| Issue |
EPJ Web Conf.
Volume 364, 2026
XXXI International Conference on Ultra-Relativistic Nucleus-Nucleus Collisions “Quark Matter 2025”
|
|
|---|---|---|
| Article Number | 01001 | |
| Number of page(s) | 9 | |
| Section | Plenary Sessions | |
| DOI | https://doi.org/10.1051/epjconf/202636401001 | |
| Published online | 17 April 2026 | |
https://doi.org/10.1051/epjconf/202636401001
Our contribution to cosmology - The origin of matter and radiation
Institut fuer Kernphysik, Goethe Universität, Frankfurt am Main, Germany
* e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
Published online: 17 April 2026
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.
© The Authors, published by EDP Sciences, 2026
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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