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Neutron stars could be more compact than black holes ⚡ экспресс

Original: "Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability"
arXiv:2605.19731 · 2026-05-19 · CC BY 4.0 · ⏱ 1 min · General Relativity High Energy HEP Theory
Tweaks to gravity allow neutron stars to become more compact than black holes.
Abstract

In general relativity, black holes represent the maximal compactness achievable. However, recent work has constructed neutron star solutions in quasi-topological gravity (QTG) that surpass the black-hole compactness bound. A detailed analysis of equilibrium configurations and radial stability in QTG is presented, using several representative equations of state and varying the gravitational coupling constant. The results reveal that in the high-central-density regime, the compactness exceeding the black-hole limit follows a universal behavior. Moreover, QTG corrections become increasingly significant at large densities and can render radially stable configurations that would be unstable in general relativity, across a broad parameter range. These findings confirm ultra-compact neutron stars as theoretically robust strong-field objects and motivate further exploration of their dynamical behavior and observational signatures.

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In the standard picture, black holes are the undisputed density champions: all their matter is squeezed into a single point. Imagine the entire mass of Mount Everest packed into a grain of salt. But physicists have found a theoretical trick. If you add tiny corrections to the ordinary law of gravity—corrections that only activate at mind-boggling densities—then neutron stars can crunch down even further, snatching the record. These corrections, born from spacetime curvature, act like extra support: the star doesn’t collapse into a black hole but stays as a sphere, just compressed to the absolute limit.

What’s more, in this state a neutron star can mimic a black hole: it’s so dense that light struggles to escape, yet it lacks an event horizon—that sinister point of no return.

Researchers tested different models, varying the composition and tweaking the theory’s parameters. It turns out the behavior of these stars is universal—what they’re made of doesn’t matter. They remain stable even where, according to Einstein, they’d be doomed to collapse. On top of that, these objects can churn out gravitational waves—ripples in spacetime picked up by detectors like LIGO. So, lurking in the depths of space, there might be “almost-black-holes,” and we can actually hear them.

🎯 If a sugar cube were made of neutron star stuff, it would weigh as much as Mount Everest.

🎬 In science fiction, super-dense “neutronium” is a favorite material for impenetrable armor, like in Star Trek.

Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
neutron star black hole spacetime curvature gravitational waves
Laws
Hawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsFermi–Dirac statisticsequivalence principle
Original: arXiv:2605.19731 · CC BY 4.0 · bridge42worlds