Knowledge (XXG)

Ultrarelativistic limit

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1074: 1031: 487: 296: 248: 529: 409: 83: 109: 328: 167: 57: 766: 367: 129: 369:. Particles with a very small mass do not need much energy to travel at a speed close to c. The latter is used to derive orbits of massless particles such as the 433: 187: 1115: 374: 777: 441: 1057: 337:
This can result from holding the mass fixed and increasing the kinetic energy to very large values or by holding the energy
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is proper time, and travel starts at rest and without changing direction of acceleration (see
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The energy of an ultrarelativistic particle is almost completely due to its kinetic energy
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Fixed target collision with ultrarelativistic motion of the center of mass:
412: 331: 20: 370: 1026:{\displaystyle E_{k}=(\gamma -1)mc^{2}={\frac {1}{2}}mv^{2}+\left} 748:. Its kinetic energy can be approximated by first term of the 632:
are energies of the particle and the target respectively (so
482:{\displaystyle 1-\beta \approx {\frac {1}{2\gamma ^{2}}}} 1089: 780: 754: 496: 444: 421: 391: 355: 304: 256: 198: 175: 141: 117: 91: 65: 39: 385:
Below are few ultrarelativistic approximations when
349:to very small values which also imply a very large 27:when its speed is very close to the speed of light 1025: 760: 666:For calculations of the energy of a particle, the 523: 481: 427: 403: 361: 322: 290: 242: 181: 161: 123: 103: 77: 51: 250:. The total energy can also be approximated as 1109: 8: 722:), the approximation is essentially exact. 670:of the ultrarelativistic limit for a speed 1116: 1102: 535:Motion with constant proper acceleration: 995: 982: 976: 967: 945: 921: 915: 885: 875: 869: 856: 842: 825: 816: 785: 779: 753: 495: 470: 457: 443: 420: 390: 354: 303: 291:{\displaystyle E=\gamma mc^{2}\approx pc} 273: 255: 234: 203: 197: 174: 151: 140: 116: 90: 64: 38: 744:, where its speed is much smaller than 243:{\displaystyle E_{k}=(\gamma -1)mc^{2}} 657:is energy in the center of mass frame. 524:{\displaystyle w\approx \ln(2\gamma )} 373:from those of massive particles (cf. 7: 1070: 1068: 375:Kepler problem in general relativity 718:practically indistinguishable from 1088:. You can help Knowledge (XXG) by 14: 1072: 381:Ultrarelativistic approximations 16:Very close to the speed of light 404:{\displaystyle \beta \approx 1} 78:{\displaystyle \beta \approx 1} 964: 954: 933: 924: 806: 794: 518: 509: 224: 212: 33:. Notations commonly used are 1: 662:Accuracy of the approximation 568:is proper acceleration (with 343:fixed and shrinking the mass 104:{\displaystyle \gamma \gg 1} 323:{\displaystyle p=\gamma mv} 1161: 1067: 1058:Aichelburg–Sexl ultraboost 698:%. For particles such as 554:is the distance traveled, 162:{\displaystyle \beta =v/c} 52:{\displaystyle v\approx c} 330:is the Lorentz invariant 761:{\displaystyle \gamma } 362:{\displaystyle \gamma } 189:is the speed of light. 