What question did this study set out to answer?

To challenge the traditional view of intergalactic voids by proposing a granular model of cosmic vacuum.

February 10, 2026Open Access

The Granular Cosmic Vacuum

Puntos clave

To challenge the traditional view of intergalactic voids by proposing a granular model of cosmic vacuum.
Introduces the concept of microscopic white holes as basic units of the vacuum.
Explains structural separation of galaxies versus intergalactic voids.
Analyzes the predictions of modified vacuum behavior in quantum and astrophysical contexts.
Predicts attenuation of TeV γ-rays from distant blazars and GRBs due to vacuum structure.
Indicates a measurable change in the Casimir force at specific scales.
Demonstrates failure of ΛCDM model in explaining observed phenomena in P2 domain.

Resumen

We propose that the apparent “empty” intergalactic voids are not a smooth Einsteinian spacetime with a quantum-field vacuum, but a granular lattice of microscopic white holes (MWs) – quanta of pure cosmic vacuum – each formed by the superposition of three mass-branes and stabilized by three contracted temporal strings. Within galaxies (Pattern P1), standard GR + QFT + Standard Model remain valid; the “failures” of ΛCDM arise when those theories are forced to describe the P2 domain. This structural separation naturally explains the absence of particle dark matter and predicts two observable consequences: 1) a small, distance-dependent extra attenuation of TeV γ-rays from distant blazars/GRBs, and 2) a sub-percent modification of the Casimir force at 100 nm–1 µm scales. Both effects provide laboratory and astrophysical tests of the granular vacuum hypothesis.

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