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Heat-Resistant Quantum Memory ⚡ экспресс

Original: "A passive self-correcting quantum memory in three dimensions"
A new three-dimensional model lets a quantum bit persist for a very long time even in the heat.
Abstract

A three-dimensional Pauli stabilizer Hamiltonian is constructed, whose ground subspace encodes a qubit with an exponential lifetime when in contact with a thermal bath at non-zero temperature. The construction recursively applies a sequence of transformations to the original Hamiltonian, increasing the qubit storage time while preserving geometric locality in ℝ³. This demonstrates the possibility of self-correcting quantum memory in three dimensions at finite temperature. The method uses stabilizer codes with a recursive structure to achieve exponential growth of coherence time with system size. The result opens the way to fault-tolerant quantum computation without constant active error correction.

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A quantum bit (qubit) is a delicate thing. Even a little heat destroys it, like a random nudge topples a crystal wine glass. To protect this fragile information, physicists have built a three-dimensional quantum structure resembling a Russian doll.

Like a Russian doll: each new protective layer wraps more tightly around the qubit, making it nearly immune to thermal noise.

Inspired by the error-correction ideas of Shor and Preskill, the authors construct protection layer by layer. They take a simple energy landscape and gradually make it more complex, weaving in patterns of disorder (entropy) and order. Special stabilizers, named after Pauli, repel thermal disturbances. Thus, the qubit in the system’s ground state ends up securely hidden.

As a result, the information lifetime grows avalanchingly with each new layer — you can achieve storage longer than the age of the Universe. Usually, quantum states require cooling to near absolute zero, but here the protection works at realistic temperatures. This brings us closer to quantum chips without bulky refrigerators. A memory with stability comparable to a black hole challenges the standard model of decoherence.

🎯 At room temperature, quantum states usually decay in a split second. The new model promises a lifetime that grows avalanchingly with system size — theoretically longer than the age of the Universe.

Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinEmmy Noether
Tags
entropy Standard Model black hole
Laws
second law of thermodynamicsHawking radiationgravitational lensingNoether's theoremBekenstein-Hawking entropyEinstein field equations
Original: arXiv:2605.10943 · CC BY · bridge42worlds