{ "id": "1501.07837", "version": "v1", "published": "2015-01-30T16:49:49.000Z", "updated": "2015-01-30T16:49:49.000Z", "title": "Death by Dynamics: Planetoid-Induced Explosions on White Dwarfs", "authors": [ "Rosanne Di Stefano", "Robert Fisher", "James Guillochon", "James F. Steiner" ], "comment": "15 pages, 1 figure, 1 table", "categories": [ "astro-ph.HE", "astro-ph.SR" ], "abstract": "At intervals as short as ten thousand years, each white dwarf (WD) passes within a solar radius of a planetoid, i.e., a comet, asteroid, or planet. Gravitational tidal forces tear the planetoid apart; its metal-rich debris falls onto the WD, enriching the atmosphere. A third of WDs exhibit atmospheric \"pollution\". For roughly every hundred planetoid disruptions, a planetoid collides with a WD. We simulate a small number of collisions, in which \"death-by-dynamics\" refers to the fate of the planetoid. We also compute the energies and likely durations of a broad sample of collision events, and identify detection strategies at optical and X-ray wavelengths. Collisions with the most massive planetoids can be detected in external galaxies. Some may trigger nuclear burning. If one in $\\sim 10^7-10^8$ of WD-planetoid collisions creates the conditions needed for a Type Ia supernova (SN~Ia), \"death-by-dynamics\" would also refer to the fate of the WD, and could provide a novel channel for the production of SN~Ia. We consider the circumstances under which the rate of SNe~Ia can be increased by interactions with planetoids.", "revisions": [ { "version": "v1", "updated": "2015-01-30T16:49:49.000Z" } ], "analyses": { "keywords": [ "white dwarf", "planetoid-induced explosions", "gravitational tidal forces tear", "wd-planetoid collisions creates", "type ia supernova" ], "note": { "typesetting": "TeX", "pages": 15, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1342249 } } }