Knowledge (XXG)

Principle of covariance

Source đź“ť

170: 389: 251: 222: 520: 486: 455: 432: 412: 271: 193: 54:
of the physical laws under the group of admissible transformations although in most cases the equations are actually invariant. However, in the theory of
20:
emphasizes the formulation of physical laws using only those physical quantities the measurements of which the observers in different
108: 632: 315: 40: 571: 309:
equation of motion of a charged particle in an electromagnetic field (a generalization of Newton's second law)
79: 583: 547: 286: 523: 99: 285:
the admissible frames of reference are all inertial frames. The transformations between frames are the
32: 67: 36: 593: 588: 535: 458: 282: 21: 227: 198: 43:
between admissible frames of reference of the physical theory. This group is referred to as the
290: 55: 495: 91: 78:. Time is then absolute and the transformations between admissible frames of references are 44: 464: 58:, the equations are not invariant under reflections (but are, of course, still covariant). 539: 298: 87: 71: 437: 417: 397: 256: 178: 83: 75: 626: 306: 559: 555: 551: 294: 543: 489: 614:
Formal Structure of Electromagnetics: General Covariance and Electromagnetics
563: 289:
which (together with the rotations, translations, and reflections) form the
567: 302: 82:
which (together with rotations, translations, and reflections) form the
95: 434:
are the mass and charge of the particle (invariant 4-scalars);
550:) coordinate transformations. The covariant quantities are 542:. The transformations between frames are all arbitrary ( 305:
and others). An example of a covariant equation is the
27:
Mathematically, the physical quantities must transform
165:{\displaystyle m{\frac {d{\vec {v}}}{dt}}={\vec {F}},} 498: 467: 440: 420: 400: 318: 259: 230: 201: 181: 111: 384:{\displaystyle m{\frac {du^{a}}{ds}}=qF^{ab}u_{b},} 514: 480: 449: 426: 406: 383: 265: 245: 216: 187: 164: 74:with relative velocities much smaller than the 538:, the admissible frames of reference are all 293:. The covariant quantities are four-scalars, 50:The principle of covariance does not require 8: 570:. Main example of covariant equation is the 175:where the covariant quantities are the mass 253:acting on the body, and the invariant time 503: 497: 472: 466: 439: 419: 399: 372: 359: 332: 322: 317: 258: 232: 231: 229: 203: 202: 200: 180: 148: 147: 122: 121: 115: 110: 301:(and also more complicated objects like 195:of a moving body (scalar), the velocity 98:. An example of a covariant equation is 86:. The covariant physical quantities are 605: 70:the admissible frames of reference are 524:electromagnetic field strength tensor 7: 14: 62:Covariance in Newtonian mechanics 530:Covariance in general relativity 277:Covariance in special relativity 224:of the body (vector), the force 24:could unambiguously correlate. 237: 208: 153: 127: 1: 31:, that is, under a certain 649: 246:{\displaystyle {\vec {F}}} 217:{\displaystyle {\vec {v}}} 41:coordinate transformations 572:Einstein field equations 80:Galilean transformations 584:Principle of relativity 287:Lorentz transformations 18:principle of covariance 516: 515:{\displaystyle F^{ab}} 482: 451: 428: 408: 385: 267: 247: 218: 189: 166: 517: 483: 481:{\displaystyle u^{a}} 452: 429: 409: 386: 268: 248: 219: 190: 167: 633:Theory of relativity 616:, Dover publications 496: 465: 438: 418: 398: 316: 257: 228: 199: 179: 109: 100:Newton's second law 68:Newtonian mechanics 