124:{\displaystyle \gamma } 23:, a particle is called 1084:-related article is a 1027: 762: 525: 483: 429: 405: 363: 324: 292: 244: 183: 163: 125: 105: 79: 53: 1043:Relativistic particle 1028: 763: 526: 484: 430: 406: 364: 325: 293: 245: 184: 164: 126: 106: 80: 54: 778: 752: 710:) are usually above 494: 442: 419: 389: 353: 302: 254: 196: 173: 139: 115: 89: 63: 37: 1048:Classical mechanics 730:The opposite case ( 581:proper acceleration 1135:Special relativity 1053:Special relativity 1023: 758: 742:classical particle 583:for more details). 521: 479: 425: 401: 359: 320: 288: 240: 179: 159: 121: 101: 75: 49: 1097: 1096: 1004: 974: 891: 864: 833: 740:) is a so-called 477: 428:{\displaystyle w} 182:{\displaystyle c} 25:ultrarelativistic 1152: 1145:Relativity stubs 1118: 1111: 1104: 1076: 1069: 1032: 1030: 1029: 1024: 1022: 1018: 1005: 1003: 1002: 990: 989: 977: 975: 973: 972: 971: 953: 952: 939: 922: 920: 919: 892: 890: 889: 880: 879: 870: 865: 857: 847: 846: 834: 826: 821: 820: 790: 789: 767: 765: 764: 759: 747: 739: 721: 717: 713: 705: 697: 693: 683: 679: 656: 647: 631: 622: 613: 612: 611: 578: 574: 567: 553: 549: 530: 528: 527: 522: 488: 486: 485: 480: 478: 476: 475: 474: 458: 434: 432: 431: 426: 410: 408: 407: 402: 368: 366: 365: 360: 348: 342: 329: 327: 326: 321: 297: 295: 294: 289: 278: 277: 249: 247: 246: 241: 239: 238: 208: 207: 188: 186: 185: 180: 168: 166: 165: 160: 155: 130: 128: 127: 122: 110: 108: 107: 102: 84: 82: 81: 76: 58: 56: 55: 50: 32: 1160: 1159: 1155: 1154: 1153: 1151: 1150: 1149: 1125: 1124: 1123: 1122: 1066: 1039: 991: 978: 963: 941: 940: 923: 911: 881: 871: 855: 851: 838: 812: 781: 776: 775: 769:binomial series 750: 749: 745: 731: 728: 719: 715: 711: 703: 695: 685: 681: 671: 664: 655: 649: 646: 639: 633: 630: 624: 621: 615: 610: 604: 597: 595: 593: 587: 576: 569: 555: 551: 536: 492: 491: 466: 462: 440: 439: 417: 416: 387: 386: 383: 351: 350: 344: 338: 300: 299: 269: 252: 251: 230: 199: 194: 193: 171: 170: 137: 136: 113: 112: 87: 86: 61: 60: 35: 34: 28: 17: 12: 11: 5: 1158: 1156: 1148: 1147: 1142: 1140:Approximations 1137: 1127: 1126: 1121: 1120: 1113: 1106: 1098: 1095: 1094: 1077: 1065: 1062: 1061: 1060: 1055: 1050: 1045: 1038: 1035: 1034: 1033: 1021: 1017: 1014: 1011: 1008: 1001: 998: 994: 988: 985: 981: 970: 966: 962: 959: 956: 951: 948: 944: 938: 935: 932: 929: 926: 918: 914: 910: 907: 904: 901: 898: 895: 888: 884: 878: 874: 868: 863: 860: 854: 850: 845: 841: 837: 832: 829: 824: 819: 815: 811: 808: 805: 802: 799: 796: 793: 788: 784: 757: 727: 724: 708:Lorentz factor 668:relative error 663: 660: 659: 658: 653: 644: 637: 628: 619: 608: 602: 591: 584: 532: 531: 520: 517: 514: 511: 508: 505: 502: 499: 489: 473: 469: 465: 461: 456: 453: 450: 447: 424: 400: 397: 394: 382: 379: 358: 319: 316: 313: 310: 307: 287: 284: 281: 276: 272: 268: 265: 262: 259: 237: 233: 229: 226: 223: 220: 217: 214: 211: 206: 202: 178: 158: 154: 150: 147: 144: 133:Lorentz factor 120: 100: 97: 94: 74: 71: 68: 48: 45: 42: 15: 13: 10: 9: 6: 4: 3: 2: 1157: 1146: 1143: 1141: 1138: 1136: 1133: 1132: 1130: 1119: 1114: 1112: 1107: 1105: 1100: 1099: 1093: 1091: 1087: 1083: 