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White hole

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710: 1023:. Depending on where the space-like hypersurface is chosen, the Einstein-Rosen bridge can either connect two black hole event horizons in each universe (with points in the interior of the bridge being part of the black hole region of the spacetime), or two white hole event horizons in each universe (with points in the interior of the bridge being part of the white hole region). It is impossible to use the bridge to cross from one universe to the other, however, because it is impossible to enter a white hole event horizon from the outside, and anyone entering a black hole horizon from either universe will inevitably hit the black hole singularity. 1031:– general relativity must also allow the time-reverse of this type of "realistic" black hole that forms from collapsing matter. The time-reversed case would be a white hole that has existed since the beginning of the universe, and that emits matter until it finally "explodes" and disappears. Despite the fact that such objects are permitted theoretically, they are not taken as seriously as black holes by physicists, since there would be no processes that would naturally lead to their formation; they could exist only if they were built into the initial conditions of the 1060:. In both cases, however, it is not possible to reach the region "in" the white hole, so the behavior of it - and, in particular, what may come out of it - is completely impossible to predict. In this sense, a white hole is a configuration according to which the evolution of the universe cannot be predicted, because it is not deterministic. A "bare singularity" is another example of a non-deterministic configuration, but does not have the status of a white hole, however, because there is no region inaccessible from a given region. In its basic conception, the 2616: 40: 2426: 861:, discussed below, the white hole event horizon in the past becomes a black hole event horizon in the future, so any object falling towards it will eventually reach the black hole horizon). Imagine a gravitational field, without a surface. Acceleration due to gravity is the greatest on the surface of any body. But since black holes lack a surface, acceleration due to gravity increases exponentially, but never reaches a final value as there is no considered surface in a singularity. 3446: 723: 3506: 902: 3530: 3456: 3482: 3518: 3494: 1003:
means that the interior black-hole region can contain a mix of particles that fell in from either universe (and thus an observer who fell in from one universe might be able to see light that fell in from the other one), and likewise particles from the interior white-hole region can escape into either universe. All four regions can be seen in a spacetime diagram that uses
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between crossing the horizon and passing the outside observer). The black hole/white hole appears "eternal" from the perspective of an outside observer, in the sense that particles traveling outward from the white hole interior region can pass the observer at any time, and particles traveling inward,
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argued that the time reversal of a black hole in thermal equilibrium results in a white hole in thermal equilibrium (each absorbing and emitting energy to equivalent degrees). Consequently, this may imply that black holes and white holes are reciprocal in structure, wherein the Hawking radiation from
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itself is a white hole. It further suggests that the emergence of a white hole, which was named a "Small Bang", is spontaneous—all the matter is ejected at a single pulse. Thus, unlike black holes, white holes cannot be continuously observed; rather, their effects can be detected only around the
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at extremely high densities. Such an interaction prevents the formation of a gravitational singularity. Instead, the collapsing matter on the other side of the event horizon reaches an enormous but finite density and rebounds, forming a regular Einstein–Rosen bridge. The other side of the bridge
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Just as there are two separate interior regions of the maximally extended spacetime, there are also two separate exterior regions, sometimes called two different "universes", with the second universe allowing us to extrapolate some possible particle trajectories in the two interior regions. This
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Depending on the type of black hole solution considered, there are several types of white holes. In the case of the Schwarzschild black hole mentioned above, a geodesic coming out of a white hole comes from the "gravitational singularity" it contains. In the case of a black hole possessing an
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Note that the maximally extended Schwarzschild metric describes an idealized black hole/white hole that exists eternally from the perspective of external observers; a more realistic black hole that forms at some particular time from a collapsing star would require a different metric. When the
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whose core contracts until it turns into a black hole. Such a configuration is not static: we start from a massive and extended body which contracts to give a black hole. The black hole therefore does not exist for all eternity, and there is no corresponding white hole.
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separation, giving what is called a 'space-like surface') and draw an "embedding diagram" depicting the curvature of space at that time, the embedding diagram will look like a tube connecting the two exterior regions, known as an "Einstein-Rosen bridge" or
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are born from the collapse of stars, white holes represent the theoretical birth of space, time, and potentially even universes. At the center, space and time do not end into a singularity, but continue across a short transition region where the
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infalling stellar matter is added to a diagram of a black hole's history, it removes the part of the diagram corresponding to the white hole interior region. But because the equations of general relativity are time-reversible – they exhibit
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A view of black holes first proposed in the late 1980s might be interpreted as shedding some light on the nature of classical white holes. Some researchers have proposed that when a black hole forms, a Big Bang may occur at the
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process that can lead to the formation of such a configuration, and imposing it from the creation of the universe amounts to assuming a very specific set of initial conditions which has no concrete motivation.
