Thermonuclear Dynamo inside an Alfven Black Hole
| dc.creator | Winterberg, F. | |
| dc.date | 2008-02-22 | |
| dc.date.accessioned | 2026-07-07T09:22:53Z | |
| dc.date.available | 2026-07-07T09:22:53Z | |
| dc.description | As in an acoustic black hole where the fluid is moving faster than the speed of sound and where the sound waves are swept along, in an Alfven black hole the plasma is moving faster than the Alfven velocity, with the Alfven waves swept along and eliminated as the cause of the magneto hydrodynamic instabilities. To realize an Alfven black hole, it is proposed to bring a plasma into rapid rotation by radially arranged lumped parameter transmission lines intersecting the plasma under an oblique angle. The rotating plasma slides frictionless over magnetic mirror fields directed towards the rotating plasma, with the mirror fields generated by magnetic solenoids positioned at the end of each transmission line. It is then shown that, with this configuration one can realize a thermonuclear dynamo, which also can serve as the analogue of a magnetar. | |
| dc.description | 25 pages with 6 figures | |
| dc.identifier | https://arxiv.org/abs/0802.3406 | |
| dc.identifier | http://arxiv.org/abs/0802.3406 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/155534 | |
| dc.subject | Plasma Physics | |
| dc.title | Thermonuclear Dynamo inside an Alfven Black Hole | |
| dc.type | text |