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Precision quantum simulation of magnon spectra and interactions

This paper reports the high-precision analog-digital quantum simulation of a 97-qubit 2D XY spin-1/2 magnet, successfully extracting temperature-dependent magnon spectra and lifetimes while characterizing nonlinear scattering mechanisms that exceed the predictive capabilities of classical matrix-product state methods.

Original authors: Trond I. Andersen, Nikita Astrakhantsev, Jeronimo Martinez, Will Morong, Johannes Motruk, Dario Rossi, Brayden Ware, Bryce Kobrin, Weijie Wu, Elizabeth Bennewitz, Manuel Rudolph, Tom Westerhout, Amira
Published 2026-07-16
📖 6 min read🧠 Deep dive

Original authors: Trond I. Andersen, Nikita Astrakhantsev, Jeronimo Martinez, Will Morong, Johannes Motruk, Dario Rossi, Brayden Ware, Bryce Kobrin, Weijie Wu, Elizabeth Bennewitz, Manuel Rudolph, Tom Westerhout, Amira Abbas, Rajeev Acharya, Laleh Aghababaie Beni, Ross Alcaraz, Sayra Alcaraz, Markus Ansmann, Frank Arute, Kunal Arya, Walt Askew, Juan Atalaya, Christopher Ayala, Ryan Babbush, Brian Ballard, Joseph Bardin, Hector Bates, Andreas Bengtsson, Majid Bigdeli Karimi, Alexander Bilmes, Simon Bilodeau, Felix Borjans, Alexandre Bourassa, Jenna Bovaird, Dylan Bowers, Leon Brill, Peter Brooks, Michael Broughton, David Browne, Brett Buchea, Bob Buckley, Tim Burger, Brian Burkett, Jamal Busnaina, Nicholas Bushnell, Jonas Bylander, Anthony Cabrera, Juan Campero, Hung-Shen Chang, Silas Chen, Zijun Chen, Ben Chiaro, Liang-Ying Chih, Agnetta Cleland, Bryan Cochrane, Matt Cockrell, Josh Cogan, Paul Conner, Tom Connolly, Harold Cook, Rodrigo Cortinas, William Courtney, Alexander Crook, Benjamin Curtin, Adam Dally, Sayan Das, Martin Damyanov, Dripto Debroy, Himadri Dey, Stijn de Graaf, Laura De Lorenzo, Sean Demura, Lucia De Rose, Agustin Di Paolo, Leon Ding, Howard Dobbs, Paul Donohoe, Ebru Dogan, Ilya Drozdov, Andrew Dunsworth, Rasmus Edholm, Valerie Ehimhen, Alec Eickbusch, Aviv Elbag, Lior Ella, Mahmoud Elzouka, David Enriquez, Catherine Erickson, Lara Faoro, Vinicius Ferreira, Marcos Flores, Leslie Flores Burgos, Sam Fontes, Ebrahim Forati, Jeremiah Ford, Brooks Foxen, Masaya Fukami, Alan Fung, Lenny Fuste, Suhas Ganjam, Gonzalo Garcia, Christopher Garrick, Robert Gasca, Helge Gehring, Robert Geiger, Élie Genois, William Giang, Dar Gilboa, James Goeders, Edward Gonzales, Raja Gosula, Alejandro Grajales Dau, Dietrich Graumann, Joel Grebel, Alex Greene, Jonathan Gross, Jose Guerrero, Tan Ha., Steve Habegger, Tanner Hadick, Ali Hadjikhani, Michael Hamilton, Monica Hansen, Matthew Harrigan, Sean Harrington, Jeanne Hartshorn, Stephen Heslin, Paula Heu, Oscar Higgott, Reno Hiltermann, Jeremy Hilton, Hsin-Yuan Huang, Michael Hucka, Christopher Hudspeth, Ashley Huff, William Huggins, Aditya Jayaraman, Evan Jeffrey, Shaun Jevons, Zhang Jiang, Xiaoxuan Jin, Cody Jones, Chaitali Joshi, Kelsey Josund, Pavol Juhas, Andreas Kabel, Bharath Kannan, Hui Kang, Kiseo Kang, Amir Karamlou, Ryan Kaufman, Tanuj Khattar, Mostafa Khezri, Seon Kim, Paul Klimov, Can Knaut, Alexander Korotkov, Fedor Kostritsa, John Mark Kreikebaum, Ryuho Kudo, Arun Kumar, Ben Kueffler, Vladislav Kurilovich, Vitali Kutsko, Nathan Lacroix, Tiano Lange-Dei, Brandon Langley, Pavel Laptev, Kim-Ming Lau, Emma Leavell, Loïck Le Guevel, Justin Ledford, Joy Lee, Kenny Lee, Brian Lester, Wendy Leung, Matthew Lloyd, Lily Li, Wing Li, Ming Li, Alexander Lill, Mike Lindmark, William Livingston, Aditya Locharla, Erik Lucero, Daniel Lundahl, Aaron Lunt, Sid Madhuk, Donald Macaskill, Aniket Maiti, Ashley Maloney, Salvatore Mandra, Leigh Martin, Orion Martin, Eric Mascot, Paul Masih Das, Anselme Massimino, Melvin Mathews, Cameron Maxfield, Jarrod McClean, Matthew McEwen, Seneca Meeks, Anthony Megrant, Tim Menke, Kevin Miao, Zlatko Minev, Reza Molavi, Sebastian Molina, Shirin Montazeri, Akira Nakamura, Charles Neill, Konstantin Nesterov, Michael Newman, Roselle Ngaloy, Anthony Nguyen, Murray Nguyen, Chia-Hung Ni, Murphy Niu, Nicholas Noll, Sergey Novikov, Logan Oas, Ricky Oliver, Will Oliver, Raymond Orosco, Kristoffer Ottosson, Alice Pagano, Manan Patel, Sherman Peek, David Peterson, Alex Pizzuto, Thomas Plumb-Reyes, Elias Portoles, Rebecca Potter, Orion Pritchard, Sam Probst, Michael Qian, Chris Quintana, Matthew Rakher, Arpit Ranadive, Ganesh Ramachandran, Armin Razavi, Matthew Reagor, Rachel Resnick, David Rhodes, Daniel Riley, Gabrielle Roberts, Roberto Rodriguez, Emma Ropes, Eliott Rosenberg, Emma Rosenfeld, Dario Rosenstock, Elizabeth Rossi, Pedram Roushan, David Rower, Robert Salazar, Kannan Sankaragomathi, Murat Sarihan, Kevin Satzinger, Max Schaefer, Sebastian Schroeder, Henry Schurkus, Aria Shahingohar, Michael Shearn, Aaron Shorter, Shvarts Vladimir, Vlad Sivak, Spencer Small, W. Clarke Smith, David Sobel, Barrett Spells, Sofia Springer, George Sterling, Scott Stonemeyer, John Su, Jordan Suchard, Youngkyu Sung, Aaron Szasz, Alex Sztein, Tomoyuki Tanaka, Madeline Taylor, Jothi Thiruraman, Douglas Thor, Brandur Thorgrimsson, Dogan Timucin, Eifu Tomita, Alfredo Torres, M. Mert Torunbalci, Hao Tran, Abeer Vaishnav, Justin Vargas, Gopinath Vasalamarri, Sergey Vdovichev, Guifre Vidal, Benjamin Villalonga, Meghan Voorhees, Steven Waltman, Jonathan Waltz, Shannon Wang, Danni Wang, James Watson, Yonghua Wei, Travis Weidel, Theodore White, Kristi Wong, Bryan Woo, Christopher Wood, Maddy Woodson, Cheng Xing, Z. Jamie Yao, Ping Yeh, Bicheng Ying, Juhwan Yoo, Noureldin Yosri, Elliot Young, Grayson Young, Adam Zalcman, Ran Zhang, Yaxing Zhang, Yiqing Zhou, Ningfeng Zhu, Nicholas Zobrist, Zhenjie Zou, Sergio Boixo, Yu Chen, Julian Kelly, Hartmut Neven, Vadim Smelyanskiy, Dvir Kafri, L. B. Ioffe, Kostyantyn Kechedzhi, Xiao Mi, Dmitry Abanin