22:frames of reference 594:General covariance 589:Lorentz covariance 536:general relativity 512: 478: 459:invariant interval 450:{\displaystyle ds} 447: 424: 404: 381: 283:special relativity 263: 243: 214: 185: 162: 562:etc., defined on 427:{\displaystyle q} 407:{\displaystyle m} 347: 266:{\displaystyle t} 240: 211: 188:{\displaystyle m} 156: 142: 130: 56:weak interactions 640: 617: 610: 566:considered as a 540:reference frames 521: 519: 518: 513: 511: 510: 492:(4-vector); and 487: 485: 484: 479: 477: 476: 456: 454: 453: 448: 433: 431: 430: 425: 413: 411: 410: 405: 390: 388: 387: 382: 377: 376: 367: 366: 348: 346: 338: 337: 336: 323: 272: 270: 269: 264: 252: 250: 249: 244: 242: 241: 233: 223: 221: 220: 215: 213: 212: 204: 194: 192: 191: 186: 171: 169: 168: 163: 158: 157: 149: 143: 141: 133: 132: 131: 123: 116: 45:covariance group 16:In physics, the 648: 647: 643: 642: 641: 639: 638: 637: 623: 622: 621: 620: 611: 607: 602: 580: 532: 499: 494: 493: 468: 463: 462: 436: 435: 416: 415: 396: 395: 368: 355: 339: 328: 324: 314: 313: 299:Minkowski space 279: 255: 254: 226: 225: 197: 196: 177: 176: 134: 117: 107: 106: 72:inertial frames 64: 12: 11: 5: 646: 644: 636: 635: 625: 624: 619: 618: 604: 603: 601: 598: 597: 596: 591: 586: 579: 576: 548:differentiable 531: 528: 509: 506: 502: 475: 471: 446: 443: 423: 403: 392: 391: 380: 375: 371: 365: 362: 358: 354: 351: 345: 342: 335: 331: 327: 321: 291:PoincarĂ© group 278: 275: 262: 239: 236: 210: 207: 184: 173: 172: 161: 155: 152: 146: 140: 137: 129: 126: 120: 114: 84:Galilean group 76:speed of light 63: 60: 33:representation 13: 10: 9: 6: 4: 3: 2: 645: 634: 631: 630: 628: 615: 609: 606: 599: 595: 592: 590: 587: 585: 582: 581: 577: 575: 573: 569: 565: 561: 560:tensor fields 557: 556:vector fields 553: 552:scalar fields 549: 545: 541: 537: 529: 527: 525: 507: 504: 500: 491: 473: 469: 460: 444: 441: 421: 401: 378: 373: 369: 363: 360: 356: 352: 349: 343: 340: 333: 329: 325: 319: 312: 311: 310: 308: 307:Lorentz force 304: 300: 297:etc., of the 296: 292: 288: 284: 276: 274: 260: 234: 205: 182: 159: 150: 144: 138: 135: 124: 118: 112: 105: 104: 103: 101: 97: 93: 89: 85: 81: 77: 73: 69: 61: 59: 57: 53: 48: 46: 42: 38: 34: 30: 25: 23: 19: 613: 608: 533: 526:(4-tensor). 461:(4-scalar); 393: 295:four-vectors 280: 174: 65: 51: 49: 28: 26: 17: 15: 29:covariantly 612:E.J.Post, 600:References 544:invertible 490:4-velocity 52:invariance 564:spacetime 303:bispinors 238:→ 209:→ 154:→ 128:→ 90:scalars, 88:Euclidean 627:Category 578:See also 568:manifold 522:is the 488:is the 457:is the 96:tensors 92:vectors 35:of the 394:where 94:, and 37:group 546:and 414:and 534:In 281:In 66:In 39:of 629:: 574:. 558:, 554:, 273:. 102:, 47:. 508:b 505:a 501:F 474:a 470:u 445:s 442:d 422:q 402:m 379:, 374:b 370:u 364:b 361:a 357:F 353:q 350:= 344:s 341:d 334:a 330:u 326:d 320:m 261:t 235:F 206:v 183:m 160:, 151:F 145:= 139:t 136:d 125:v 119:d 113:m

Index

frames of reference
representation
group
coordinate transformations
covariance group
weak interactions
Newtonian mechanics
inertial frames
speed of light
Galilean transformations
Galilean group
Euclidean
vectors
tensors
Newton's second law
special relativity
Lorentz transformations
Poincaré group
four-vectors
Minkowski space
bispinors
Lorentz force
invariant interval
4-velocity
electromagnetic field strength tensor
general relativity
reference frames
invertible
differentiable
scalar fields

Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.

↑