Display title | Astronomy:Phantom energy |
Default sort key | Phantom Energy |
Page length (in bytes) | 4,449 |
Namespace ID | 3024 |
Namespace | Astronomy |
Page ID | 376301 |
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>Wincert |
Date of page creation | 06:44, 6 February 2024 |
Latest editor | imported>Wincert |
Date of latest edit | 06:44, 6 February 2024 |
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. | Phantom energy is a hypothetical form of dark energy satisfying the equation of state $ P=w\rho c^{2} $ with $ w<-1 $. It possesses negative kinetic energy, and predicts expansion of the universe in excess of that predicted by a cosmological constant, which leads to a Big Rip. The idea of phantom... |