Q star

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by SpaceImplorerExplorerImplorer (talk | contribs) at 17:47, 6 April 2020 (→‎See also). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

A Q-Star, also known as a grey hole, is a hypothetical type of a compact, heavy neutron star with an exotic state of matter. Such a star can be smaller than the progenitor star's Schwarzschild radius and have a gravitational pull so strong that some, but not all light, cannot escape.[citation needed] 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

  1. ^ a b Kusenko, Alexander (2006). "Properties and signatures of supersymmetric Q-balls". arXiv:hep-ph/0612159. {{cite journal}}: Cite journal requires |journal= (help)

External links