The Birth of a Gravastar: How a Star Escapes a Black Hole ✛ ✎

Original: "Formation of gravastars"
arXiv:2509.15302 · 2025-09-18 · arXiv non-exclusive · independent analysis · 1 min
A star's collapse can end not as a black hole, but as a gravastar, a bubble of dark energy.

A dying massive star usually shrinks into a black hole — a trap from which even light cannot escape. But another finale is possible: a gravastar — a bubble of dark energy, the mysterious force pushing the cosmos apart.

Simulations of a collapsing cloud revealed: deep in the center, a tiny nugget of dark energy is born. It inflates, like a soap bubble in a vacuum. Upon reaching the critical radius where a black hole would normally appear (first calculated by Karl Schwarzschild), the expansion halts. Infalling matter hangs suspended on the bubble — a stable gravastar is born. The surprise: inside, space stretches as rapidly as in the first moments after the Big Bang — a whole mini-universe beneath the shell.

For comparison: a neutron star resists gravity through particle repulsion, while a gravastar relies on the push of dark energy.

The trick doesn't always work. The star must be sufficiently 'fluffy': its mass-to-radius ratio (in special units) must be less than 3/8. Otherwise, collapse into a black hole is inevitable.

Inside a gravastar, space expands like a newborn Universe — a miniature cosmos hidden from us by a glowing shell.

\mathcal{C} = 3/8
Threshold value: if the mass-to-radius ratio is less than 3/8, a gravastar forms; otherwise, a black hole.
Scientists
Stephen HawkingJacob BekensteinFritz ZwickyBernhard RiemannJoseph WeberKarl Schwarzschild
Concepts
gravastar black hole formation quasistar direct collapse black holes gravitational instability star formation gas gravitational collapse obscured quasar apparent horizon gas disk host galaxy dark star event horizon stability white hole gap microquasar quasar feedback open cluster naked singularity tidal disruption event