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A collapsar (a portmanteau word formed by "collapsed" + "star") is a star which has undergone gravitational collapse.[1] When a star no longer has enough fuel for significant fusion reactions, there are three possible outcomes, depending on the remnant star's mass: If it is less than the Chandrasekhar limit (1.4 solar masses), the star will stabilize and shrink, becoming a white dwarf; between the Chandrasekhar limit and the Tolman–Oppenheimer–Volkoff limit (approximately 2.9 M☉), it will become a neutron star; and above the Tolman–Oppenheimer–Volkoff limit, the star will become a black hole. However, it is theorized that the high density of neutron star cores allow for quark matter and, as a result, a star that is more massive than even the Tolman–Oppenheimer–Volkoff limit, yet still is not a black hole.[2]
| Stars |  | |
|---|---|---|
| Stellar processes | ||
| Collapse | ||
| Supernovae | ||
| Compact and exotic objects | ||
| Particles, forces, and interactions | ||
| Quantum theory | ||
| Degenerate matter | ||
| Related topics | ||
 | This article about stellar astronomy is a stub. You can help Wikipedia by expanding it. |
