How a Black Hole Turns Off Particle Mass ✎ express

Original: "The Higgs vacuum in the presence of strong gravitational fields: curvature induced electroweak symmetry restoration"
· Paul G. Abel
arXiv:2607.24469 · 2026-07-27 · arXiv non-exclusive · independent analysis · 2 min
Inside a black hole, gravity may temporarily switch off the main mechanism that gives particles their mass.

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At the center of nearly every galaxy lurks a supermassive black hole. Its gravity is so strong that it warps space itself. But few stop to wonder: what does it do to the very fabric of reality — the fields that permeate the cosmos?

One such field is the Higgs field. Under normal conditions, it acts like a thick syrup: the more a particle 'gets stuck' in it, the heavier it becomes. Without it, electrons would be massless and would fly off at the speed of light, and atoms simply wouldn't form. The new work shows that inside a black hole, this syrup becomes increasingly thin. The culprit is the monstrous curvature of space, measured by a mathematical quantity — the Kretschmann scalar. The author introduces a coupling between the Higgs field and this curvature and finds: the closer to the hole's center, the weaker the field's influence. At some critical radius (for a typical stellar black hole, roughly one hundred-thousandth the size of an atomic nucleus), the Higgs field completely 'switches off.' Electroweak symmetry is restored, and particles stop feeling their familiar mass.

This critical point lies deep below the event horizon, but still far from the Planck scale, where spacetime is thought to dissolve into quantum foam. That means ordinary physics still applies there. It's a kind of 'pocket' inside the black hole where the usual laws of the microworld are temporarily suspended, yet the theory itself remains workable.

For a black hole with the mass of the Sun, the critical radius is about 10⁻²⁰ meters. That's a hundred thousand times smaller than a proton, but a billion times larger than the Planck length.
The Kretschmann scalar is a way to measure the curvature of empty space without matter. Inside a Schwarzschild black hole, it grows as 1/r⁶, meaning it increases very rapidly as you approach the center.

If the Higgs field suddenly vanished across the entire universe, electrons would become massless, and the size of atoms would grow to infinity, the world would instantly evaporate.

In Peter Watts's novel Blindsight, alien beings use fields reminiscent of the Higgs field to control their own biology and the space around them.

r_c \sim \left( \frac{\xi}{M_{Pl}} \right)^{1/3} r_s
The critical radius r_c at which the Higgs field vanishes: ξ is the dimensionless coupling constant, M_{Pl} is the Planck mass, and r_s is the gravitational radius of the black hole.
Scientists
Stephen HawkingJacob BekensteinJohn Archibald WheelerFritz ZwickyKarl SchwarzschildSubrahmanyan Chandrasekhar
Concepts
classical gravity schwarzschild metric black hole singularity gravitational field quantum gravity and symmetry higgs field higgs mechanism gravitational radius spacetime curvature schwarzschild black hole spin curvature coupling backreaction vacuum Schwinger effect kerr metric wald entropy flat space planck mass naked singularity logarithmic correction