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like the one at the center of the black hole's interior. In order to satisfy this requirement, it turns out that in addition to the black hole interior region that particles enter when they fall through the
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In 2014, the idea of the Big Bang being produced by a supermassive white hole explosion was explored in the framework of a five-dimensional vacuum by Madriz Aguilar, Moreno and Bellini.
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away, it had been assumed that they were the seat of exotic physical phenomena such as a white hole, or a phenomenon of continuous creation of matter (see the article on the
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from the outside, there must be a separate white hole interior region, which allows us to extrapolate the trajectories of particles that an outside observer sees rising up
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an ordinary black hole is identified with a white hole's emission of energy and matter. Hawking's semi-classical argument is reproduced in a quantum mechanical
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Another widespread idea is that white holes would be very unstable, would last a very short time and even after forming could collapse and become black holes.
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Klebanov, Igor R. (October 2001). "TASI lectures: Introduction to the AdS/CFT correspondence". In Harvey, Jeffrey; Kachru, Shamit; Silverstein, Eva (eds.).
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At present, very few scientists believe in the existence of white holes and it is considered only a mathematical exercise with no real-world counterpart.
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theory of gravity extends general relativity by removing a constraint of the symmetry of the affine connection and regarding its antisymmetric part, the
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are violated by quantum effects. From this region, space and time emerge with the structure of a white hole interior, a possibility already suggested by
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Sitio oficial de la Nasa en donde se explica la cuestión: los cuásares fueron supuestos como agujeros blancos pero la hipótesis quedó descartada
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becomes a new, growing baby universe. For observers in the baby universe, the parent universe appears as the only white hole. Accordingly, the
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To be able to exist, a white hole must either arise from a physical process leading to its formation, or be present from the creation of the
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is the Einstein–Rosen interior of a black hole existing as one of possibly many inside a larger universe. The Big Bang was a nonsingular
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were discovered it was assumed that these were the sought-after white holes but this assumption has now been discarded.
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of constant time (a set of points that all have the same time coordinate, such that every point on the surface has a
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Descubren nuevas evidencias de la transición al blanco de los agujeros negros, Universidad Complutense de Madrid.
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White holes as a kind of "exit" from black holes, both types of singularities would probably be connected by a
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with a gas of radiation (not compulsory). Because a thermal-equilibrium state is time-reversal-invariant,
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has a white hole region in its past. This region does not exist for black holes that have formed through
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which will eventually reach the black hole interior region can also pass the observer at any time.
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should not have any "edges". For any possible trajectory of a free-falling particle (following a
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anime, as the radiance it exudes is both sentient and evil, known as the Light of Destruction.
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In this spacetime, it is possible to come up with coordinate systems such that if you pick a
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can be seen as a naked singularity in outer space, but does not correspond to a white hole.
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Finally, it has been postulated that white holes could be the temporal inverse of a
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spacetime. The horizontal direction is space and the vertical direction is time.
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Madriz Aguilar, José Edgar; Moreno, Claudia; Bellini, Mauricio (January 2014).
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A. Retter & S. Heller (2012). "The revival of white holes as Small Bangs".
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The possibility of the existence of white holes was put forward by cosmologist
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Cosmic Catastrophes: Exploding Stars, Black Holes, and Mapping the Universe
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End of Black Hole Is Starting of Big Bang – Discussed in Newsgroup in 1999
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In its mode of formation, a black hole comes from a residue of a massive
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with no charge and no rotation. Here, "maximally extended" implies that
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Unlike black holes for which there is a well-studied physical process,
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at which the observable universe had a finite, minimum scale factor.
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Barceló, Carlos; Carballo-Rubio, Raúl; Garay, Luis J (18 May 2017).
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anomalous gamma-ray burst that occurred in 2006 was a "white hole".
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generates a repulsive spin–spin interaction that is significant in
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and others have proposed that these supermassive black holes could
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event itself. The paper even proposed identifying a new group of
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Astronomers Alon Retter and Shlomo Heller suggest that the
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Forward to the Future 2:Back to the Past, with Interest...
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can escape from it. In this sense, it is the reverse of a
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Hawking, S. W. (1976). "Black Holes and Thermodynamics".
