The Elusive Lightweight Black Hole: Key to Dark Matter? express

Original: "Implications for Primordial Black Hole Dark Matter from a Single Subsolar Mass Gravitational-wave Detection in LVK O1--O4"
arXiv:2602.21295 · 2026-02-24 · CC BY 4.0 · 1 min
Astronomers have spotted a black hole too lightweight to come from a star.

📄 Showing the "Simple" version — "Popular" is not ready yet. Add it to favorites to help prioritize it.

The gravitational waves detectors LIGO and Virgo picked up a deep rumble — the aftermath of two invisible objects merging. Their combined mass turned out to be less than the Sun's. Stellar evolution doesn't produce such lightweight black holes: a dying star doesn't collapse into such a tiny finale.

This signal has revived Stephen Hawking's hypothesis of primordial black holes — clumps of matter born in the first moments after the Big Bang, described by the Standard Model of physics. If this detected pair really is such relics, they could be part of dark matter, the invisible glue that holds galaxies together. Calculations allow that at least 4% of dark matter consists of such objects.

Here's the twist: a half-solar-mass black hole is just a couple of kilometers across: you could walk around it in half an hour, yet its pull is stronger than a star cluster's. The signal S251112cm is still being studied, but the lack of a visible flash is typical for black holes. Confirmation would open a direct path from spacetime ripples to solving the universe's composition.

A black hole with half the Sun's mass has a radius of about 1.5 kilometers, such an object could fit into a small town center, but would pull in everything around it with monstrous force.

Scientists
Stephen HawkingJacob BekensteinFritz ZwickyVera RubinKarl SchwarzschildSubrahmanyan Chandrasekhar
Concepts
intermediate mass black hole early universe black holes gw190814 mass ratio LIGO dark matter subhalo hills mechanism inspiral dark matter annihilation gwtc ringdown neutron star binary merger gravitational wave echoes m87 event axion detection hawking radiation mechanism binary star detection bubble collision primordial black hole