Cosmology of a Heisenberg fluid
S.Joffily, M. Novello

TL;DR
This paper explores a cosmological model where the universe's large-scale structure is influenced by non-linear fermions following Heisenberg dynamics, offering a novel approach to understanding cosmic evolution.
Contribution
It introduces a new cosmological framework based on Heisenberg fermions, extending traditional models with non-linear fermionic interactions.
Findings
Demonstrates how Heisenberg fermions can drive cosmic expansion
Provides mathematical formulation of the model
Suggests potential implications for early universe physics
Abstract
We consider a scenario in which the global geometry of the universe is driven by non-linear fermions obeying Heisenberg dynamics.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Relativity and Gravitational Theory