1078: 1075: 1071: 1063: 1059: 1056: 1054: 1051: 1049: 1046: 1044: 1041: 1040: 1036: 1019: 1015: 1012: 1009: 1006: 999: 996: 992: 986: 983: 979: 968: 960: 957: 949: 946: 942: 936: 930: 927: 916: 912: 908: 905: 902: 899: 896: 893: 886: 882: 876: 872: 866: 861: 858: 852: 848: 843: 839: 835: 830: 827: 822: 817: 813: 809: 803: 800: 797: 791: 786: 782: 774: 773: 772: 770: 755: 743: 738: 734: 725: 723: 709: 701: 692: 688: 678: 674: 669: 661: 652: 643: 636: 627: 618: 607: 601: 590: 585: 582: 572: 566: 562: 558: 547: 543: 539: 534: 533: 515: 512: 506: 503: 500: 497: 490: 471: 467: 463: 459: 454: 451: 448: 445: 438: 437: 436: 422: 414: 398: 395: 392: 380: 378: 376: 372: 356: 347: 341: 335: 333: 317: 314: 311: 308: 305: 285: 282: 279: 274: 270: 266: 263: 260: 257: 235: 231: 227: 221: 218: 215: 209: 204: 200: 190: 176: 156: 152: 148: 145: 142: 134: 118: 98: 95: 92: 72: 69: 66: 46: 43: 40: 31: 26: 22: 1090:expanding it 1079: 741: 736: 732: 729: 726:Other limits 690: 686: 676: 672: 665: 650: 641: 634: 625: 616: 605: 599: 588: 570: 564: 560: 556: 545: 541: 537: 384: 345: 339: 336: 191: 29: 24: 18: 694:it is just 684:%, and for 415:is denoted 1129:Categories 1082:relativity 1064:References 801:− 798:γ 756:γ 700:neutrinos 680:is about 516:γ 507:⁡ 501:≈ 468:γ 455:≈ 452:β 449:− 396:≈ 393:β 357:γ 312:γ 280:≈ 264:γ 219:− 216:γ 143:β 119:γ 96:≫ 93:γ 70:≈ 67:β 44:≈ 1037:See also 702:, whose 550:, where 413:rapidity 332:momentum 648:), and 596:√ 131:is the 21:physics 689:= 0.99 675:= 0.95 614:where 411:. The 371:photon 298:where 111:where 1080:This 1086:stub 623:and 377:). 169:and 575:), 573:≫ 1 544:/(2 85:or 59:or 19:In 1131:: 771:: 735:≪ 712:10 682:10 654:CM 640:≫ 594:≈ 592:CM 571:aτ 565:dτ 561:dφ 559:= 540:≈ 504:ln 435:: 334:. 135:, 1117:e 1110:t 1103:v 1092:. 1020:] 1016:. 1013:. 1010:. 1007:+ 1000:n 997:2 993:c 987:n 984:2 980:v 969:2 965:) 961:! 958:n 955:( 950:n 947:2 943:2 937:! 934:) 931:n 928:2 925:( 917:2 913:c 909:m 906:+ 903:. 900:. 897:. 894:+ 887:2 883:c 877:4 873:v 867:m 862:8 859:3 853:[ 849:+ 844:2 840:v 836:m 831:2 828:1 823:= 818:2 814:c 810:m 807:) 804:1 795:( 792:= 787:k 783:E 746:c 737:c 733:v 720:c 716:v 714:( 706:( 704:γ 696:2 691:c 687:v 677:c 673:v 651:E 645:2 642:E 638:1 635:E 629:2 626:E 620:1 617:E 609:2 606:E 603:1 600:E 598:2 589:E 577:τ 563:/ 557:a 552:d 548:) 546:a 542:e 538:d 519:) 513:2 510:( 498:w 472:2 464:2 460:1 446:1 423:w 399:1 346:m 340:E 318:v 315:m 309:= 306:p 286:c 283:p 275:2 271:c 267:m 261:= 258:E 236:2 232:c 228:m 225:) 222:1 213:( 210:= 205:k 201:E 177:c 157:c 153:/ 149:v 146:= 99:1 73:1 47:c 41:v 30:c

Index

physics
Lorentz factor
momentum
photon
Kepler problem in general relativity
rapidity
proper acceleration
relative error
neutrinos
Lorentz factor
binomial series
Relativistic particle
Classical mechanics
Special relativity
Aichelburg–Sexl ultraboost
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relativity
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expanding it
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Approximations
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