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Black Hole Physics: Basic Concepts and New Developments
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from the event horizon. For an observer outside using
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Like black holes, white holes have properties such as
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introduced the idea of white holes as a solution to
1115: 2186: 1886:Farhi, Edward & Guth, Alan H. (January 1987). 1858: 1785: 783:that cannot be entered from the outside, although 105: 3542: 2427:Embedding of the inverted Schwarzschild Solution 1128:Lee Smolin § Cosmological natural selection 1092:In view of the enormous quantities radiated by 2182: 2180: 1869:"Trou blanc : définition et explications" 1705:(1988). "БЁЛАЯ ДЫРА" [White hole]. In 1552: 1499: 2513: 1983:"Every Black Hole Contains Another Universe?" 1927:"Radial motion into an Einstein–Rosen bridge" 1650: 893:, whose time reversal is the same as itself. 748: 2252: 1701: 1276:serves as a major source of conflict in the 2177: 1769: 1742: 1289:serves as a very important location in the 3079:Magnetospheric eternally collapsing object 2520: 2506: 1738: 1736: 1313:appears in the animated television series 825:and may be essential for their formation. 755: 741: 2357: 2297: 2202: 2157: 2124: 2077: 2056: 2025: 2005: 1942: 1924: 1885: 1763: 1670: 1601: 1141:, which would create a new universe that 859:maximally extended Schwarzschild solution 2472:Forward to the Future 1:Trapped in Time! 1589: 900: 2457:Shockwave cosmology inside a Black Hole 2125:Roy Britt, Robert (17 September 2003). 2006:Popławski, Nikodem J. (November 2010). 1794: 1733: 1729:(in Russian). Наука. 1976. p. 310. 1470: 3543: 2501: 2139:from the original on 27 February 2024 1531: 1249: 1201: 1067: 3455: 1925:Popławski, Nikodem J. (April 2010). 2158:Moskowitz, Clara (17 August 2009). 2127:"Did cosmos begin as a black hole?" 1539:University of California, Riverside 889:is described by a thermal gas in a 13: 1651:Carlo Rovelli (10 December 2018). 905:A diagram of the structure of the 66: 14: 3587: 3571:Hypothetical astronomical objects 2462:Michio Kaku: Mr Parallel Universe 2420: 885:treatment, where a black hole in 3528: 3516: 3504: 3492: 3480: 3454: 3445: 3444: 2743:Tolman–Oppenheimer–Volkoff limit 2614: 2445:Schwarzschild Wormhole animation 1116:Big Bang/Supermassive White Hole 722: 721: 708: 38: 16:Hypothetical region of spacetime 2860:Innermost stable circular orbit 2527: 2390: 2333: 2322: 2273: 2246: 2235: 2151: 2118: 2050: 1999: 1991:. 12 April 2010. Archived from 1975: 1918: 1879: 1825: 1534:"Is the Big Bang a black hole?" 3286:Timeline of black hole physics 2404:(in Spanish). 17 December 2018 2316:10.1016/j.physletb.2013.12.005 2255:"Израильтяне нашли белую дыру" 2044:10.1016/j.physletb.2010.09.056 1961:10.1016/j.physletb.2010.03.029 1717: 1695: 1681:10.1103/PhysRevLett.121.241301 1644: 1583: 1546: 1525: 1493: 1464: 1: 3054:Nonsingular black hole models 2346:Classical and Quantum Gravity 1457: 1189:A 2012 paper argues that the 1153:Einstein–Cartan–Sciama–Kibble 1050:Reissner-Nordström black hole 1038: 907:maximally extended black hole 2429:2d plot White hole in Google 2253:Леонид Попов (27 May 2011). 