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Spherically symmetric spacetime

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22: 1737: 189:). The isometries are then interpreted as rotations and a spherically symmetric spacetime is often described as one whose metric is "invariant under rotations". The spacetime metric induces a metric on each orbit 2-sphere (and this induced metric must be a multiple of the metric of a 2-sphere). Conventionally, the metric on the 2-sphere is written in 1918: 758: 1547: 3240:
As these equations are effectively two-dimensional, they can be solved without overwhelming difficulty for a variety of assumptions about the nature of the infalling material (that is, for the assumption of a spherically symmetric black hole that is accreting charged or neutral dust, gas, plasma or
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which describes the gradient (in the free-falling tetrad frame) of the circumferential radius along the radial direction. This is not in general unity; compare, for example, to the standard Swarschild solution, or the Reissner–Nordström solution. The sign of
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is the inverse vierbein. The convention here and in what follows is that the roman indexes refer to the flat orthonormal tetrad frame, while the greek indexes refer to the coordinate frame. The inverse vierbein can be directly read off of the above metric as
1374: 551: 2037: 1732:{\displaystyle e_{\;\mu }^{i}={\begin{bmatrix}{\frac {1}{\alpha }}&0&0&0\\-{\frac {\beta _{t}}{\alpha \beta _{r}}}&{\frac {1}{\beta _{r}}}&0&0\\0&0&r&0\\0&0&0&r\sin \theta \\\end{bmatrix}}} 2814: 2741: 2118: 2539: 270: 1159: 2869: 2970: 1913:{\displaystyle e_{i}^{\;\mu }={\begin{bmatrix}\alpha &\beta _{t}&0&0\\0&\beta _{r}&0&0\\0&0&{\frac {1}{r}}&0\\0&0&0&{\frac {1}{r\sin \theta }}\\\end{bmatrix}}} 3235: 1501: 1263: 2533: 1433: 3023: 493: 2297: 2248: 2426:
These two relations on the circumferential radius provide another reason why this particular parameterization of the metric is convenient: it has a simple intuitive characterization.
828: 753:{\displaystyle ds^{2}=g_{\mu \nu }dx^{\mu }dx^{\nu }=-{\frac {dt^{2}}{\alpha ^{2}}}+{\frac {1}{\beta _{r}^{2}}}\left(dr-\beta _{t}{\frac {dt}{\alpha }}\right)^{2}+r^{2}\,g(\Omega ).} 1269: 968: 2421: 2388: 1926: 1195: 2472: 2175: 2148: 3053: 398: 2355: 2328: 2202: 1076: 1019: 921: 790: 39: 3073: 1539: 894: 988: 3150: 357: 3294:
Andrew J. S. Hamilton and Pedro P. Avelino, "The physics of the relativistic counter-streaming instability that drives mass inflation inside black holes" (2008),
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in the presence of radially moving matter or energy. Because spherically symmetric spacetimes are by definition irrotational, they are not realistic models of
2747: 2674: 2051: 2663:{\displaystyle \Gamma _{rtr}=-\beta _{t}{\frac {\partial \ln \alpha }{\partial r}}+{\frac {\partial \beta _{t}}{\partial r}}-\partial _{t}\ln \beta _{r}} 199: 86: 1084: 58: 2820: 2900: 292: 65: 1038: 408: 3166: 1439: 3326: 105: 1204: 1021:
can be interpreted as the radial derivative of the circumferential radius in a freely-falling frame; this becomes explicit in the
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in nature. However, their metrics are considerably simpler than those of rotating spacetimes, making them much easier to analyze.
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Note that the above metric is written as a sum of squares, and therefore it can be understood as explicitly encoding a
3318: 2976: 526: 178: 441: 32: 507: 2259: 2210: 328: 1369:{\displaystyle e_{\;\mu }^{r}dx^{\mu }={\frac {1}{\beta _{r}}}\left(dr-\beta _{t}{\frac {dt}{\alpha }}\right)} 795: 79: 3076: 2042:
The particularly simple form of the above is a prime motivating factor for working with the given metric.
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is defined so that it is the circumferential radius, that is, so that the proper circumference at radius
3153: 512: 436: 296: 295:. A spherically symmetric spacetime can be characterised in another way, namely, by using the notion of 2032:{\displaystyle (e_{\;\mu }^{i})^{T}e_{i}^{\;\nu }=e_{\mu }^{\;\;i}e_{i}^{\;\nu }=\delta _{\mu }^{\nu }} 327:, there are precisely 3 rotational Killing vector fields. Stated in another way, the dimension of the 307:
of Killing vector fields and thus generate these vector fields. For a spherically symmetric spacetime
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The vierbein relates vector fields in the coordinate frame to vector fields in the tetrad frame, as
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was the proper rate of change of the circumferential radius; this can now be explicitly written as
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similar to those of rotating spacetimes, and these typically have qualitative features (such as
3322: 190: 3058: 3258: 1509: 1046: 1022: 873: 500: 420: 401: 973: 3273: 3126: 2887: 2435: 333: 186: 138: 3311: 3106: 3082: 2891: 2883: 2809:{\displaystyle \Gamma _{\theta r\theta }=\Gamma _{\phi r\phi }={\frac {\beta _{r}}{r}}} 2736:{\displaystyle \Gamma _{\theta t\theta }=\Gamma _{\phi t\phi }={\frac {\beta _{t}}{r}}} 853: 833: 310: 166: 142: 2113:{\displaystyle \partial _{i}=e_{i}^{\;\mu }{\frac {\partial \;\;}{\partial x^{\mu }}}} 3343: 2177:
which is the radial derivative in the rest frame. By construction, as noted earlier,
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due to counter-moving streams of infalling matter in the interior of a black hole.
