Q star
From Infogalactic: the planetary knowledge core
<templatestyles src="Module:Hatnote/styles.css"></templatestyles>
A Q-Star, also known as a gray hole, is hypothetical type of a compact, heavy neutron star with an exotic state of matter. The Q stands for a conserved particle number. A Q-Star may be mistaken for a stellar black hole.
Types of Q-stars
- SUSY Q-ball[1]
- B-ball, stable Q-balls with a large baryon number B. They may exist in neutron stars that have absorbed Q-ball(s).[1]
See also
References
<templatestyles src="Reflist/styles.css" />
Cite error: Invalid <references> tag; parameter "group" is allowed only.
<references />, or <references group="..." />External links
- Abstract, Are Q-stars a serious threat for stellar-mass black hole candidates?, Miller J.C., Shahbaz T., Nolan L.A, 1997
- Abstract, No observational proof of the black-hole event-horizon, Marek A. Abramowicz, Wlodek Kluzniak, Jean-Pierre Lasota, 2002
| Types |
 |
|
|---|---|---|
| Size | ||
| Formation | ||
| Properties | ||
| Models | ||
| Issues | ||
| Metrics | ||
| Lists | ||
| Related | ||
| Evolution |
|
|---|---|
| Protostars | |
| Luminosity class | |
| Spectral classification |
|
| Remnants | |
| Theoretical stars | |
| Nucleosynthesis | |
| Structure | |
| Properties | |
| Star systems | |
| Earth-centric observation of |
|
| Lists | |
| Related articles | |
| Classes |
  |
|
|---|---|---|
| Physics of | ||
| Related | ||
| Progenitors | ||
| Remnants | ||
| Discovery | ||
| Lists | ||
| Notable | ||
| Research |
|
|
<templatestyles src="Asbox/styles.css"></templatestyles>
 |
This star-related article is a stub. You can help Wikipedia by expanding it. |
- ↑ 1.0 1.1 Properties and signatures of supersymmetric Q-balls, Alexander Kusenko, 2006
