A Shadow Matter Universe
| dc.creator | Lew, H. | |
| dc.date | 1993-03-12 | |
| dc.date.accessioned | 2026-07-07T03:55:58Z | |
| dc.date.available | 2026-07-07T03:55:58Z | |
| dc.description | The cosmological and astrophysical implications of a shadow matter model which could also have interesting experimental consequences are examined. The model has identical microphysics for both the ordinary and shadow worlds but requires a macroscopic asymmetry from nucleosynthesis constraints. It is proposed that this macroscopic asymmetry can be generated at the quark-hadron phase transition. | |
| dc.description | 11 pages (LaTeX), PURD-TH-93-04 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9303252 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9303252 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/44767 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | A Shadow Matter Universe | |
| dc.type | text |