Original title: Tidal forces in the quantum Oppenheimer--Snyder black hole
Anuar Idrissov, Hernando Quevedo · September 2026
In standard physics, falling into a black hole ends at a central point of infinite density, where tidal forces stretch you infinitely. Researchers wanted to know what happens when loop quantum gravityA theoretical framework that combines quantum mechanics with gravity to resolve singularities. is added to the model. This theory replaces the crushing center with a bouncing ball of dust. The researchers calculated the tidal forces acting on a falling object using a custom reference frame. They found that far away, gravity acts just like normal. But inside the black hole, the stretching and squeezing forces flip direction. An object dropped from rest never reaches the center. Instead, it stops at a turning point inside an inner boundary. The stretching force stays completely finite instead of blowing up to infinity. This safety comes directly from the bounce. If quantum effects are strong enough, the black hole loses its horizons entirely, putting this whole bouncing process in plain view.
Imagine packing a suitcase where the deeper you push clothes, the more resistance you feel. Normally, this resistance could become so extreme at the very bottom that it would destroy anything. In this quantum model, a mechanism acts like a shock absorber: as resistance builds, it suddenly reverses and decreases, so the clothes stop before hitting the bottom, avoiding destruction. This is similar to how particles falling into the quantum black hole experience tidal forces that peak and then soften, preventing infinite crushing.
This work addresses the singularity problem in black holes, where tidal forces become infinite and break physics. By showing they remain finite in a quantum model, it suggests a way to avoid this fundamental breakdown.
The study is limited to the quantum Oppenheimer-Snyder model and does not cover all black hole types. It is a theoretical analysis with no experimental confirmation. The results depend on a quantum parameter, and beyond a certain value, the geometry changes significantly.
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Tidal forces in the quantum Oppenheimer--Snyder black hole — Anuar Idrissov, Hernando Quevedo
Abstract licence: CC0
Explanation generated by Synthesis from the abstract — it is not the original paper. This is a preprint, so it hasn't necessarily been peer reviewed.