2221:10.1016/j.newast.2011.07.003 1912:10.1016/0370-2693(87)90429-1 1509:The nature of space and time 1108:in the center of which is a 1005:Kruskal–Szekeres coordinates 775:is a hypothetical region of 7: 3276:Rossi X-ray Timing Explorer 3241:Hypercompact stellar system 3231:Gamma-ray burst progenitors 1745:"White Holes and Wormholes" 1593:Strings, Branes and Gravity 1323: 1316:Voltron: Legendary Defender 857:(though in the case of the 836: 219:Gravitational time dilation 21:White hole (disambiguation) 10: 3592: 2962:Black hole complementarity 2929:Bousso's holographic bound 2914:Quasi-periodic oscillation 2612: 2606:Malament–Hogarth spacetime 2096:10.1103/PhysRevD.85.107502 1805:Cambridge University Press 1795:Wheeler, J. Craig (2007). 1772:"Collapse to a black hole" 1620:10.1142/9789812799630_0007 1451:Many-worlds interpretation 1361:Conformal cyclic cosmology 1125: 1119: 896: 833:supermassive white holes. 339:Mathisson–Papapetrou–Dixon 180:Pseudo-Riemannian manifold 18: 3440: 3314: 3166: 3128: 3107: 3046: 3005: 2954: 2833:Gravitational singularity 2820: 2713: 2623: 2548: 2535: 2438:27 September 2011 at the 1658:American Physical Society 1471:Carroll, Sean M. (2004). 1346:Gravitational singularity 992:Schwarzschild coordinates 979:gravitational singularity 913:In the 1930s, physicists 3417:PSO J030947.49+271757.31 3342:SDSS J150243.09+111557.3 2875:Blandford–Znajek process 2376:10.1088/1361-6382/aa6962 1988:National Geographic News 1725: 955:Einstein field equations 819:Supermassive black holes 809:Einstein field equations 344:Hamilton–Jacobi–Einstein 324:Einstein field equations 147:Mathematical formulation 2673:Active galactic nucleus 2433:Schwarzschild Wormholes 1726:Вселенная, жизнь, разум 1711:ФИЗИЧЕСКАЯ ЭНЦИКЛОПЕДИЯ 1577:10.1103/PhysRevD.13.191 1143:expands outside of the 1110:supermassive black hole 868:, the black hole emits 3301:Tidal disruption event 3271:Supermassive dark star 3189:Black holes in fiction 3174:Outline of black holes 2807:Supermassive dark star 2726:Gravitational collapse 1532:Gibbs, Philip (1997). 1473:Spacetime and Geometry 1208:gravitational collapse 1029:Time reversal symmetry 1021:Schwarzschild wormhole 965:describing an eternal 949:in 1964, developed by 910: 872:and so it can come to 813:gravitational collapse 214:Gravitational redshift 107: 3561:Concepts in astronomy 3179:Black Hole Initiative 2992:Holographic principle 2450:21 April 1999 at the 1840:. Springer. pp.  904: 502:Weyl−Lewis−Papapetrou 457:Kerr–Newman–de Sitter 277:Einstein–Rosen bridge 209:Gravitational lensing 165:Equivalence principle 108: 2982:Final parsec problem 2941:Schwarzschild radius 2489:4 March 2016 at the 2477:4 March 2016 at the 1751:on 27 September 2011 1356:Black hole cosmology 1336:White hole cosmology 963:Schwarzschild metric 923:Einstein's equations 887:anti-de Sitter space 432:Einstein–Rosen waves 158:Fundamental concepts 47: 19:For other uses, see 3281:Superluminal motion 3256:Population III star 3226:Gravitational waves 3184:Black hole starship 2967:Information paradox 2368:2017CQGra..34j5007B 2308:2014PhLB..728..244M 2213:2012NewA...17...73R 2088:2012PhRvD..85j7502P 2036:2010PhLB..694..181P 1953:2010PhLB..687..110P 1904:1987PhLB..183..149F 1832:Frolov, Valeri P.; 1703:Старобинский, А. А. 1612:2001sbg..conf..615K 1569:1976PhRvD..13..191H 1501:Hawking, Stephen W. 1184:Shockwave cosmology 1174:observable universe 1132:Shockwave cosmology 1102:steady state theory 874:thermal equilibrium 805:eternal black holes 386:Kaluza–Klein theory 272:Minkowski spacetime 224:Gravitational waves 3566:General relativity 3115:Optical black hole 3028:Reissner–Nordström 2987:Firewall (physics) 2892:Gravitational lens 2058:Popławski, Nikodem 1995:on 27 August 2019. 