Original paper licensed under CC BY 4.0 (http://creativecommons.org/licenses/by/4.0/). This is an AI-generated explanation of the paper below. It is not written or endorsed by the authors. For technical accuracy, refer to the original paper. Read full disclaimer

Imagine you are trying to understand how a complex machine works, like a giant, invisible orchestra playing a symphony. In the world of physics, this "orchestra" is made of tiny particles called atoms, and the music they play is the behavior of materials—why some things are magnetic, why others conduct electricity without resistance, or how they change when heated. For decades, scientists have tried to predict this music using giant classical computers. But when the particles start acting in truly "quantum" ways—where they can be in many places at once and talk to each other instantly—these computers get overwhelmed, like a calculator trying to solve a puzzle that requires counting every grain of sand on a beach.

To solve this, physicists have built "quantum simulators." Think of these not as calculators, but as tiny, controllable versions of the real thing. Instead of just doing math on a screen, they use real quantum particles (like super-cooled atoms or superconducting circuits) to act out the physics. If you want to know how a magnet behaves, you build a tiny magnet out of these quantum particles and watch it dance. The big challenge has been getting these simulators to be precise enough to hear the faint, complex notes of the music, especially when the particles start bumping into each other and creating new, messy interactions. This paper is about finally tuning that instrument so perfectly that we can hear those messy notes clearly for the first time.


