Dark Stars: Cradle of Giant Black Holes express

Original: "Early Formation of Supermassive Black Holes via Dark Star Gravitational Instability"
arXiv:2511.08578 · 2025-11-11 · CC BY 4.0 · 1 min
In the infant Universe, stars powered by dark matter could grow to monstrous sizes and collapse into black holes.

Right after the Big Bang, unusual luminaries could be born — dark stars. Unlike the Sun, they didn’t burn nuclear fuel but fed on collisions of dark matter particles, which release energy. Like a snowball rolling downhill, such a star rapidly sucked in gas, gaining up to millions of solar masses. Its own gravity created enormous spacetime curvature, and the star collapsed into a black hole. This scenario was predicted by Subrahmanyan Chandrasekhar and Richard Feynman: no internal pressure can stop such a collapse. This is likely how the seeds of supermassive black holes, which we see in the centers of galaxies, formed. Without dark stars, ordinary stars wouldn’t have had enough time to grow these giants in the young Universe. Amazing fact: a million-solar-mass dark star would stretch out to Pluto’s orbit, yet its surface would be colder than an incandescent light bulb.

A giant dark star would span the distance from the Sun to Pluto, yet its surface would give off less heat than a household light bulb — a stunning contrast between size and temperature.

Scientists
Stephen HawkingJacob BekensteinFritz ZwickyBernhard RiemannJoseph WeberKarl Schwarzschild
Concepts
supermassive black hole growth supermassive black hole formation dark star quasistar nuclear reaction mass gap early universe star formation galaxy growth mechanisms hills mechanism stellar evolution Chandrasekhar limit dark matter subhalo quasar feedback early universe galaxies first stars nucleosynthesis starburst host galaxy microquasar population iii stars gravitational instability gas accretion