Black hole: Difference between revisions
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imported>Anthony Argyriou (explain rotating black hole) |
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Black holes are thought to be the result of collapsing matter following the explosion of large stars into [[supernova|supernovae]]. For a star to be capable of compaction into a singularity, it must have a mass greater than 3.4 times that of the Sun. Specifically, if the remnants of a star which has exhausted the energy available from [[nuclear fusion]] reactions are greater than about 3.4 times the mass of the [[sun]], [[electron degeneracy]] and [[neutron degeneracy]] are insufficient to prevent the star from collapsing into a black hole. Recent cosmology has considered the possibility of smaller black holes forming in the very early history of the universe, due to fluctuations in mass distribution when the density of the universe was significantly higher than is observed now. | Black holes are thought to be the result of collapsing matter following the explosion of large stars into [[supernova|supernovae]]. For a star to be capable of compaction into a singularity, it must have a mass greater than 3.4 times that of the Sun. Specifically, if the remnants of a star which has exhausted the energy available from [[nuclear fusion]] reactions are greater than about 3.4 times the mass of the [[sun]], [[electron degeneracy]] and [[neutron degeneracy]] are insufficient to prevent the star from collapsing into a black hole. Recent cosmology has considered the possibility of smaller black holes forming in the very early history of the universe, due to fluctuations in mass distribution when the density of the universe was significantly higher than is observed now. | ||
There are both rotating and stationary black holes, a [[singularity]] and event horizon(s) being the major features of both. The event horizon is the boundary of a black hole where gravitational forces become so strong that not even light can escape. Relativity states that the singularity is a point of infinite space time curvature, and the singularity of a black hole is covered by the event horizon. To an outside observer, objects falling into a black hole will take an [[infinity|infinite]] amount of time to reach the [[event horizon]]. However, the amount of time as measured by the object falling into the black hole can be very short. | There are both rotating and stationary black holes, a [[singularity]] and event horizon(s) being the major features of both. The event horizon is the boundary of a black hole where gravitational forces become so strong that not even light can escape. Relativity states that the singularity is a point of infinite space time curvature, and the singularity of a black hole is covered by the event horizon. To an outside observer, objects falling into a black hole will take an [[infinity|infinite]] amount of time to reach the [[event horizon]]. However, the amount of time as measured by the object falling into the black hole can be very short. A rotating black hole, according to the Kerr solutions of general relativity, will have two event horizons, and there are spacetime paths through the event horizon which do not intersect the singularity. | ||
According to [[quantum mechanics]], the location of the matter within a black hole is [[quantum uncertainty|uncertain]]. Additionally, a phenomenon called Hawking radiation predicts that black holes can "leak" a very small amount of mass. So theoretically, black holes are not truly "black" due to emitted radiation. Black holes have a surface temperature defined by their mass. The larger the [[mass]] of a black hole, the larger the diameter, and the lower the amount of energy which escapes, thus the lower the temperature, and the longer the time it takes for the black hole to "evaporate". | According to [[quantum mechanics]], the location of the matter within a black hole is [[quantum uncertainty|uncertain]]. Additionally, a phenomenon called Hawking radiation predicts that black holes can "leak" a very small amount of mass. So theoretically, black holes are not truly "black" due to emitted radiation. Black holes have a surface temperature defined by their mass. The larger the [[mass]] of a black hole, the larger the diameter, and the lower the amount of energy which escapes, thus the lower the temperature, and the longer the time it takes for the black hole to "evaporate". | ||
Revision as of 21:49, 20 June 2007
A black hole is an object in spacetime which has an escape velocity greater than c, the speed of light. Since light cannot escape, the object absorbs all light, hence the term black.
Black holes are thought to be the result of collapsing matter following the explosion of large stars into supernovae. For a star to be capable of compaction into a singularity, it must have a mass greater than 3.4 times that of the Sun. Specifically, if the remnants of a star which has exhausted the energy available from nuclear fusion reactions are greater than about 3.4 times the mass of the sun, electron degeneracy and neutron degeneracy are insufficient to prevent the star from collapsing into a black hole. Recent cosmology has considered the possibility of smaller black holes forming in the very early history of the universe, due to fluctuations in mass distribution when the density of the universe was significantly higher than is observed now.
There are both rotating and stationary black holes, a singularity and event horizon(s) being the major features of both. The event horizon is the boundary of a black hole where gravitational forces become so strong that not even light can escape. Relativity states that the singularity is a point of infinite space time curvature, and the singularity of a black hole is covered by the event horizon. To an outside observer, objects falling into a black hole will take an infinite amount of time to reach the event horizon. However, the amount of time as measured by the object falling into the black hole can be very short. A rotating black hole, according to the Kerr solutions of general relativity, will have two event horizons, and there are spacetime paths through the event horizon which do not intersect the singularity.
According to quantum mechanics, the location of the matter within a black hole is uncertain. Additionally, a phenomenon called Hawking radiation predicts that black holes can "leak" a very small amount of mass. So theoretically, black holes are not truly "black" due to emitted radiation. Black holes have a surface temperature defined by their mass. The larger the mass of a black hole, the larger the diameter, and the lower the amount of energy which escapes, thus the lower the temperature, and the longer the time it takes for the black hole to "evaporate".