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Spherically symmetric models are not entirely inappropriate: many of them have
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scalar can be found in Hamilton & Avelino. The Einstein equations become
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Circumferential radius, given below, convenient for studying mass inflation.
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is the proper rate of change of the circumferential radius (that is, where
529:, sometimes used for studying static spherically symmetric perfect fluids. 1042: 1034: 145:) that are unaffected by rotation. One such application is the study of 265:{\displaystyle g_{\Omega }=d\theta ^{2}+\sin ^{2}\theta \,d\varphi ^{2}} 1742:
The vierbein itself is the inverse(-transpose) of the inverse vierbein
1154:{\displaystyle g_{\mu \nu }=\eta _{ij}\,e_{\;\mu }^{i}\,e_{\;\nu }^{j}} 119: 2864:{\displaystyle \Gamma _{\phi \theta \phi }={\frac {\cot \theta }{r}}} 182: 279:
Spherical symmetry is a characteristic feature of many solutions of
3299: 2965:{\displaystyle \nabla _{t}\beta _{t}=-{\frac {M}{r^{2}}}-4\pi rp} 400:. In general, none of these are time-like, as that would imply a 126:
are commonly used to obtain analytic and numerical solutions to
3230:{\displaystyle {\frac {2M}{r}}-1=\beta _{t}^{2}-\beta _{r}^{2}} 1496:{\displaystyle e_{\;\mu }^{\phi }dx^{\mu }=r\sin \theta d\phi } 415:
is necessarily isometric to a subset of the maximally extended
15: 1258:{\displaystyle e_{\;\mu }^{t}dx^{\mu }={\frac {dt}{\alpha }}} 276:
and so the full metric includes a term proportional to this.
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effectively determines "which way is down"; the sign of
2528:{\displaystyle \Gamma _{rtt}=-\partial _{r}\ln \alpha } 1428:{\displaystyle e_{\;\mu }^{\theta }dx^{\mu }=rd\theta } 3334:
See Section 6.1 for a discussion of spherical symmetry
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distinguishes incoming and outgoing frames, so that
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of this group are 2-spheres (ordinary 2-dimensional
2438:in the tetrad frame can be written in terms of the 792:is the standard metric on the unit radius 2-sphere 46:. Unsourced material may be challenged and removed. 3310: 3229: 3144: 3115: 3091: 3067: 3047: 3017: 2964: 2863: 2808: 2735: 2662: 2527: 2466: 2415: 2382: 2349: 2322: 2291: 2242: 2196: 2169: 2142: 2112: 2031: 1912: 1731: 1533: 1495: 1427: 1368: 1257: 1189: 1153: 1070: 1013: 982: 962: 915: 888: 862: 842: 822: 784: 752: 487: 392: 351: 319: 264: 1041:. That is, the metric tensor can be written as a 411:) that any spherically symmetric solution of the 2150:which is the proper time in the rest frame, and 303:. The isometries referred to above are actually 1541:. Written as a matrix, the inverse vierbein is 3018:{\displaystyle \nabla _{t}\beta _{r}=4\pi rf} 8: 896:. In this coordinate choice, the parameter 488:{\displaystyle x^{\mu }=(t,r,\theta ,\phi )} 3290: 3288: 2091: 2090: 2078: 2005: 1989: 1988: 1969: 1938: 1762: 1556: 1448: 1389: 1278: 1213: 1176: 1140: 1123: 3241:dark matter, of high or low temperature, 3221: 3216: 3203: 3198: 3170: 3168: 3128: 3108: 3084: 3060: 3039: 3033: 2994: 2984: 2978: 2939: 2930: 2918: 2908: 2902: 2843: 2828: 2822: 2795: 2789: 2774: 2755: 2749: 2722: 2716: 2701: 2682: 2676: 2654: 2638: 2614: 2604: 2575: 2569: 2547: 2541: 2510: 2488: 2482: 2452: 2446: 2401: 2395: 2368: 2362: 2341: 2335: 2314: 2308: 2292:{\displaystyle \beta _{r}=\partial _{r}r} 2280: 2267: 2261: 2243:{\displaystyle \beta _{t}=\partial _{t}r} 2231: 2218: 2212: 2188: 2182: 2161: 2155: 2134: 2128: 2101: 2084: 2077: 2072: 2059: 2053: 2023: 2018: 2004: 1999: 1987: 1982: 1968: 1963: 1953: 1943: 1937: 1928: 1881: 1847: 1817: 1788: 1771: 1761: 1756: 1750: 1650: 1641: 1630: 1616: 1610: 1578: 1570: 1561: 1555: 1549: 1511: 1466: 1453: 1447: 1441: 1407: 1394: 1388: 1382: 1346: 1340: 1314: 1305: 1296: 1283: 1277: 1271: 1240: 1231: 1218: 1212: 1206: 1181: 1175: 1169: 1145: 1139: 1134: 1128: 1122: 1117: 1108: 1092: 1086: 1059: 1053: 1005: 999: 975: 949: 934: 928: 907: 901: 875: 855: 835: 797: 768: 734: 728: 715: 695: 689: 662: 657: 648: 637: 626: 616: 604: 591: 575: 562: 553: 541:One popular metric, used in the study of 449: 443: 364: 335: 312: 256: 248: 236: 223: 207: 201: 106:Learn how and when to remove this message 2474:in the tetrad frame, which are given by 519:are round, and thus useful for studying 3284: 823:{\displaystyle \Omega =(\theta ,\phi )} 3055:is the covariant time derivative (and 2882:A complete set of expressions for the 2123:The most interesting of these two are 7: 963:{\displaystyle \beta _{t}=dr/d\tau } 44:adding citations to reliable sources 1506:where the signature was take to be 3123:the radial energy flux. The mass 3062: 3036: 2981: 2905: 2825: 2771: 2752: 2698: 2679: 2635: 2622: 2607: 2592: 2578: 2544: 2507: 2485: 2449: 2277: 2228: 2158: 2131: 2094: 2087: 2056: 799: 776: 741: 299:, which, in a very precise sense, 208: 14: 55:"Spherically symmetric spacetime" 124:spherically symmetric spacetimes 20: 2416:{\displaystyle \beta _{r}<0} 2383:{\displaystyle \beta _{r}>0} 159:spherically symmetric spacetime 31:needs additional citations for 3139: 3133: 3103:the isotropic pressure!), and 1950: 1930: 1528: 1513: 1190:{\displaystyle e_{\;\mu }^{i}} 817: 805: 779: 773: 744: 738: 482: 458: 381: 375: 346: 340: 1: 2467:{\displaystyle \Gamma _{ijk}} 2170:{\displaystyle \partial _{r}} 2143:{\displaystyle \partial _{t}} 537:Circumferential radius metric 503:are possible; these include: 431:Spherically symmetric metrics 169:contains a subgroup which is 1029:Orthonormal tetrad formalism 3319:University of Chicago Press 3048:{\displaystyle \nabla _{t}} 495:, to write the metric (the 393:{\displaystyle \dim K(M)=3} 293:Reissner–Nordström solution 3366: 2350:{\displaystyle \beta _{r}} 2323:{\displaystyle \beta _{r}} 2197:{\displaystyle \beta _{t}} 1071:{\displaystyle \eta _{ij}} 1014:{\displaystyle \beta _{r}} 916:{\displaystyle \beta _{t}} 785:{\displaystyle g(\Omega )} 527:Gaussian polar coordinates 305:local flow diffeomorphisms 281:Einstein's field equations 128:Einstein's field equations 2390:is an ingoing frame, and 1037:, and, in particular, an 508:Schwarzschild coordinates 435:Conventionally, one uses 3309:Wald, Robert M. (1984). 2039:is the identity matrix. 830:. The radial coordinate 3068:{\displaystyle \nabla } 3245:material with various 3231: 3146: 3117: 3093: 3077:Levi-Civita connection 3069: 3049: 3019: 2966: 2865: 2810: 2737: 2664: 2529: 2468: 2423:is an outgoing frame. 