Our contribution to cosmology - The origin of matter and radiation

I review the strong-interaction sector of the cosmological evolution from early microsecond to early milliseconds in which we encounter the Quark-Gluon Plasma of non-perturbative QCD, followed by its hadronization at Hagedorn temperature, and finally the baryon-antibaryon annihilation leaving a small excess of nucleons, and radiation fields: the content of the present Universe.

Authors

Publication Details

Journal
Springer Link (Chiba Institute of Technology)
Published
2026-04-17
DOI
https://doi.org/10.1051/epjconf/202636401001/pdf
Primary Topic
High-Energy Particle Collisions Research
Type
article
Field-Weighted Citation Impact
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article

Our contribution to cosmology - The origin of matter and radiation

Reinhard Stock
Springer Link (Chiba Institute of Technology)
High-Energy Particle Collisions Research
article

Our contribution to cosmology - The origin of matter and radiation

Reinhard Stock
article en

Abstract

I review the strong-interaction sector of the cosmological evolution from early microsecond to early milliseconds in which we encounter the Quark-Gluon Plasma of non-perturbative QCD, followed by its hadronization at Hagedorn temperature, and finally the baryon-antibaryon annihilation leaving a small excess of nucleons, and radiation fields: the content of the present Universe.

Springer Link (Chiba Institute of Technology)
Openalex Percentile: Top 14%
High-Energy Particle Collisions Research
DOISourceOpenAlex
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Our contribution to cosmology - The origin of matter and radiation — Reinhard Stock · Springer Link (Chiba Institute of Technology) (2026) | TGRS Research Map | TGRS