The Quantum Orchestra and the Magic Magnon

In this study, a team from Google Quantum AI and their collaborators decided to simulate a specific kind of magnetic material: a 2D magnet made of tiny spinning particles. In this world, the "spins" of these particles create waves, much like ripples on a pond. Scientists call these ripples magnons. You can think of a magnon as a single, quantized packet of spin-wave energy. Just as a photon is a packet of light, a magnon is a packet of magnetic vibration.

The researchers wanted to do two things: first, listen to the "linear" response (how a single ripple moves and fades), and second, watch what happens when they crash two ripples together (non-linear interactions). The problem is that in the real world, these ripples are incredibly hard to isolate and control. They usually get lost in the noise of the whole system.

The Hybrid Super-Processor

To tackle this, the team used a 97-qubit superconducting processor called "Willow." Imagine this processor as a giant, 2D grid of 97 tiny quantum switches (qubits). They didn't just let these switches run wild; they used a clever "analog-digital" trick.

Think of the analog part as letting the system evolve naturally, like letting a ball roll down a hill. This is fast and efficient but hard to control precisely. The digital part is like a human hand stepping in to nudge the ball at specific moments. The team interleaved these two: they let the quantum system evolve for a moment, then quickly injected a digital "nudge" (a gate) to create a specific magnon ripple, and then let it evolve again. This allowed them to create a single, clean ripple in a sea of quantum noise, something previous methods struggled to do.

Learning the Rules of the Game

Before they could trust their results, they had to know exactly how their quantum processor was behaving. No machine is perfect; the "hill" the ball rolls down might have tiny bumps or slopes they didn't expect. To fix this, they used a technique called Hamiltonian learning.

Imagine you are trying to learn the rules of a new board game by watching people play. You don't know the exact rules, but you can see the patterns of where the pieces end up. The team ran their quantum system, watched the patterns of the qubits (the "bitstrings"), and used a computer algorithm to "learn" the exact rules (the Hamiltonian) that the machine was actually following. They learned the rules with a precision of about 0.1% of the main interaction strength. This was crucial because it meant they knew exactly what they were simulating, removing the guesswork.

The Findings: Listening to the Ripples

Once the rules were learned and the system was tuned, they started their experiments.

  1. The Linear Symphony: They created single magnon ripples and watched how they moved and died out. They found that the "lifespan" of these ripples depended heavily on where they were in the grid.

    • The Van Hove Surprise: Near certain special points in the grid (called van Hove singularities), the ripples died out very quickly. It's like a ripple hitting a crowded dance floor where everyone is bumping into it, causing it to vanish fast.
    • The Edge Effect: Conversely, ripples that lived near the edges or corners of the grid were surprisingly long-lived. They were like dancers in a quiet corner, barely bumping into anyone. The team found that these "corner modes" were highly decoupled from the rest of the system.
  2. The Non-Linear Collision: Next, they turned up the volume. They didn't just watch one ripple; they smashed two ripples together to see how they interacted.

    • They discovered that when the ripples were small, they mostly scattered off the background heat (thermal modes).
    • But when they made the ripples bigger (increasing the amplitude), a new "self-scattering" channel opened up. The ripples started crashing into themselves.
    • Using a "pump-probe" technique (hitting one ripple hard and watching how it affected a weak one), they mapped out exactly which ripples talked to which. They found that the corner ripples were a special club: they mostly talked to each other and ignored the rest of the grid.

Why Classical Computers Couldn't Do This

The paper makes a strong point about why this was necessary. The team tried to simulate these exact same experiments using classical supercomputers with a method called Matrix Product States (MPS).

  • The Result: The classical simulations worked great when the system was cold or small. But as the temperature rose and the system got bigger (approaching the 97-qubit scale), the classical simulations failed. They couldn't capture the complex entanglement (the "spooky" connections between particles) that was happening.
  • The Conclusion: The paper suggests that to get the same accuracy as their quantum experiment, a classical computer would need resources that grow exponentially—essentially, it would need more memory than exists in the universe to simulate a system of this size at these temperatures.

The Bottom Line

This paper doesn't claim to have solved all the mysteries of magnetism. Instead, it demonstrates a new, high-precision way to watch quantum particles interact in real-time. By combining analog evolution with digital control and using machine learning to tune the system, they were able to measure how magnons scatter, decay, and interact with a level of detail that classical computers simply cannot reach. They showed that these quantum ripples have distinct personalities: some are social butterflies that scatter everywhere, while others are loners that stay in the corners. This work suggests that quantum processors are now ready to act as powerful microscopes for the microscopic world, helping us understand materials that are currently too complex for our best supercomputers to model.

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