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Quantum Leap Through the Black Hole of Computation ⚡ экспресс

Original: "Exponential Quantum Speedup on Structured Hard Instances of Maximum Independent Set"
· Vicky Choi
arXiv:2601.17686 · 2026-01-25 · CC BY · ⏱ 1 min · Quantum Physics
A quantum algorithm with a special driver bypasses computational dead ends, leaving classical computers in the dust.
Abstract

Scientists have developed a quantum algorithm for hard maximum independent set problems (finding the largest set of objects not connected to each other). The key difference from standard quantum annealing is the use of a non-stochastic XX-driver, which incorporates quantum interference with sign changes. This provides access to a broader set of quantum states and allows the system to gracefully reach a solution, bypassing slow tunneling. On specially constructed examples, the algorithm is exponentially faster than classical methods and stochastic quantum annealing, finishing in polynomial time.

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Finding the largest group of strangers among a crowd is a challenge that pops up in logistics, chemistry, and scheduling. Ordinary computers hit a black hole here: not from lack of power, but because the problem's structure swallows any classical solution.

The new quantum algorithm sidesteps the trap. Instead of digging microscopic tunnels like standard annealing, it uses a driver that creates interference—as if colliding gravitational waves smooth out the bumps, forging a level route. The process stays smooth and keeps entropy low, like perfect order within a frozen star.

Thanks to this, for entire galaxies of specially designed problems, answers arrive in laughably short times, outrunning classical methods like the expansion of the universe outpaces light.

Astonishingly, scientists have built mini-models that can be run right now on existing quantum processors.
Back in the 1980s, Richard Feynman argued that nature cannot be simulated on classical machines. The new algorithm is living proof of that.

🎯 Standard quantum annealing is like trying to escape a black hole by clawing at its walls—the new one uses interference like a gravitational slingshot, hurling the solution toward the event horizon.

Scientists
Adam RiessBrian SchmidtEdwin HubbleGeorges LemaîtreMaarten SchmidtSaul Perlmutter
Tags
entropy black hole galaxy expansion of the universe
Laws
Hubble's lawsecond law of thermodynamicsHawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equations
Original: arXiv:2601.17686 · CC BY · bridge42worlds