1873:Techno-Science.net 1250:In popular culture 1202:Various hypotheses 1198:with white holes. 1068:Physical relevance 959:maximally extended 940:John Lighton Synge 936:Einstein equations 927:general relativity 915:Robert Oppenheimer 911: 769:general relativity 715:Physics portal 487:Oppenheimer–Snyder 427:Reissner–Nordström 319:Linearized gravity 267:Spacetime diagrams 170:Special relativity 103: 32:General relativity 3468: 3467: 3261:Supermassive star 3251:Naked singularity 3246:Membrane paradigm 2972:Cosmic censorship 2946:Spaghettification 2934:Immirzi parameter 2887:Hawking radiation 2828:Astrophysical jet 2797:Supermassive star 2787:Binary black hole 2721:Stellar evolution 2663:Intermediate-mass 2286:Physics Letters B 2066:Physical Review D 2013:Physics Letters B 1931:Physics Letters B 1892:Physics Letters B 1851:978-0-7923-5145-0 1818:978-0-521-85714-7 1770:Andrew Hamilton. 1743:Andrew Hamilton. 1629:978-981-02-4774-4 1556:Physical Review D 1518:978-0-691-14570-9 1411:Quantum mechanics 1381:Naked singularity 951:Nikolai Kardashev 870:Hawking radiation 866:quantum mechanics 765: 764: 398: 397: 284: 283: 3583: 3533: 3532: 3531: 3521: 3520: 3519: 3509: 3508: 3507: 3497: 3496: 3485: 3484: 3483: 3476: 3458: 3457: 3448: 3447: 3120:Sonic black hole 3069:Dark-energy star 2924:Bekenstein bound 2909:M–sigma relation 2838:Ring singularity 2618: 2522: 2515: 2508: 2499: 2498: 2414: 2413: 2411: 2409: 2394: 2388: 2387: 2361: 2337: 2331: 2326: 2320: 2319: 2301: 2277: 2271: 2270: 2268: 2266: 2261:on 4 August 2012 2257:. 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Archived from 1740: 1731: 1730: 1721: 1715: 1714: 1699: 1693: 1692: 1674: 1648: 1642: 1641: 1605: 1587: 1581: 1580: 1550: 1544: 1543: 1529: 1523: 1522: 1497: 1491: 1490: 1475:(5.7 ed.). 1468: 1267:of the same name 1196:gamma-ray bursts 1169:fermionic matter 1054:angular momentum 851:angular momentum 757: 750: 743: 730: 725: 724: 717: 713: 712: 497:van Stockum dust 482:Robertson–Walker 308: 307: 198: 197: 112: 110: 109: 104: 102: 101: 89: 81: 80: 62: 61: 42: 28: 27: 3591: 3590: 3586: 3585: 3584: 3582: 3581: 3580: 3541: 3540: 3539: 3529: 3527: 3517: 3515: 3505: 3503: 3491: 3481: 3479: 3471: 3469: 3464: 3436: 3412:ULAS J1342+0928 3372:SDSS J0849+1114 3357:Phoenix Cluster 3310: 3162: 3124: 3103: 3042: 3001: 2997:No-hair theorem 2950: 2904:Bondi accretion 2870:Penrose process 2816: 2782:Gamma-ray burst 2709: 2619: 2610: 2596:Direct collapse 2544: 2531: 2526: 2491:Wayback Machine 2479:Wayback Machine 2452:Wayback Machine 2440:Wayback Machine 2423: 2418: 2417: 2407: 2405: 2396: 2395: 2391: 2338: 2334: 2327: 2323: 2278: 2274: 2264: 2262: 2251: 2247: 2240: 2236: 2185: 2178: 2168: 2166: 2156: 2152: 2142: 2140: 2123: 2119: 2060:(29 May 2012). 