Dahli Cosmological Model

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1. Verfasser: Chabane, Dahli
Format: Recurso digital
Sprache:Englisch
Veröffentlicht: Zenodo 2026
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author Chabane, Dahli
author_facet Chabane, Dahli
contents <p><span>We propose that the apparent “empty” intergalactic voids (</span><span>P</span><span>2</span><span>) are not a smooth</span></p> <p><span>Einsteinian spacetime with a quantum-field vacuum, but a granular lattice of microscopic white holes (MWs) – quanta of the pure cosmic vacuum – each formed by </span><span>the superposition of three mass-branes and stabilized by three contracted temporal </span><span>strings. Within galaxies (</span><span>P</span><span>1</span><span>), standard GR + QFT + the Standard Model remain </span><span>valid and fully successful; the “failures” of ΛCDM arise when those theories are </span><span>forced to describe the </span><span>P</span><span>2 </span><span>domain. This structural separation naturally explains </span><span>the absence of particle dark matter and predicts two observable consequences: (1) </span><span>a small, distance-dependent extra attenuation of TeV gamma-rays from distant </span><span>blazars/GRBs, and (2) a sub-percent modification of the Casimir force at 100 nm–1 </span><span>micrometer. Both effects provide laboratory and astrophysical tests of the granular </span><span>vacuum hypothesis</span> </p>
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language eng
publishDate 2026
publisher Zenodo
record_format zenodo
spellingShingle Dahli Cosmological Model
Chabane, Dahli
Granular vacuum
Microscopic white holes
String photons
Dark energy
Dark matter
Casimir effect
Intergalactic voids
Domain structure of spacetime
Stringmembrane cosmology
<p><span>We propose that the apparent “empty” intergalactic voids (</span><span>P</span><span>2</span><span>) are not a smooth</span></p> <p><span>Einsteinian spacetime with a quantum-field vacuum, but a granular lattice of microscopic white holes (MWs) – quanta of the pure cosmic vacuum – each formed by </span><span>the superposition of three mass-branes and stabilized by three contracted temporal </span><span>strings. Within galaxies (</span><span>P</span><span>1</span><span>), standard GR + QFT + the Standard Model remain </span><span>valid and fully successful; the “failures” of ΛCDM arise when those theories are </span><span>forced to describe the </span><span>P</span><span>2 </span><span>domain. This structural separation naturally explains </span><span>the absence of particle dark matter and predicts two observable consequences: (1) </span><span>a small, distance-dependent extra attenuation of TeV gamma-rays from distant </span><span>blazars/GRBs, and (2) a sub-percent modification of the Casimir force at 100 nm–1 </span><span>micrometer. Both effects provide laboratory and astrophysical tests of the granular </span><span>vacuum hypothesis</span> </p>
title Dahli Cosmological Model
topic Granular vacuum
Microscopic white holes
String photons
Dark energy
Dark matter
Casimir effect
Intergalactic voids
Domain structure of spacetime
Stringmembrane cosmology
url https://doi.org/10.5281/zenodo.18637031