dorsal/arxiv
View SchemaDust acoustic wave in a strongly magnetized pair-dust plasma
| Authors | P. K. Shukla, M. Marklund |
|---|---|
| Categories | |
| ArXiv ID | physics/0503029 |
| URL | https://arxiv.org/abs/physics/0503029 |
| DOI | 10.1238/Physica.Topical.113a00036 |
| Journal | Physica Scripta T113, 36 (2004) |
Abstract
The existence of the dust acoustic wave (DAW) in a strongly magnetized electron-positron (pair)-dust plasma is demonstrated. In the DAW, the restoring force comes from the pressure of inertialess electrons and positrons, and the dust mass provides the inertia. The waves could be of interest in astrophysical settings such as the supernovae and pulsars, as well as in cluster explosions by intense laser beams in laboratory plasmas.
{
"annotation_id": "3761ff21-0f6e-43e4-8f20-e25f4209d311",
"date_created": "2026-03-02T18:00:56.930000Z",
"date_modified": "2026-03-02T18:00:56.930000Z",
"file_hash": "a13aa32f09a978997e8c8464395b0568418a883b9f12532b87954427da838ee4",
"private": false,
"record": {
"abstract": "The existence of the dust acoustic wave (DAW) in a strongly magnetized\nelectron-positron (pair)-dust plasma is demonstrated. In the DAW, the restoring\nforce comes from the pressure of inertialess electrons and positrons, and the\ndust mass provides the inertia. The waves could be of interest in astrophysical\nsettings such as the supernovae and pulsars, as well as in cluster explosions\nby intense laser beams in laboratory plasmas.",
"arxiv_id": "physics/0503029",
"authors": [
"P. K. Shukla",
"M. Marklund"
],
"categories": [
"physics.plasm-ph",
"astro-ph"
],
"doi": "10.1238/Physica.Topical.113a00036",
"journal_ref": "Physica Scripta T113, 36 (2004)",
"title": "Dust acoustic wave in a strongly magnetized pair-dust plasma",
"url": "https://arxiv.org/abs/physics/0503029"
},
"schema_id": "dorsal/arxiv",
"source": {
"execution_id": "c675d663-a280-44f2-a709-1b456b04b430",
"id": "arXiv Dataset IDs",
"type": "Model",
"variant": "snapshot-2026-03-01",
"version": "0.1.0"
},
"user_id": 1000002
}