2417: 2384: 2351: 2324: 2293: 2244: 2198: 2171: 2144: 2114: 2033: 1914: 1733: 1535: 1534:{\displaystyle (-+++)} 1497: 1429: 1370: 1259: 1191: 1155: 1072: 1015: 984: 964: 917: 890: 889:{\displaystyle 2\pi r} 864: 844: 824: 786: 754: 489: 417:Schwarzschild solution 413:vacuum field equations 394: 353: 321: 289:Schwarzschild solution 266: 3232: 3147: 3118: 3099:the radial pressure ( 3094: 3070: 3050: 3020: 2967: 2874:and all others zero. 2866: 2811: 2738: 2665: 2530: 2469: 2418: 2385: 2352: 2325: 2294: 2245: 2199: 2172: 2145: 2115: 2034: 1915: 1734: 1536: 1498: 1430: 1371: 1260: 1192: 1156: 1073: 1016: 985: 983:{\displaystyle \tau } 965: 918: 891: 865: 845: 825: 787: 755: 513:Isotropic coordinates 490: 437:spherical coordinates 395: 354: 322: 297:Killing vector fields 267: 3350:Lorentzian manifolds 3269:Spacetime symmetries 3264:Stationary spacetime 3167: 3145:{\displaystyle M(r)} 3127: 3107: 3083: 3059: 3032: 2977: 2901: 2821: 2748: 2675: 2540: 2481: 2445: 2394: 2361: 2334: 2307: 2260: 2211: 2181: 2154: 2127: 2052: 1927: 1749: 1548: 1510: 1440: 1381: 1270: 1205: 1168: 1085: 1052: 998: 974: 927: 900: 874: 854: 834: 796: 767: 552: 442: 363: 352:{\displaystyle K(M)} 334: 311: 200: 175:rotation group SO(3) 40:improve this article 3226: 3208: 2440:Christoffel symbols 2253:Similarly, one has 2083: 2028: 2010: 1994: 1974: 1948: 1767: 1566: 1458: 1399: 1288: 1223: 1186: 1150: 1133: 923:is defined so that 667: 425:asymptotically flat 301:preserve the metric 3313:General Relativity 3247:equations of state 3227: 3212: 3194: 3154:Misner-Thorne mass 3142: 3113: 3089: 3065: 3045: 3015: 2962: 2878:Einstein equations 2861: 2806: 2733: 2660: 2525: 2464: 2413: 2380: 2347: 2320: 2289: 2240: 2194: 2167: 2140: 2110: 2068: 2029: 2014: 1995: 1978: 1959: 1933: 1910: 1904: 1752: 1729: 1723: 1551: 1531: 1493: 1443: 1425: 1384: 1366: 1273: 1255: 1208: 1187: 1171: 1151: 1135: 1118: 1068: 1039:orthonormal tetrad 1011: 980: 960: 913: 886: 860: 840: 820: 782: 750: 653: 485: 409:Birkhoff's theorem 390: 349: 317: 285:general relativity 262: 3183: 3116:{\displaystyle f} 3092:{\displaystyle p} 2945: 2859: 2804: 2731: 2629: 2599: 2108: 1900: 1855: 1656: 1637: 1586: 1359: 1320: 1253: 994:). The parameter 863:{\displaystyle r} 843:{\displaystyle r} 708: 668: 643: 501:coordinate charts 407:It is known (see 320:{\displaystyle M} 287:, especially the 191:polar coordinates 185:in 3-dimensional 153:Formal definition 116: 115: 108: 90: 3357: 3332: 3316: 3302: 3292: 3259:Static spacetime 3236: 3234: 3233: 3228: 3225: 3220: 3207: 3202: 3184: 3179: 3171: 3151: 3149: 3148: 3143: 3122: 3120: 3119: 3114: 3098: 3096: 3095: 3090: 3074: 3072: 3071: 3066: 3054: 3052: 3051: 3046: 3044: 3043: 3024: 3022: 3021: 3016: 2999: 2998: 2989: 2988: 2971: 2969: 2968: 2963: 2946: 2944: 2943: 2931: 2923: 2922: 2913: 2912: 2870: 2868: 2867: 2862: 2860: 2855: 2844: 2839: 2838: 2815: 2813: 2812: 2807: 2805: 2800: 2799: 2790: 2785: 2784: 2766: 2765: 2742: 2740: 2739: 2734: 2732: 2727: 2726: 2717: 2712: 2711: 2693: 2692: 2669: 2667: 2666: 2661: 2659: 2658: 2643: 2642: 2630: 2628: 2620: 2619: 2618: 2605: 2600: 2598: 2590: 2576: 2574: 2573: 2558: 2557: 2534: 2532: 2531: 2526: 2515: 2514: 2499: 2498: 2473: 2471: 2470: 2465: 2463: 2462: 2422: 2420: 2419: 2414: 2406: 2405: 2389: 2387: 2386: 2381: 2373: 2372: 2356: 2354: 2353: 2348: 2346: 2345: 2329: 2327: 2326: 2321: 2319: 2318: 2298: 2296: 2295: 2290: 2285: 2284: 2272: 2271: 2249: 2247: 2246: 2241: 2236: 2235: 2223: 2222: 2203: 2201: 2200: 2195: 2193: 2192: 2176: 2174: 2173: 2168: 2166: 2165: 2149: 2147: 2146: 2141: 2139: 2138: 2119: 2117: 2116: 2111: 2109: 2107: 2106: 2105: 2092: 2085: 2082: 2076: 2064: 2063: 2038: 2036: 2035: 2030: 2027: 2022: 2009: 2003: 1993: 1986: 1973: 1967: 1958: 1957: 1947: 1942: 1919: 1917: 1916: 1911: 1909: 1908: 1901: 1899: 1882: 1856: 1848: 1822: 1821: 1793: 1792: 1766: 1760: 1738: 1736: 1735: 1730: 1728: 1727: 1657: 1655: 1654: 1642: 1638: 1636: 