2055: 2051: 2004: 2000: 1981: 1980: 1976: 1923: 1919: 1884: 1880: 1867: 1866: 1859: 1852: 1834:Igor D. Novikov 1830: 1826: 1819: 1793: 1786: 1776: 1774: 1768: 1764: 1754: 1752: 1741: 1734: 1727: 1723: 1722: 1718: 1700: 1696: 1649: 1645: 1630: 1588: 1584: 1551: 1547: 1530: 1526: 1519: 1498: 1494: 1487: 1469: 1465: 1460: 1455: 1401:Negative energy 1326: 1259:appears in the 1252: 1204: 1145:parent universe 1134: 1124: 1118: 1070: 1046:electric charge 1041: 961:version of the 919:Hartland Snyder 899: 878:Stephen Hawking 839: 827:Stephen Hawking 761: 720: 707: 706: 699: 698: 522: 521: 512: 511: 467:Lemaître–Tolman 412: 411: 400: 399: 391:Quantum gravity 378:Advanced theory 305: 304: 303: 286: 285: 234:Geodetic effect 195: 194: 185: 184: 160: 159: 143: 113: 94: 90: 85: 73: 69: 54: 50: 48: 45: 44: 24: 17: 12: 11: 5: 3589: 3579: 3578: 3573: 3568: 3563: 3558: 3553: 3538: 3537: 3525: 3513: 3501: 3489: 3466: 3465: 3463: 3462: 3452: 3441: 3438: 3437: 3435: 3434: 3432:Swift J1644+57 3429: 3424: 3419: 3414: 3409: 3404: 3399: 3394: 3389: 3384: 3382:MS 0735.6+7421 3379: 3374: 3369: 3364: 3359: 3354: 3349: 3347:Sagittarius A* 3344: 3339: 3334: 3329: 3324: 3318: 3316: 3312: 3311: 3309: 3308: 3303: 3298: 3293: 3288: 3283: 3278: 3273: 3268: 3263: 3258: 3253: 3248: 3243: 3238: 3233: 3228: 3223: 3222: 3221: 3216: 3206: 3201: 3196: 3191: 3186: 3181: 3176: 3170: 3168: 3164: 3163: 3161: 3160: 3155: 3150: 3145: 3140: 3134: 3132: 3126: 3125: 3123: 3122: 3117: 3111: 3109: 3105: 3104: 3102: 3101: 3096: 3091: 3086: 3081: 3076: 3071: 3066: 3061: 3056: 3050: 3048: 3044: 3043: 3041: 3040: 3035: 3030: 3025: 3020: 3009: 3007: 3003: 3002: 3000: 2999: 2994: 2989: 2984: 2979: 2974: 2969: 2964: 2958: 2956: 2952: 2951: 2949: 2948: 2943: 2938: 2937: 2936: 2926: 2921: 2919:Thermodynamics 2916: 2911: 2906: 2901: 2900: 2899: 2889: 2884: 2882:Accretion disk 2879: 2878: 2877: 2872: 2862: 2857: 2852: 2847: 2846: 2845: 2840: 2830: 2824: 2822: 2818: 2817: 2815: 2814: 2809: 2804: 2799: 2794: 2789: 2784: 2779: 2778: 2777: 2772: 2767: 2757: 2756: 2755: 2745: 2740: 2739: 2738: 2728: 2723: 2717: 2715: 2711: 2710: 2708: 2707: 2706: 2705: 2700: 2695: 2690: 2685: 2680: 2675: 2665: 2660: 2659: 2658: 2648: 2647: 2646: 2643: 2638: 2627: 2625: 2621: 2620: 2613: 2611: 2609: 2608: 2603: 2598: 2593: 2588: 2583: 2578: 2573: 2568: 2563: 2558: 2556:BTZ black hole 2552: 2550: 2546: 2545: 2543: 2542: 2536: 2533: 2532: 2525: 2524: 2517: 2510: 2502: 2494: 2493: 2481: 2469: 2464: 2459: 2454: 2442: 2430: 2422: 2421:External links 2419: 2416: 2415: 2389: 2352:(10): 105007. 2332: 2321: 2272: 2245: 2234: 2176: 2150: 2117: 2072:(10): 107502. 2049: 2020:(3): 181–185. 1998: 1974: 1917: 1898:(2): 149–155. 1878: 1857: 1850: 1824: 1817: 1784: 1762: 1732: 1716: 1707:ПРОХОРОВ, А.М. 1694: 1643: 1628: 1603:hep-th/0009139 1582: 1563:(2): 191–197. 1545: 1524: 1517: 1505:Penrose, Roger 1492: 1485: 1477:Addison-Wesley 1462: 1461: 1459: 1456: 1454: 1453: 1448: 1443: 1438: 1433: 1428: 1423: 1418: 1413: 1408: 1403: 1398: 1393: 1388: 1383: 1378: 1373: 1368: 1363: 1358: 1353: 1348: 1343: 1338: 1333: 1327: 1325: 1322: 1321: 1320: 1307: 1302:leads to this 1300:Brittle Hollow 1283: 1270: 1251: 1248: 1244: 1243: 1236: 1233: 1226: 1223: 1203: 1200: 1157:torsion tensor 1120:Main article: 1117: 1114: 1106:accretion disk 1069: 1066: 1040: 1037: 1007:(see figure). 898: 895: 838: 835: 763: 762: 760: 759: 752: 745: 737: 734: 733: 732: 731: 718: 701: 700: 697: 696: 689: 684: 679: 674: 669: 664: 659: 654: 649: 644: 639: 634: 629: 624: 619: 614: 609: 604: 599: 594: 589: 584: 579: 574: 569: 564: 559: 554: 549: 544: 539: 534: 529: 523: 519: 518: 517: 514: 513: 510: 509: 504: 499: 494: 489: 484: 479: 474: 469: 464: 459: 454: 449: 444: 439: 434: 429: 424: 413: 407: 406: 405: 402: 401: 396: 395: 394: 393: 388: 380: 379: 375: 374: 373: 372: 370:Post-Newtonian 367: 362: 354: 353: 349: 348: 347: 346: 341: 336: 331: 326: 321: 313: 312: 306: 302: 301: 