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Einstein's Paradox: Why the Quantum World Can't Be Fooled ⚡ экспресс

Original: "A predictive solution of the EPR paradox"
· Henryk Gzyl
arXiv:2508.20788 · 2025-08-28 · CC BY 4.0 · ⏱ 1 min · Quantum Physics
The old debate about bypassing quantum uncertainty is finally settled.
Abstract

The Einstein–Podolsky–Rosen (EPR) paradox is considered: if you know a particle's exact momentum without measurement and then measure its position, you could obtain both values, contradicting the Heisenberg uncertainty principle. However, it is shown that the paradox does not arise if you correctly account for the quantum conditional expectation after measurement or use von Neumann's post-measurement state. These two methods are equivalent. In each, the prediction is given by an operator-valued function of the observables involved in the measurement. This formalism automatically ensures the preservation of uncertainty constraints.

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Photographing a bullet in flight: a short exposure gives a sharp position, but a blurred speed; a long exposure gives a sharp trajectory, but a blurred position. In the quantum world, this isn't a camera flaw — it's a fundamental law discovered by Werner Heisenberg. Albert Einstein devised a trick. Take two particles born in the same event, like two snapshots on a single frame. Measure the speed of the first, and the second will reveal the same speed. Then measure the position of the second, and it seems both parameters are known. But the moment you measure the position, the link breaks: the speed information vanishes, as if a darkroom fogged the finished print. New calculations close the case: you can’t fool quantum uncertainty.

Surprisingly, this unsuccessful attempt by Einstein laid the groundwork for quantum cryptography — the technology that today secures interbank transfers.

Nature is wise: by forbidding one thing, it opens another.

🎯 Though Einstein doubted quantum mechanics until the end of his life, his paradox helped develop the theory of quantum entanglement, which underpins quantum computers.

Scientists
Emmy NoetherJacob BekensteinStephen HawkingLudwig BoltzmannAlbert EinsteinRobert H. Dicke
Tags
Standard Model entropy spacetime curvature
Laws
second law of thermodynamicsNoether's theoremBekenstein-Hawking entropyBoltzmann distributionfirst law of thermodynamicsequivalence principle
Original: arXiv:2508.20788 · CC BY 4.0 · bridge42worlds