Whether can the decision of the orthopositronium problem to stimulate studying the problem of a dark matter in the Universe?
| dc.creator | Levin, B. M. | |
| dc.creator | Sokolov, V. I. | |
| dc.date | 2006-10-03 | |
| dc.date.accessioned | 2026-07-07T07:26:50Z | |
| dc.date.available | 2026-07-07T07:26:50Z | |
| dc.description | The nature of a dark matter in the Universe can be connected with realization of the (plus/minus) Planck mass in final state of the beta-plus-decay of the nuclei Na-22, Ga-68, etc. and in a gravitational field of sufficient force. This hypothesis (the topological quantum transition - a generalized "displacement current") follows out of the phenomenological model that has explained the anomalies of the orthopositronium, forming in substance by the beta-decay positrons. Vacuumlike state of substance of the positive mass (Gliner, 1965) is structured in this model (the "microstructure" of vacuum) as the long-range "atom" with the Planck mass in the limited macroscopic "volume" of space-time. Accordingly, the negative mass C-field (Hoyle & Narlikar, 1964) plays the role of a compensating field. | |
| dc.description | 8 pages | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0610063 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0610063 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/117168 | |
| dc.subject | Astrophysics | |
| dc.title | Whether can the decision of the orthopositronium problem to stimulate studying the problem of a dark matter in the Universe? | |
| dc.type | text |