First principles cosmology of the Standard Model epoch
Daniel Friedan

TL;DR
This paper constructs a cosmological model from first principles within the Standard Model and General Relativity, describing a universe starting near a classical solution with dark matter as a classical gauge field effect, without additional physics.
Contribution
It presents a novel first-principles cosmology derived solely from the Standard Model and GR, with a specific initial state and dark matter as a classical gauge field effect.
Findings
Homogeneous, isotropic, flat universe from initial conditions
Dark matter emerges as a classical gauge field effect
No free parameters or physics beyond the Standard Model
Abstract
This is a short summary of a project to construct a first principles cosmology of the Standard Model epoch, the period starting shortly before the electro-weak transition. The cosmology is derived from a simple initial state entirely within the SM and General Relativity. The initial state is semi-classical -- concentrated near a classical solution of the SM equations of motion -- and is precisely specified by a few simple conditions. The dark matter is a classical effect, a coherent state of the SU(2)-weak gauge field and the Higgs field. The leading order, classical universe contains only the dark matter. Ordinary matter is a correction due to the fluctuations of the SM fields around the classical trajectory. The initial state produces a homogeneous, isotropic, flat universe. There are no adjustable parameters. No physics beyond the SM is invoked. Only the classical calculations have…
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Cosmology and Gravitation Theories · Relativity and Gravitational Theory
