Q Star
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 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 term Q-Star should not be mistaken for quark star, as the Q does not stand for quark, but rather for a conserved particle number. A Q-Star may be mistaken for a stellar black hole. One such candidate is the compact object in V404 Cyg. A quark star or strange star is a hypothetical type of exotic star composed of quark matter, or strange matter...
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 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 term Q-Star should not be mistaken for quark star, as the Q does not stand for quark, but rather for a conserved particle number. A Q-Star may be mistaken for a stellar black hole. One such candidate is the compact object in V404 Cyg. A quark star or strange star is a hypothetical type of exotic star composed of quark matter, or strange matter. These are ultra-dense phases of degenerate matter theorized to form inside particularly massive neutron stars. It is theorized that when the neutron-degenerate matter which makes up a neutron star is put under sufficient pressure due to the star''s gravity, the individual neutrons break down into their constituent quarks, up quarks and down quarks. Some of these quarks may then become strange quarks and form strange matter. The star then becomes known as a "quark star" or "strange star", similar to a single gigantic hadron (but bound by gravity rather than the strong force).
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