Negative Feild and Positive Particle Newtonian pressure model

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Authors: Mark Chrisman
Cited by: 0

Abstract

Emergent Hubble Tension resolve from running simulations showing planetary ans star formations from pressure only, no pull gravity could match S.M. and we noticed our model had slightly steeper curve in a specific area. The steeper curve resolved Hubble Tension 100% with simulation not intended to do so. All data enclosed.

Fields of Study & Subjects

Cosmology and Gravitation Theories Relativity and Gravitational Theory Galaxies: Formation Evolution Phenomena

Publication details

Journal / source
Zenodo (CERN European Organization for Nuclear Research)
Publication date
3 March 2026
Language
EN
Document type
Dataset