelspin glassspin glass dynamicsSYK modeltransition from frozen to chaotic states
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