1635: 1634: 1621: 1620: 1611: 1587: 1579: 1565: 1560: 1540: 1538: 1537: 1532: 1502: 1500: 1499: 1494: 1471: 1470: 1457: 1452: 1434: 1432: 1431: 1426: 1412: 1411: 1398: 1393: 1375: 1373: 1372: 1367: 1365: 1361: 1360: 1355: 1347: 1345: 1344: 1321: 1319: 1318: 1306: 1301: 1300: 1287: 1282: 1264: 1262: 1261: 1256: 1254: 1249: 1241: 1236: 1235: 1222: 1217: 1196: 1194: 1193: 1188: 1185: 1180: 1160: 1158: 1157: 1152: 1149: 1144: 1132: 1127: 1116: 1115: 1100: 1099: 1077: 1075: 1074: 1069: 1067: 1066: 1047:Minkowski metric 1023:tetrad formalism 1020: 1018: 1017: 1012: 1010: 1009: 989: 987: 986: 981: 969: 967: 966: 961: 953: 939: 938: 922: 920: 919: 914: 912: 911: 895: 893: 892: 887: 869: 867: 866: 861: 849: 847: 846: 841: 829: 827: 826: 821: 791: 789: 788: 783: 759: 757: 756: 751: 733: 732: 720: 719: 714: 710: 709: 704: 696: 694: 693: 669: 666: 661: 649: 644: 642: 641: 632: 631: 630: 617: 609: 608: 596: 595: 583: 582: 567: 566: 494: 492: 491: 486: 454: 453: 402:static spacetime 399: 397: 396: 391: 358: 356: 355: 350: 326: 324: 323: 318: 271: 269: 268: 263: 261: 260: 241: 240: 228: 227: 212: 211: 139:Penrose diagrams 111: 104: 100: 97: 91: 89: 48: 24: 16: 3365: 3364: 3360: 3359: 3358: 3356: 3355: 3354: 3340: 3339: 3329: 3308: 3305: 3293: 3286: 3282: 3274:De Sitter space 3255: 3172: 3165: 3164: 3125: 3124: 3105: 3104: 3081: 3080: 3057: 3056: 3035: 3030: 3029: 2990: 2980: 2975: 2974: 2935: 2914: 2904: 2899: 2898: 2888:Einstein tensor 2880: 2845: 2824: 2819: 2818: 2791: 2770: 2751: 2746: 2745: 2718: 2697: 2678: 2673: 2672: 2650: 2634: 2621: 2610: 2606: 2591: 2577: 2565: 2543: 2538: 2537: 2506: 2484: 2479: 2478: 2448: 2443: 2442: 2436:connection form 2432: 2430:Connection form 2397: 2392: 2391: 2364: 2359: 2358: 2337: 2332: 2331: 2310: 2305: 2304: 2276: 2263: 2258: 2257: 2227: 2214: 2209: 2208: 2184: 2179: 2178: 2157: 2152: 2151: 2130: 2125: 2124: 2097: 2093: 2086: 2055: 2050: 2049: 1949: 1925: 1924: 1903: 1902: 1886: 1879: 1874: 1869: 1863: 1862: 1857: 1845: 1840: 1834: 1833: 1828: 1823: 1813: 1811: 1805: 1804: 1799: 1794: 1784: 1782: 1772: 1747: 1746: 1722: 1721: 1707: 1702: 1697: 1691: 1690: 1685: 1680: 1675: 1669: 1668: 1663: 1658: 1646: 1639: 1626: 1622: 1612: 1604: 1603: 1598: 1593: 1588: 1571: 1546: 1545: 1508: 1507: 1462: 1438: 1437: 1403: 1379: 1378: 1348: 1336: 1326: 1322: 1310: 1292: 1268: 1267: 1242: 1227: 1203: 1202: 1166: 1165: 1104: 1088: 1083: 1082: 1055: 1050: 1049: 1031: 1001: 996: 995: 972: 971: 930: 925: 924: 903: 898: 897: 872: 871: 852: 851: 832: 831: 794: 793: 765: 764: 724: 697: 685: 675: 671: 670: 633: 622: 618: 600: 587: 571: 558: 550: 549: 539: 445: 440: 439: 433: 361: 360: 359:is 3; that is, 332: 331: 329:Killing algebra 309: 308: 252: 232: 219: 203: 198: 197: 187:Euclidean space 155: 143:Cauchy horizons 112: 101: 95: 92: 49: 47: 37: 25: 12: 11: 5: 3363: 3361: 3353: 3352: 3342: 3341: 3338: 3337: 3327: 3304: 3303: 3283: 3281: 3278: 3277: 3276: 3271: 3266: 3261: 3254: 3251: 3238: 3237: 3224: 3219: 3215: 3211: 3206: 3201: 3197: 3193: 3190: 3187: 3182: 3178: 3175: 3141: 3138: 3135: 3132: 3112: 3088: 3064: 3042: 3038: 3026: 3025: 3014: 3011: 3008: 3005: 3002: 2997: 2993: 2987: 2983: 2972: 2961: 2958: 2955: 2952: 2949: 2942: 2938: 2934: 2929: 2926: 2921: 2917: 2911: 2907: 2892:Weyl curvature 2884:Riemann tensor 2879: 2876: 2872: 2871: 2858: 2854: 2851: 2848: 2842: 2837: 2834: 2831: 2827: 2816: 2803: 2798: 2794: 2788: 2783: 2780: 2777: 2773: 2769: 2764: 2761: 2758: 2754: 2743: 2730: 2725: 2721: 2715: 2710: 2707: 2704: 2700: 2696: 