Chirality in the Early Universe
| dc.creator | Chang, Ngee Pong | |
| dc.date | 1995-12-30 | |
| dc.date.accessioned | 2026-07-07T03:58:43Z | |
| dc.date.available | 2026-07-07T03:58:43Z | |
| dc.description | The early big bang is an alphabet soup of quarks, W bosons, gluons, and other exotic particles and flavors. In the usual scenario, there is no place for the pion. It dissociates in the alphabet soup of the early universe. I will show that this scenario is naive. The thermal vacuum is a far more complex state, and the pion remains a Nambu-Goldstone particle at high $T$, and will not dissociate. It propagates at the speed of light but {\em with a halo}. | |
| dc.description | 6 pages, LaTeX. To appear in Proceedings of "International Conference on the Frontiers of Physics", Shantou, China, 5-9 August, 1995, to be published by World Scientific Publishers | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9512443 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9512443 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/45929 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Chirality in the Early Universe | |
| dc.type | text |