298: 294: 293: 292: 291: 288: 287: 282: 281: 280: 279: 274: 269: 261: 260: 254: 253: 252: 251: 246: 241: 236: 231: 229:Frame-dragging 226: 221: 216: 211: 206: 204:Kepler problem 196: 192: 191: 190: 187: 186: 183: 182: 177: 172: 167: 161: 157: 156: 155: 152: 151: 150: 149: 144: 142: 141: 136: 131: 125: 123: 115: 114: 100: 97: 93: 88: 84: 79: 76: 72: 68: 65: 60: 57: 53: 43: 35: 34: 15: 9: 6: 4: 3: 2: 3588: 3577: 3574: 3572: 3569: 3567: 3564: 3562: 3559: 3557: 3554: 3552: 3549: 3548: 3546: 3536: 3526: 3524: 3514: 3512: 3502: 3500: 3495: 3490: 3488: 3478: 3477: 3474: 3461: 3453: 3451: 3443: 3442: 3439: 3433: 3430: 3428: 3425: 3423: 3420: 3418: 3415: 3413: 3410: 3408: 3407:Markarian 501 3405: 3403: 3400: 3398: 3395: 3393: 3390: 3388: 3385: 3383: 3380: 3378: 3375: 3373: 3370: 3368: 3365: 3363: 3360: 3358: 3355: 3353: 3350: 3348: 3345: 3343: 3340: 3338: 3335: 3333: 3332:XTE J1118+480 3330: 3328: 3327:XTE J1650-500 3325: 3323: 3320: 3319: 3317: 3313: 3307: 3304: 3302: 3299: 3297: 3294: 3292: 3289: 3287: 3284: 3282: 3279: 3277: 3274: 3272: 3269: 3267: 3264: 3262: 3259: 3257: 3254: 3252: 3249: 3247: 3244: 3242: 3239: 3237: 3234: 3232: 3229: 3227: 3224: 3220: 3217: 3215: 3212: 3211: 3210: 3207: 3205: 3202: 3200: 3197: 3195: 3192: 3190: 3187: 3185: 3182: 3180: 3177: 3175: 3172: 3171: 3169: 3165: 3159: 3156: 3154: 3151: 3149: 3146: 3144: 3141: 3139: 3136: 3135: 3133: 3131: 3127: 3121: 3118: 3116: 3113: 3112: 3110: 3106: 3100: 3097: 3095: 3092: 3090: 3087: 3085: 3082: 3080: 3077: 3075: 3072: 3070: 3067: 3065: 3062: 3060: 3057: 3055: 3052: 3051: 3049: 3045: 3039: 3036: 3034: 3031: 3029: 3026: 3024: 3021: 3018: 3014: 3013:Schwarzschild 3011: 3010: 3008: 3004: 2998: 2995: 2993: 2990: 2988: 2985: 2983: 2980: 2978: 2975: 2973: 2970: 2968: 2965: 2963: 2960: 2959: 2957: 2953: 2947: 2944: 2942: 2939: 2935: 2932: 2931: 2930: 2927: 2925: 2922: 2920: 2917: 2915: 2912: 2910: 2907: 2905: 2902: 2898: 2895: 2894: 2893: 2890: 2888: 2885: 2883: 2880: 2876: 2873: 2871: 2868: 2867: 2866: 2863: 2861: 2858: 2856: 2855:Photon sphere 2853: 2851: 2850:Event horizon 2848: 2844: 2841: 2839: 2836: 2835: 2834: 2831: 2829: 2826: 2825: 2823: 2819: 2813: 2810: 2808: 2805: 2803: 2800: 2798: 2795: 2793: 2790: 2788: 2785: 2783: 2780: 2776: 2775:Related links 2773: 2771: 2768: 2766: 2763: 2762: 2761: 2758: 2754: 2753:Related links 2751: 2750: 2749: 2746: 2744: 2741: 2737: 2736:Related links 2734: 2733: 2732: 2729: 2727: 2724: 2722: 2719: 2718: 2716: 2712: 2704: 2701: 2699: 2696: 2694: 2691: 2689: 2686: 2684: 2681: 2679: 2676: 2674: 2671: 2670: 2669: 2666: 2664: 2661: 2657: 2654: 2653: 2652: 2649: 2644: 2642: 2639: 2637: 2634: 2633: 2632: 2629: 2628: 2626: 2622: 2617: 2607: 2604: 2602: 2599: 2597: 2594: 2592: 2589: 2587: 2584: 2582: 2579: 2577: 2574: 2572: 2569: 2567: 2564: 2562: 2561:Schwarzschild 2559: 2557: 2554: 2553: 2551: 2547: 2541: 2538: 2537: 2534: 2530: 2523: 2518: 2516: 2511: 2509: 2504: 2503: 2500: 2496: 2492: 2488: 2485: 2482: 2480: 2476: 2473: 2470: 2468: 2465: 2463: 2460: 2458: 2455: 2453: 2449: 2446: 2443: 2441: 2437: 2434: 2431: 2428: 2425: 2424: 2403: 2399: 2393: 2385: 2381: 2377: 2373: 2369: 2365: 2360: 2355: 2351: 2347: 2343: 2336: 2330: 2325: 2317: 2313: 2309: 2305: 2300: 2295: 2291: 2287: 2283: 2276: 2260: 2256: 2249: 2243: 2238: 2230: 2226: 2222: 2218: 2214: 2210: 2205: 2200: 2196: 2192: 2191: 2190:New Astronomy 2183: 2181: 2165: 2161: 2154: 2138: 2134: 2133: 2128: 2121: 