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Static spacetime

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127: 834: 25: 400: 689: 604: 765: 515: 624: 563: 300: 455: 651: 435: 539: 488: 238: 728: 875: 89: 61: 68: 170: 148: 108: 42: 141: 721: 75: 784: 249: 691:). It is from the latter fact that a static spacetime obtains its name, as the geometry of the space-like slice 46: 311: 899: 868: 57: 816:, Cambridge Monographs on Mathematical Physics, vol. 1, London-New York: Cambridge University Press, 199:, which is the geometry of a stationary spacetime that does not change in time but can rotate. Thus, the 656: 268:
satisfying this additional integrability condition. These spacetimes form one of the simplest classes of
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In general, "almost all" spacetimes will not be static. Some explicit examples include:
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if it does not change over time and is also irrotational. It is a special case of a
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Formally, a spacetime is static if it admits a global, non-vanishing,
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Spacetime which does not change over time and is irrotational
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is the square of the norm of the Killing vector field,
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provides an example of a stationary spacetime that is
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(1973), 395:{\displaystyle g=-\beta (x)dt^{2}+g_{S}} 134:This article includes a list of general 814:The large scale structure of space-time 887: 279:which is a Lorentzian warped product 828: 437:is a (positive definite) metric and 120: 47:adding citations to reliable sources 18: 684:{\displaystyle \lambda =-\beta (x)} 13: 714:(the portion of it covered by the 498: 140:it lacks sufficient corresponding 14: 911: 776:Examples of non-static spacetimes 653:are independent of time (in fact 264:.) Thus, a static spacetime is a 832: 801:in them are not even stationary. 785:Spherically symmetric spacetimes 125: 23: 599:{\displaystyle \lambda =g(K,K)} 34:needs additional citations for 760:{\displaystyle R_{\mu \nu }=0} 678: 672: 593: 581: 457:is a positive function on the 389: 383: 354: 348: 336: 333: 321: 318: 211:is an example that is static. 1: 805: 699:Examples of static spacetimes 510:{\displaystyle \partial _{t}} 848:. You can help Knowledge by 7: 695:does not change over time. 260:are necessarily space-like 10: 916: 827: 305:with a metric of the form 277:standard static spacetime 207:static; the non-rotating 619:{\displaystyle \lambda } 558:{\displaystyle \lambda } 490:may be identified with 295:{\displaystyle \times } 250:orthogonal distribution 155:more precise citations. 844:-related article is a 761: 706:Schwarzschild solution 685: 647: 620: 600: 559: 535: 511: 484: 451: 450:{\displaystyle \beta } 431: 396: 296: 234: 209:Schwarzschild solution 762: 686: 648: 646:{\displaystyle g_{S}} 621: 601: 560: 536: 512: 485: 452: 432: 430:{\displaystyle g_{S}} 397: 297: 235: 900:Lorentzian manifolds 735: 657: 630: 610: 569: 549: 525: 494: 474: 441: 414: 312: 286: 270:Lorentzian manifolds 266:stationary spacetime 224: 219:Killing vector field 197:stationary spacetime 43:improve this article 799:gravitational waves 459:Riemannian manifold 757: 722:Reissner–Nordström 681: 643: 616: 596: 555: 531: 521:, the manifold of 507: 480: 447: 427: 410:is the real line, 392: 292: 230: 185:general relativity 58:"Static spacetime" 857: 856: 534:{\displaystyle K} 483:{\displaystyle K} 233:{\displaystyle K} 181: 180: 173: 119: 118: 111: 93: 907: 895:Relativity stubs 878: 871: 864: 836: 829: 824: 797:Spacetimes with 766: 764: 763: 758: 750: 749: 690: 688: 687: 682: 652: 650: 649: 644: 642: 641: 625: 623: 622: 617: 605: 603: 602: 597: 564: 562: 561: 556: 