No Astrophysical Dyadospheres
| dc.creator | Page, Don N. | |
| dc.date | 2006-05-18 | |
| dc.date.accessioned | 2026-07-07T07:08:28Z | |
| dc.date.available | 2026-07-07T07:08:28Z | |
| dc.description | It is shown how pair production itself would prevent the astrophysical formation of dyadospheres, hypothetical regions where the electric field exceeds the critical value for rapid Schwinger pair production. Pair production is a self-regulating process that would discharge a growing electric field, in the example of a hypothetical collapsing charged stellar core, before it reached 6% of the minimum dyadosphere value, keeping the pair production rate more than 26 orders of magnitude below the dyadosphere value, and keeping the efficiency below 0.0002(M/M_sun)^{1/2}. | |
| dc.description | 64 pages, LaTeX | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0605432 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0605432 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/110722 | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | No Astrophysical Dyadospheres | |
| dc.type | text |