The Higgs Field Opens a Passage Through a Black Hole ✛

Original: "The Higgs Field Governs the Interior Spacetime of Black Holes"
· Itzhak Bars
arXiv:2509.06800 · 2025-09-08 · CC BY 4.0 · 1 min
In extreme gravity, the Higgs field gives birth to antigravity, turning a black hole into a traversable region.

The Higgs field is an invisible ocean that fills the cosmos. In its calm state, its “waters” merely slow particles down slightly, creating the effect of mass. But at the heart of a black hole, monstrous gravity turns the ocean into a furious whirlpool: it not only pulls in but also pushes out with tremendous force. Antigravity emerges, counteracting spacetime curvature and preventing it from collapsing into a point.

This is a prediction of the i(SM+GR) theory, which unites Einstein’s gravity with the Standard Model of particles. Instead of a singularity, a dead end that Hawking and Penrose considered the end of physics, space continues. The black hole becomes a tunnel through which one can pass and perhaps glimpse the era before the Big Bang. The most surprising part: for all this to work, the Higgs field flips the sign of its energy — from a slowing agent to an accelerator of space.

The Higgs field is responsible for only a small fraction of the mass of ordinary matter, but without it, electrons would have no mass, and atoms could not exist.

A tunnel through a black hole resembles the wormholes of science fiction — bridges between distant corners of the universe.

R_- = -\frac{36\lambda}{8\pi \tilde{G}_N}
The curvature of the antigravity region is negative and determined by the parameter λ and the new gravitational constant G̃_N. This is anti-de Sitter space, shaped like a saddle.
Scientists
Roger PenroseEdward WittenJuan MaldacenaStephen HawkingJacob BekensteinFritz Zwicky
Concepts
higgs field black hole singularity gravitational field higgs mechanism classical gravity rotating black hole gravitational singularity semiclassical gravity supergravity scalar perturbations inner horizon Hawking area theorem Birkhoff's theorem horizon area general relativity schwarzschild metric host galaxy backreaction self interaction gravastar