2113: 2109: 2105: 2101: 2097: 2093: 2089: 2085: 2080: 2075: 2071: 2067: 2063: 2059: 2053: 2045: 2041: 2037: 2033: 2028: 2023: 2019: 2015: 2014: 2009: 2002: 1994: 1990: 1989: 1984: 1978: 1970: 1966: 1962: 1958: 1954: 1950: 1945: 1940: 1936: 1932: 1928: 1921: 1913: 1909: 1905: 1901: 1897: 1893: 1889: 1882: 1874: 1870: 1864: 1862: 1853: 1847: 1843: 1839: 1835: 1828: 1820: 1814: 1810: 1806: 1801: 1800: 1791: 1789: 1773: 1766: 1750: 1746: 1739: 1737: 1728: 1720: 1712: 1708: 1704: 1698: 1690: 1686: 1682: 1678: 1673: 1668: 1664: 1660: 1659: 1654: 1647: 1639: 1635: 1631: 1625: 1621: 1617: 1613: 1609: 1604: 1599: 1595: 1594: 1586: 1578: 1574: 1570: 1566: 1562: 1558: 1557: 1549: 1541: 1540: 1535: 1528: 1520: 1514: 1510: 1506: 1502: 1496: 1488: 1486:0-8053-8732-3 1482: 1478: 1474: 1467: 1463: 1452: 1449: 1447: 1444: 1442: 1439: 1437: 1434: 1432: 1429: 1427: 1424: 1422: 1419: 1417: 1414: 1412: 1409: 1407: 1404: 1402: 1399: 1397: 1396:Negative mass 1394: 1392: 1389: 1387: 1384: 1382: 1379: 1377: 1376:Exotic matter 1374: 1372: 1369: 1367: 1364: 1362: 1359: 1357: 1354: 1352: 1349: 1347: 1344: 1342: 1339: 1337: 1334: 1332: 1331:Arrow of time 1329: 1328: 1318: 1317: 1312: 1308: 1305: 1301: 1297: 1296: 1292: 1288: 1284: 1281: 1280: 1275: 1271: 1268: 1264: 1263: 1258: 1254: 1253: 1247: 1241: 1237: 1234: 1231: 1227: 1224: 1221: 1217: 1213: 1212: 1211: 1209: 1199: 1197: 1192: 1187: 1185: 1181: 1179: 1175: 1170: 1166: 1165:Dirac spinors 1162: 1158: 1154: 1149: 1147: 1146: 1140: 1133: 1129: 1123: 1113: 1111: 1107: 1103: 1099: 1095: 1090: 1087: 1086:astrophysical 1083: 1078: 1075: 1065: 1063: 1059: 1055: 1051: 1048:ψ ** Ώ ** ώ ( 1047: 1036: 1034: 1030: 1024: 1022: 1017: 1013: 1008: 1006: 1000: 997: 993: 989: 985: 984:event horizon 980: 976: 972: 968: 964: 960: 957:known as the 956: 952: 948: 943: 941: 937: 932: 928: 924: 920: 916: 908: 903: 894: 892: 888: 884: 879: 875: 871: 867: 862: 860: 856: 855:event horizon 852: 848: 844: 834: 832: 828: 824: 820: 816: 814: 810: 806: 802: 798: 794: 790: 786: 782: 778: 774: 770: 758: 753: 751: 746: 744: 739: 738: 736: 735: 729: 719: 716: 711: 705: 704: 703: 702: 695: 694: 690: 688: 685: 683: 680: 678: 675: 673: 670: 668: 665: 663: 660: 658: 655: 653: 650: 648: 645: 643: 640: 638: 635: 633: 632:Chandrasekhar 630: 628: 625: 623: 620: 618: 615: 613: 610: 608: 605: 603: 600: 598: 595: 593: 590: 588: 585: 583: 580: 578: 575: 573: 570: 568: 565: 563: 560: 558: 555: 553: 550: 548: 547:Schwarzschild 545: 543: 540: 538: 535: 533: 530: 528: 525: 524: 516: 515: 508: 507:Hartle–Thorne 505: 503: 500: 498: 495: 493: 490: 488: 485: 483: 480: 478: 475: 473: 470: 468: 465: 463: 460: 458: 455: 453: 450: 448: 445: 443: 440: 438: 435: 433: 430: 428: 425: 422: 418: 417:Schwarzschild 415: 414: 410: 404: 403: 392: 389: 387: 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Index

White hole (disambiguation)
General relativity
Spacetime curvature schematic
Introduction
History
Timeline
Tests
Mathematical formulation
Equivalence principle
Special relativity
World line
Pseudo-Riemannian manifold
Kepler problem
Gravitational lensing
Gravitational redshift
Gravitational time dilation
Gravitational waves
Frame-dragging
Geodetic effect
Event horizon
Singularity
Black hole
Spacetime
Spacetime diagrams
Minkowski spacetime
Einstein–Rosen bridge
Linearized gravity
Einstein field equations
Friedmann
Geodesics

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