Dark Matter: A Hidden Threat to Neutron Stars express

Original: "Compact Stars as Portals to Extra-Dimensional Dark Matter"
arXiv:2512.14837 · 2025-12-16 · CC BY 4.0 · 1 min
A tiny clump of dark matter can destroy a neutron star if space hides extra dimensions.

A neutron star is the compressed remnant of a sun: a mountain of matter the size of a thimble. If dark matter, the invisible substance that holds galaxies together, accumulates inside, under certain conditions it spells doom. In ordinary space, an incredible mass is needed, but hidden dimensions change the rules.

Gravity is curved spacetime, like a stretched trampoline. Dark matter particles, like tiny ball bearings, slightly dent it. Extra dimensions roll them into a leaden marble that tears the fabric — a black hole forms. Zwicky predicted neutron stars, Rubin proved the reality of dark matter; now their ideas converge in a terrifying scenario.

A twist: the miniature hole doesn't evaporate instantly — extra dimensions slow down the radiation. It devours the star whole, imposing strict limits on the properties of dark matter: particles heavier than tens of TeV are ruled out if the dimensions are real. In flat three-dimensional space, the threshold would be orders of magnitude higher — by millions.

Extra dimensions could be no larger than an atomic nucleus — about a femtometer, which is a billion times thinner than a hair.

Like in 'Interstellar,' where five-dimensional space helped survive a black hole — only here, hidden dimensions create that hole in the first place.

Scientists
Roger PenroseStephen HawkingVera RubinFritz ZwickyJacob BekensteinKarl Schwarzschild
Concepts
dark star stellar mass black hole neutron star dark matter supermassive black hole superdense matter Chandrasekhar limit stellar remnant nuclear reaction mass gap extra dimension quasistar metal poor ecdm model interstellar space gravastar population iii stars compact object terrestrial exoplanet galactic halo domain walls dimensionality