Английская Википедия:Dark star (dark matter)
Шаблон:Short description Шаблон:About
A dark star is a hypothetical type of star that may have existed early in the universe before conventional stars were able to form and thrive.
Properties
The dark stars would be composed mostly of normal matter, like modern stars, but a high concentration of neutralino dark matter present within them would generate heat via annihilation reactions between the dark-matter particles. This heat would prevent such stars from collapsing into the relatively compact and dense sizes of modern stars and therefore prevent nuclear fusion among the 'normal' matter atoms from being initiated.[1]
Under this model, a dark star is predicted to be an enormous cloud of molecular hydrogen and helium ranging between 1 and 960 astronomical units (AU) in radius and with a surface temperature and luminosity low enough that the emitted radiation would be invisible to the naked eye.[1][2]
In the unlikely event that dark stars have endured to the modern era, they could be detectable by their emissions of gamma rays, neutrinos, and antimatter and would be associated with clouds of cold molecular hydrogen gas that normally would not harbor such energetic, extreme, and rare particles.[3][2]
Possible dark star candidates
In April 2023, a study investigated four extremely redshifted objects discovered by the James Webb Space Telescope.[4] Their study suggested that three of these four, namely JADES-GS-z13-0, JADES-GS-z12-0, and JADES-GS-z11-0, are consistent with being point sources, and further suggested that the only point sources which could exist in this time and be bright enough to be observed at these phenomenal distances and redshifts (z = 10–13) were supermassive dark stars in the early universe, powered by dark matter annihilation.[4] Their spectral analysis of the objects suggested that they were between 500,000 and 1 million solar masses (Шаблон:Solar mass), as well as having a luminosity of billions of Suns (Шаблон:Solar luminosity); they would also likely be huge, possibly with radii surpassing 10,000 solar radii (Шаблон:Solar radius), far exceeding the size of the largest modern stars.[4]
See also
References
Further reading
- Шаблон:Cite conference
- Шаблон:Cite press release
- Шаблон:Cite conference
- Шаблон:Cite journal
- Шаблон:Cite journal
- Шаблон:Cite journal
- Шаблон:Cite journal
External links
- Шаблон:Cite press release
- Шаблон:Cite web
- Шаблон:Cite web
- Шаблон:Cite web
- Шаблон:Cite web
- Шаблон:Cite web
- Шаблон:Cite web
Шаблон:Star Шаблон:Dark matter Шаблон:Black holes