540: 538: 537: 532: 516: 514: 513: 508: 506: 505: 489: 487: 486: 481: 456: 454: 453: 448: 436: 434: 433: 428: 426: 425: 401: 399: 398: 393: 382: 381: 369: 368: 301: 299: 298: 293: 239: 237: 236: 231: 176: 169: 165: 162: 156: 151:this article by 142:inline citations 129: 128: 121: 114: 107: 103: 100: 94: 92: 51: 27: 19: 915: 914: 910: 909: 908: 906: 905: 904: 885: 884: 883: 882: 808: 778: 742: 738: 736: 733: 732: 712:De Sitter space 704:The (exterior) 701: 658: 655: 654: 637: 633: 631: 628: 627: 611: 608: 607: 570: 567: 566: 550: 547: 546: 526: 523: 522: 501: 497: 495: 492: 491: 475: 472: 471: 442: 439: 438: 421: 417: 415: 412: 411: 377: 373: 364: 360: 313: 310: 309: 287: 284: 283: 225: 222: 221: 177: 166: 160: 157: 147:Please help to 146: 130: 126: 115: 104: 98: 95: 52: 50: 40: 28: 17: 12: 11: 5: 913: 903: 902: 897: 881: 880: 873: 866: 858: 855: 854: 837: 826: 825: 807: 804: 803: 802: 795: 788: 777: 774: 773: 772: 767:discovered by 756: 753: 748: 745: 741: 725: 719: 709: 700: 697: 680: 677: 674: 671: 668: 665: 662: 640: 636: 615: 595: 592: 589: 586: 583: 580: 577: 574: 554: 530: 504: 500: 479: 446: 424: 420: 404: 403: 391: 388: 385: 380: 376: 372: 367: 363: 359: 356: 353: 350: 347: 344: 341: 338: 335: 332: 329: 326: 323: 320: 317: 291: 229: 191:is said to be 179: 178: 133: 131: 124: 117: 116: 31: 29: 22: 15: 9: 6: 4: 3: 2: 912: 901: 898: 896: 893: 892: 890: 879: 874: 872: 867: 865: 860: 859: 853: 851: 847: 843: 838: 835: 831: 830: 823: 819: 815: 810: 809: 800: 796: 793: 792:Kerr solution 789: 786: 783: 782: 781: 770: 754: 751: 746: 743: 739: 730: 729:Weyl solution 726: 723: 720: 717: 713: 710: 707: 703: 702: 696: 694: 675: 669: 666: 663: 660: 638: 634: 613: 590: 587: 584: 578: 575: 572: 552: 544: 528: 520: 502: 477: 470: 469:Killing field 465: 463: 460: 444: 422: 418: 409: 386: 378: 374: 370: 365: 361: 357: 351: 345: 342: 339: 330: 327: 324: 315: 308: 307: 306: 304: 289: 282: 278: 273: 271: 267: 263: 262:hypersurfaces 259: 255: 251: 247: 243: 227: 220: 217: 212: 210: 206: 202: 201:Kerr solution 198: 194: 190: 186: 175: 172: 164: 154: 150: 144: 143: 137: 132: 123: 122: 113: 110: 102: 91: 88: 84: 81: 77: 74: 70: 67: 63: 60: â€“  59: 55: 54:Find sources: 48: 44: 38: 37: 32:This article 30: 26: 21: 20: 850:expanding it 839: 813: 779: 769:Hermann Weyl 716:static patch 692: 543:trajectories 542: 518: 466: 461: 407: 405: 302: 280: 276: 274: 245: 242:irrotational 241: 213: 204: 192: 182: 167: 158: 139: 105: 96: 86: 79: 72: 65: 53: 41:Please help 36:verification 33: 153:introducing 889:Categories 842:relativity 806:References 254:involutive 161:April 2021 136:references 99:April 2021 69:newspapers 747:ν 744:μ 670:β 667:− 661:λ 614:λ 573:λ 553:λ 499:∂ 445:β 346:β 343:− 290:× 258:foliation 240:which is 189:spacetime 248:, whose 216:timelike 822:0424186 606:, both 149:improve 83:scholar 820:  724:space. 406:where 193:static 138:, but 85:  78:  71:  64:  56:  840:This 90:JSTOR 76:books 846:stub 790:The 727:The 626:and 517:and 246:i.e. 187:, a 62:news 272:. 252:is 205:not 183:In 45:by 891:: 818:MR 718:). 464:. 244:, 877:e 870:t 863:v 852:. 771:. 755:0 752:= 740:R 708:. 693:S 679:) 676:x 673:( 664:= 639:S 635:g 594:) 591:K 588:, 585:K 582:( 579:g 576:= 541:- 529:K 519:S 503:t 478:K 462:S 423:S 419:g 408:R 402:, 390:] 387:x 384:[ 379:S 375:g 371:+ 366:2 362:t 358:d 355:) 352:x 349:( 340:= 337:] 334:) 331:x 328:, 325:t 322:( 319:[ 316:g 303:S 281:R 228:K 174:) 168:( 163:) 159:( 145:. 112:) 106:( 101:) 97:( 87:· 80:· 73:· 66:· 39:.

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"Static spacetime"
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general relativity
spacetime
stationary spacetime
Kerr solution
Schwarzschild solution
timelike
Killing vector field
orthogonal distribution
involutive
foliation
hypersurfaces
stationary spacetime
Lorentzian manifolds
Riemannian manifold

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