2691: 2688: 2685: 2681: 2670: 2657: 2653: 2649: 2646: 2641: 2637: 2633: 2627: 2624: 2617: 2613: 2609: 2603: 2597: 2594: 2589: 2586: 2583: 2580: 2572: 2568: 2564: 2561: 2556: 2553: 2550: 2546: 2535: 2524: 2521: 2518: 2513: 2509: 2505: 2502: 2497: 2494: 2491: 2487: 2461: 2458: 2455: 2451: 2431: 2428: 2412: 2409: 2404: 2400: 2379: 2376: 2371: 2367: 2344: 2340: 2317: 2313: 2300: 2299: 2288: 2283: 2279: 2275: 2270: 2266: 2251: 2250: 2239: 2234: 2230: 2226: 2221: 2217: 2191: 2187: 2164: 2160: 2137: 2133: 2121: 2120: 2104: 2100: 2096: 2089: 2081: 2075: 2071: 2067: 2062: 2058: 2026: 2021: 2017: 2013: 2008: 2002: 1998: 1992: 1985: 1981: 1977: 1972: 1966: 1962: 1956: 1952: 1946: 1941: 1936: 1932: 1921: 1920: 1907: 1898: 1895: 1892: 1889: 1885: 1880: 1878: 1875: 1873: 1870: 1868: 1865: 1864: 1861: 1858: 1854: 1851: 1846: 1844: 1841: 1839: 1836: 1835: 1832: 1829: 1827: 1824: 1820: 1816: 1812: 1810: 1807: 1806: 1803: 1800: 1798: 1795: 1791: 1787: 1783: 1781: 1778: 1777: 1775: 1770: 1765: 1759: 1755: 1740: 1739: 1726: 1720: 1717: 1714: 1711: 1708: 1706: 1703: 1701: 1698: 1696: 1693: 1692: 1689: 1686: 1684: 1681: 1679: 1676: 1674: 1671: 1670: 1667: 1664: 1662: 1659: 1653: 1649: 1645: 1640: 1633: 1629: 1625: 1619: 1615: 1609: 1606: 1605: 1602: 1599: 1597: 1594: 1592: 1589: 1585: 1582: 1577: 1576: 1574: 1569: 1564: 1559: 1554: 1530: 1527: 1524: 1521: 1518: 1515: 1504: 1503: 1492: 1489: 1486: 1483: 1480: 1477: 1474: 1469: 1465: 1461: 1456: 1451: 1446: 1435: 1424: 1421: 1418: 1415: 1410: 1406: 1402: 1397: 1392: 1387: 1376: 1364: 1358: 1354: 1351: 1343: 1339: 1335: 1332: 1329: 1325: 1317: 1313: 1309: 1304: 1299: 1295: 1291: 1286: 1281: 1276: 1265: 1252: 1248: 1245: 1239: 1234: 1230: 1226: 1221: 1216: 1211: 1184: 1179: 1174: 1162: 1161: 1148: 1143: 1138: 1131: 1126: 1121: 1114: 1111: 1107: 1103: 1098: 1095: 1091: 1065: 1062: 1058: 1030: 1027: 1008: 1004: 979: 959: 956: 952: 948: 945: 942: 937: 933: 910: 906: 885: 882: 879: 859: 839: 819: 816: 813: 810: 807: 804: 801: 781: 778: 775: 772: 761: 760: 749: 746: 743: 740: 737: 731: 727: 723: 718: 713: 707: 703: 700: 692: 688: 684: 681: 678: 674: 665: 660: 656: 652: 647: 640: 636: 629: 625: 621: 615: 612: 607: 603: 599: 594: 590: 586: 581: 578: 574: 570: 565: 561: 557: 543:mass inflation 538: 535: 534: 533: 530: 524: 510: 484: 481: 478: 475: 472: 469: 466: 463: 460: 457: 452: 448: 432: 429: 389: 386: 383: 380: 377: 374: 371: 368: 348: 345: 342: 339: 316: 274: 273: 259: 255: 251: 247: 244: 239: 235: 231: 226: 222: 218: 215: 210: 206: 167:isometry group 154: 151: 147:mass inflation 114: 113: 28: 26: 19: 13: 10: 9: 6: 4: 3: 2: 3362: 3351: 3348: 3347: 3345: 3335: 3330: 3328:0-226-87033-2 3324: 3320: 3315: 3314: 3307: 3306: 3301: 3297: 3291: 3289: 3285: 3279: 3275: 3272: 3270: 3267: 3265: 3262: 3260: 3257: 3256: 3252: 3250: 3248: 3244: 3222: 3217: 3213: 3209: 3204: 3199: 3195: 3191: 3188: 3185: 3180: 3176: 3173: 3163: 3162: 3161: 3159: 3158:interior mass 3155: 3136: 3130: 3110: 3102: 3086: 3078: 3040: 3012: 3009: 3006: 3003: 3000: 2995: 2991: 2985: 2973: 2959: 2956: 2953: 2950: 2947: 2940: 2936: 2932: 2927: 2924: 2919: 2915: 2909: 2897: 2896: 2895: 2893: 2889: 2885: 2877: 2875: 2856: 2852: 2849: 2846: 2840: 2835: 2832: 2829: 2817: 2801: 2796: 2792: 2786: 2781: 2778: 2775: 2767: 2762: 2759: 2756: 2744: 2728: 2723: 2719: 2713: 2708: 2705: 2702: 2694: 2689: 2686: 2683: 2671: 2655: 2651: 2647: 2644: 2639: 2631: 2625: 2615: 2611: 2601: 2595: 2587: 2584: 2581: 2570: 2566: 2562: 2559: 2554: 2551: 2548: 2536: 2522: 2519: 2516: 2511: 