A Black Hole as a Cloud of Spacetime Bits express

Original: "Black hole mergers as probes of spacetime's condensed degrees of freedom?"
· Arno Keppens, Lester Kurvers
arXiv:2605.18922 · 2026-05-18 · CC BY 4.0 · 1 min
The event horizon isn't an empty boundary: it's a dense clump of tiny 'atoms' of spacetime.

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The event horizon of a black hole is often depicted as a one-way membrane: everything falls in, nothing comes out. But what if it's not an empty boundary but a cloud of the tiniest 'bits' of spacetime itself? In a new study, physicists treat a black hole as a condensate of such bits — much like steam condensing into water droplets.

Every droplet has a surface, and for a black hole, the horizon plays that role. The area of this surface is linked to the number of bits, and hence to the amount of disorder, or entropy. The more bits, the heavier the hole and the larger its radius. This approach naturally explains why a black hole's entropy is so huge: it simply counts all the microscopic 'atoms' of space gathered at the horizon.

If a black hole is a condensate, then there's no point of infinite density inside. Instead, spacetime smoothly rearranges itself, avoiding a singularity.

Recent observations of black hole mergers, when two holes spiral into each other and merge into one, offer clues. The waves from such events carry the imprint of the horizon, and the data fit the condensate model. The cloud of bits quivers and oscillates like a stretched drumhead, and these vibrations can be heard in gravitational waves.

So a familiar image, a cloud gathered around an invisible center, returns to us with new meaning. The horizon turns out to be not a boundary of emptiness but the densest place in the universe, woven from the very fabric of space.

Original abstract

as written by the authors arXiv:2605.18922

Black hole physics currently lacks a fully coherent understanding of the black hole mass (density), entropy, and interior (non-)singularity. These concepts are related to the black hole radius, area (of the horizon), and volume (within the horizon), respectively, in the Schwarzschild solution to Einstein's field equations. In this work, we argue that these concepts can be given reasonable interpretations in terms of spacetime's thermodynamic degrees of freedom, which constitute the metric, when the black hole is considered as a condensate thereof. Recent observations of black hole merger events support our proposal.

If you could break a solar-mass black hole into 'atoms' of spacetime, their number would exceed the total number of atoms in the visible universe.

In Fred Hoyle's novel 'The Black Cloud,' an intelligent gas cloud exhibits properties reminiscent of a condensate: it gathers from diffuse matter and acquires internal structure — much like a black hole in the new hypothesis.

S \propto A
The entropy S of a black hole is proportional to the area A of its horizon
Scientists
Jacob BekensteinStephen HawkingJohn Archibald WheelerFritz ZwickyKarl SchwarzschildSubrahmanyan Chandrasekhar
Concepts
black hole entropy schwarzschild metric black hole thermodynamics horizon area wald entropy entropic shadow schwarzschild radius mass ratio mass inflation inner horizon logarithmic correction area Einstein field equations naked singularity kerr metric relativity modified gravity singularities singularity gravitational radius quantum gravity and symmetry