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A Cosmic Net for Quantum Gravity ⚡ экспресс

Original: "A Renormalizable and Unitary Approach to Quantum Gravity"
arXiv:2605.17817 · 2026-05-18 · CC BY 4.0 · ⏱ 1 min · HEP Theory General Relativity
A new model adds an invisible field, making gravity predictable even in the world of atoms.
Abstract

Bringing together gravity and quantum theory usually leads to infinities. Scientists added an auxiliary field to the equations, which, like a strict inspector, keeps the calculations from running wild. This approach makes quantum gravity finite and returns us to ordinary Einstein theory in the everyday world. Will we finally be able to tame gravity?

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Gravity is a cosmic net: massive bodies stretch it, and lighter objects roll along its curves. But in the world of atoms, this net begins to tremble chaotically, producing infinite values in the equations. Spacetime curvature ceases to be smooth.

Usually, quantum corrections to gravity explode into infinities. The new idea introduces a strict constraint that tames them.

Physicists proposed adding an invisible field—a rigid scaffold that keeps the net from excessive shaking. Without it, even empty vacuum would possess monstrous energy: in every cubic centimeter lurked power capable of vaporizing Earth. With the scaffold, only moderate quantum tremors remain, and the theory makes sense—infinities vanish, information is not lost, as required by entropy, the measure of irreversible chaos.

For large bodies—planets, stars, galaxies—this quantum order changes nothing. The theory smoothly transitions into Einstein’s classical equations, confirmed by centuries of observations.

This is still a mathematical sketch, but it paves the way to unify the laws of the macro-world and micro-world.

🎯 Quantum gravity is a stubborn puzzle: a black hole’s strong field and the tiny scale of the nucleus demand mutually exclusive properties from the theory.

🎬 Such ideas echo the quest for a 'theory of everything,' which in science fiction grants mastery over space and time.

Scientists
Emmy NoetherJacob BekensteinStephen HawkingLudwig BoltzmannAlbert EinsteinRobert H. Dicke
Tags
spacetime curvature Standard Model entropy
Laws
second law of thermodynamicsNoether's theoremBekenstein-Hawking entropyBoltzmann distributionfirst law of thermodynamicsequivalence principle
Original: arXiv:2605.17817 · CC BY 4.0 · bridge42worlds