2503: 2500: 2495: 2492: 2489: 2477: 2476: 2475: 2459: 2456: 2453: 2441: 2437: 2429: 2427: 2424: 2410: 2407: 2402: 2398: 2377: 2374: 2369: 2365: 2342: 2338: 2315: 2311: 2286: 2281: 2273: 2268: 2264: 2256: 2255: 2254: 2237: 2232: 2224: 2219: 2215: 2207: 2206: 2205: 2189: 2185: 2162: 2135: 2102: 2098: 2079: 2073: 2069: 2065: 2060: 2048: 2047: 2046: 2043: 2040: 2024: 2019: 2015: 2011: 2006: 2000: 1996: 1990: 1983: 1979: 1975: 1970: 1964: 1960: 1954: 1944: 1939: 1934: 1905: 1896: 1893: 1890: 1887: 1883: 1876: 1871: 1866: 1859: 1852: 1849: 1842: 1837: 1830: 1825: 1818: 1814: 1808: 1801: 1796: 1789: 1785: 1779: 1773: 1768: 1763: 1757: 1753: 1745: 1744: 1743: 1724: 1718: 1715: 1712: 1709: 1704: 1699: 1694: 1687: 1682: 1677: 1672: 1665: 1660: 1651: 1647: 1643: 1631: 1627: 1623: 1617: 1613: 1607: 1600: 1595: 1590: 1583: 1580: 1572: 1567: 1562: 1557: 1552: 1544: 1543: 1542: 1525: 1522: 1519: 1516: 1490: 1487: 1484: 1481: 1478: 1475: 1472: 1467: 1463: 1459: 1454: 1449: 1444: 1436: 1422: 1419: 1416: 1413: 1408: 1404: 1400: 1395: 1390: 1385: 1377: 1362: 1356: 1352: 1349: 1341: 1337: 1333: 1330: 1327: 1323: 1315: 1311: 1307: 1302: 1297: 1293: 1289: 1284: 1279: 1274: 1266: 1250: 1246: 1243: 1237: 1232: 1228: 1224: 1219: 1214: 1209: 1201: 1200: 1199: 1182: 1177: 1172: 1146: 1141: 1136: 1129: 1124: 1119: 1112: 1109: 1105: 1101: 1096: 1093: 1089: 1081: 1080: 1079: 1063: 1060: 1056: 1048: 1044: 1040: 1036: 1028: 1026: 1024: 1006: 1002: 993: 977: 957: 954: 950: 946: 943: 940: 935: 931: 908: 904: 883: 880: 877: 857: 837: 814: 811: 808: 802: 770: 747: 735: 729: 725: 721: 716: 711: 705: 701: 698: 690: 686: 682: 679: 676: 672: 663: 658: 654: 650: 645: 638: 634: 627: 623: 619: 613: 610: 605: 601: 597: 592: 588: 584: 579: 576: 572: 568: 563: 559: 555: 548: 547: 546: 544: 536: 531: 528: 525: 522: 518: 514: 511: 509: 506: 505: 504: 502: 498: 479: 476: 473: 470: 467: 464: 461: 455: 450: 446: 438: 430: 428: 426: 422: 418: 414: 410: 405: 403: 387: 384: 378: 372: 369: 366: 343: 337: 330: 314: 306: 302: 298: 294: 290: 286: 282: 277: 257: 253: 249: 245: 242: 237: 233: 229: 224: 220: 216: 213: 204: 196: 195: 194: 192: 188: 184: 180: 176: 172: 168: 164: 160: 152: 150: 148: 144: 140: 135: 133: 129: 125: 121: 110: 107: 99: 88: 85: 81: 78: 74: 71: 67: 64: 60: 57: â€“  56: 52: 51:Find sources: 45: 41: 35: 34: 29:This article 27: 23: 18: 17: 3333: 3312: 3242: 3239: 3100: 3027: 2881: 2873: 2433: 2425: 2301: 2252: 2122: 2044: 2041: 1922: 1741: 1505: 1163: 1032: 762: 540: 497:line element 434: 406: 278: 275: 158: 156: 136: 123: 117: 102: 96:October 2020 93: 83: 76: 69: 62: 50: 38:Please help 33:verification 30: 3317:. Chicago: 3160:, given by 992:proper time 517:light cones 515:, in which 499:). Several 132:black holes 3280:References 1164:where the 521:null dusts 171:isomorphic 66:newspapers 3300:0811.1926 3214:β 3210:− 3196:β 3186:− 3063:∇ 3037:∇ 3007:π 2992:β 2982:∇ 2954:π 2948:− 2928:− 2916:β 2906:∇ 2853:θ 2850:⁡ 2836:ϕ 2833:θ 2830:ϕ 2826:Γ 2793:β 2782:ϕ 2776:ϕ 2772:Γ 2763:θ 2757:θ 2753:Γ 2720:β 2709:ϕ 2703:ϕ 2699:Γ 2690:θ 2684:θ 2680:Γ 2652:β 2648:⁡ 2636:∂ 2632:− 2623:∂ 2612:β 2608:∂ 2593:∂ 2588:α 2585:⁡ 2579:∂ 2567:β 2563:− 2545:Γ 2523:α 2520:⁡ 2508:∂ 2504:− 2486:Γ 2450:Γ 2399:β 2366:β 2339:β 2312:β 2278:∂ 2265:β 2229:∂ 2216:β 2186:β 2159:∂ 2132:∂ 2103:μ 2095:∂ 2088:∂ 2080:μ 2057:∂ 2025:ν 2020:μ 2016:δ 2007:ν 1984:μ 1971:ν 1940:μ 1923:That is, 1897:θ 1894:⁡ 1815:β 1786:β 1780:α 1764:μ 1719:θ 1716:⁡ 1648:β 1628:β 1624:α 1614:β 1608:− 1584:α 1558:μ 1517:− 1491:ϕ 1485:θ 1482:⁡ 1468:μ 