| Display title | Astronomy:Electroweak star |
| Default sort key | Electroweak Star |
| Page length (in bytes) | 4,795 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 374847 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
| Number of redirects to this page | 0 |
| Counted as a content page | Yes |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>HamTop |
| Date of page creation | 03:27, 27 June 2023 |
| Latest editor | imported>HamTop |
| Date of latest edit | 03:27, 27 June 2023 |
| Total number of edits | 1 |
| Recent number of edits (within past 90 days) | 0 |
| Recent number of distinct authors | 0 |
Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | An electroweak star is a theoretical type of exotic star, whereby the gravitational collapse of the star is prevented by radiation pressure resulting from electroweak burning, that is, the energy released by conversion of quarks to leptons through the electroweak force. This process occurs in a volume... |
