A New Signature of Dark Matter
| dc.creator | Abbas, S. | |
| dc.creator | Abbas, A. | |
| dc.creator | Mohanty, S. | |
| dc.date | 1997-09-06 | |
| dc.date | 1998-12-31 | |
| dc.date.accessioned | 2026-07-07T09:03:36Z | |
| dc.date.available | 2026-07-07T09:03:36Z | |
| dc.description | Dark matter capture and annihilation in planets and their satellites, in addition to producing neutrinos (already the basis of several ongoing experiments), is shown to lead to more significant heat generation in these bodies for a uniform dark matter halo. This thermal output becomes more prominent when clumped dark matter passes through the solar system. The dark matter annihilations should be treated as a new source of heat in the solar system which in some special cases may lead to unique imprints. Such new signatures of the dark matter are found in the generation of the puzzling magnetic field of Ganymede. This new source of heat perhaps cannot explain the formation and segregation of Ganymedean structure (which are probably due to conventional gravitational and radioactive heating), but provides a possible explanation of the origin of the Ganymedean magnetic field. | |
| dc.description | Revised substantially, 9 pages Latex | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9709269 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9709269 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/149074 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.subject | Geophysics | |
| dc.title | A New Signature of Dark Matter | |
| dc.type | text |