1455:ϕ 1450:μ 1423:θ 1409:μ 1396:θ 1391:μ 1357:α 1338:β 1334:− 1312:β 1298:μ 1280:μ 1251:α 1233:μ 1215:μ 1178:μ 1142:ν 1125:μ 1106:η 1097:ν 1094:μ 1057:η 1003:β 978:τ 958:τ 932:β 905:β 881:π 815:ϕ 809:θ 800:Ω 777:Ω 742:Ω 706:α 687:β 683:− 655:β 635:α 614:− 606:ν 593:μ 580:ν 577:μ 480:ϕ 474:θ 451:μ 370:⁡ 254:φ 246:θ 243:⁡ 221:θ 209:Ω 163:spacetime 3344:Category 3253:See also 2890:and the 1043:pullback 1035:vierbein 291:and the 177:and the 3152:is the 1045:of the 990:is the 183:spheres 173:to the 120:physics 80:scholar 3325:  3028:where 2886:, the 763:Here, 421:static 179:orbits 165:whose 82:  75:  68:  61:  53:  3296:arXiv 545:, is 161:is a 87:JSTOR 73:books 3323:ISBN 3243:i.e. 3075:the 2434:The 2408:< 2375:> 423:and 59:news 3249:.) 3156:or 3101:not 3079:), 2847:cot 1891:sin 1713:sin 1479:sin 870:is 367:dim 283:of 234:sin 193:as 118:In 42:by 3346:: 3321:. 3287:^ 2645:ln 2582:ln 2517:ln 1078:: 1025:. 427:. 404:. 157:A 122:, 3336:. 3331:. 3298:: 3223:2 3218:r 3205:2 3200:t 3192:= 3189:1 3181:r 3177:M 3174:2 3140:) 3137:r 3134:( 3131:M 3111:f 3087:p 3041:t 3013:f 3010:r 3004:4 3001:= 2996:r 2986:t 2960:p 2957:r 2951:4 2941:2 2937:r 2933:M 2925:= 2920:t 2910:t 2857:r 2841:= 2802:r 2797:r 2787:= 2779:r 2768:= 2760:r 2729:r 2724:t 2714:= 2706:t 2695:= 2687:t 2656:r 2640:t 2626:r 2616:t 2602:+ 2596:r 2571:t 2560:= 2555:r 2552:t 2549:r 2512:r 2501:= 2496:t 2493:t 2490:r 2460:k 2457:j 2454:i 2411:0 2403:r 2378:0 2370:r 2343:r 2316:r 2287:r 2282:r 2274:= 2269:r 2238:r 2233:t 2225:= 2220:t 2190:t 2163:r 2136:t 2099:x 2074:i 2070:e 2066:= 2061:i 2012:= 2001:i 1997:e 1991:i 1980:e 1976:= 1965:i 1961:e 1955:T 1951:) 1945:i 1935:e 1931:( 1906:] 1888:r 1884:1 1877:0 1872:0 1867:0 1860:0 1853:r 1850:1 1843:0 1838:0 1831:0 1826:0 1819:r 1809:0 1802:0 1797:0 1790:t 1774:[ 1769:= 1758:i 1754:e 1725:] 1710:r 1705:0 1700:0 1695:0 1688:0 1683:r 1678:0 1673:0 1666:0 1661:0 1652:r 1644:1 1632:r 1618:t 1601:0 1596:0 1591:0 1581:1 1573:[ 1568:= 1563:i 1553:e 1529:) 1526:+ 1523:+ 1520:+ 1514:( 1488:d 1476:r 1473:= 1464:x 1460:d 1445:e 1420:d 1417:r 1414:= 1405:x 1401:d 1386:e 1363:) 1353:t 1350:d 1342:t 1331:r 1328:d 1324:( 1316:r 1308:1 1303:= 1294:x 1290:d 1285:r 1275:e 1247:t 1244:d 1238:= 1229:x 1225:d 1220:t 1210:e 1183:i 1173:e 1147:j 1137:e 1130:i 1120:e 1113:j 1110:i 1102:= 1090:g 1064:j 1061:i 1007:r 955:d 951:/ 947:r 944:d 941:= 936:t 909:t 884:r 878:2 858:r 838:r 818:) 812:, 806:( 803:= 780:) 774:( 771:g 748:. 745:) 739:( 736:g 730:2 726:r 722:+ 717:2 712:) 702:t 699:d 691:t 680:r 677:d 673:( 664:2 659:r 651:1 646:+ 639:2 628:2 624:t 620:d 611:= 602:x 598:d 589:x 585:d 573:g 569:= 564:2 560:s 556:d 523:. 483:) 477:, 471:, 468:r 465:, 462:t 459:( 456:= 447:x 388:3 385:= 382:) 379:M 376:( 373:K 347:) 344:M 341:( 338:K 315:M 272:, 258:2 250:d 238:2 230:+ 225:2 217:d 214:= 205:g 109:) 103:( 98:) 94:( 84:· 77:· 70:· 63:· 36:.

Index


verification
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adding citations to reliable sources
"Spherically symmetric spacetime"
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books
scholar
JSTOR
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physics
Einstein's field equations
black holes
Penrose diagrams
Cauchy horizons
mass inflation
spacetime
isometry group
isomorphic
rotation group SO(3)
orbits
spheres
Euclidean space
polar coordinates
Einstein's field equations
general relativity
Schwarzschild solution
Reissner–Nordström solution
Killing vector fields

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