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Q star
Hypothetical compact star From Wikipedia, the free encyclopedia
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A Q-star, also known as a grey hole, is a hypothetical type of 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 light, but not all light, can escape.[1] Light going in the opposite direction of the star’s center would be the most likely to escape from it, while light going in a direction almost parallel to its surface is the most likely not to escape. The Q stands for a conserved particle number. A Q-star may be mistaken for a stellar black hole.[2] Some stellar black holes might be grey holes, two of which are V404 Cygni and Cygnus X-1. [1]

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Types of Q-stars
- Q-ball[3]
- B-ball, stable Q-balls with a large baryon number B. They may exist in neutron stars that have absorbed Q-ball(s).[3]
See also
References
Further reading
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