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Constant of motion

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1575: 912: 1570:{\displaystyle {\begin{aligned}{\frac {d}{dt}}\left\langle Q\right\rangle &={\frac {d}{dt}}\left\langle \psi \right|Q\left|\psi \right\rangle \\&=\left({\frac {d}{dt}}\left\langle \psi \right|\right)Q\left|\psi \right\rangle +\left\langle \psi \right|{\frac {dQ}{dt}}\left|\psi \right\rangle +\left\langle \psi \right|Q\left({\frac {d}{dt}}\left|\psi \right\rangle \right)\\&=-{\frac {1}{i\hbar }}\left\langle H\psi \right|Q\left|\psi \right\rangle +\left\langle \psi \right|{\frac {dQ}{dt}}\left|\psi \right\rangle +{\frac {1}{i\hbar }}\left\langle \psi \right|Q\left|H\psi \right\rangle \\&=-{\frac {1}{i\hbar }}\left\langle \psi \right|HQ\left|\psi \right\rangle +\left\langle \psi \right|{\frac {dQ}{dt}}\left|\psi \right\rangle +{\frac {1}{i\hbar }}\left\langle \psi \right|QH\left|\psi \right\rangle \\&=-{\frac {1}{i\hbar }}\left\langle \psi \right|\left\left|\psi \right\rangle +\left\langle \psi \right|{\frac {dQ}{dt}}\left|\psi \right\rangle \end{aligned}}} 723: 2358: 2153: 1749: 563: 2404:, defined as any functions of only the phase-space coordinates that are constant along an orbit. Every integral of motion is a constant of motion, but the converse is not true because a constant of motion may depend on time. Examples of integrals of motion are the angular momentum vector, 2207: 120:
is the intersection of a sphere (conservation of total angular momentum) and an ellipsoid (conservation of energy), a trajectory that might be otherwise hard to derive and visualize. Therefore, the identification of constants of motion is an important objective in
1987: 1587: 2519: 917: 335: 897: 718:{\displaystyle {\frac {d}{dt}}\langle \psi |Q|\psi \rangle =-{\frac {1}{i\hbar }}\left\langle \psi \right|\left\left|\psi \right\rangle +\left\langle \psi \right|{\frac {dQ}{dt}}\left|\psi \right\rangle \,} 2440: 2212: 424: 1971: 1860: 2202: 2353:{\displaystyle {\begin{aligned}{\frac {d}{dt}}\langle Q\rangle &=-{\frac {1}{i\hbar }}\left(E\langle \psi |Q|\psi \rangle -E\langle \psi |Q|\psi \rangle \right)\\&=0\end{aligned}}} 2593:
observables or fixes a gauge. In a canonical language, this usually means either constructing functions which Poisson-commute on the constraint surface with the gauge generating
2575: 2148:{\displaystyle {\frac {d}{dt}}\langle Q\rangle =-{\frac {1}{i\hbar }}\langle \psi |\left|\psi \rangle =-{\frac {1}{i\hbar }}\langle \psi |\left(HQ-QH\right)|\psi \rangle } 1924: 833: 774: 1809: 503: 1882: 1744:{\displaystyle {\frac {d}{dt}}\langle \psi |Q|\psi \rangle ={\frac {-1}{i\hbar }}\langle \psi |\left|\psi \rangle +\langle \psi |{\frac {dQ}{dt}}|\psi \rangle \,} 253: 471: 451: 355: 248: 2396:
coordinates (position and velocity, or position and momentum) and time that is constant throughout a trajectory. A subset of the constants of motion are the
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The simplest but least systematic approach is the intuitive ("psychic") derivation, in which a quantity is hypothesized to be constant (perhaps because of
847: 61: 2445: 368: 2598: 1929: 1818: 2158: 2601:. Such gauge invariant observables are thus the `constants of motion' of the gauge generators and referred to as Dirac observables. 2407: 516:
constants of motion, such that the Poisson bracket of any pair of constants of motion vanishes, is known as a completely
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only if it is integrable; as of 2024, there is no known consistent method for quantizing chaotic dynamical systems.
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provide a commonly used and straightforward method for identifying constants of motion, particularly when the
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Constants of motion are useful because they allow properties of the motion to be derived without solving the
2521:. An example of a function that is a constant of motion but not an integral of motion would be the function 2707: 145: 533: 101: 2524: 521: 188: 69: 43: 2594: 842: 176: 153: 109: 65: 54: 553: 476: 362: 149: 1867: 529: 216: 208: 192: 180: 172: 168: 8: 2360:
This is the reason why eigenstates of the Hamiltonian are also called stationary states.
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throughout the motion, imposing in effect a constraint on the motion. However, it is a
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not explicitly dependent on time), the energy of the system is a constant of motion (a
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provides a systematic way of deriving such quantities from the symmetry. For example,
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A constant of motion may be defined in a given force field as any function of
2701: 838: 525: 330:{\displaystyle 0={\frac {dA}{dt}}={\frac {\partial A}{\partial t}}+\{A,H\},} 906: 2393: 549: 141:) and later shown mathematically to be conserved throughout the motion. 117: 105: 97: 560:, and it does not itself depend explicitly on time. This is because 122: 28: 2597:
or to fix the flow of the latter by singling out points within each
892:{\displaystyle i\hbar {\frac {\partial \psi }{\partial t}}=H\psi .} 212: 164: 113: 250:
is a constant of the motion if its total time derivative is zero
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There are several methods for identifying constants of motion.
128: 520:. Such a collection of constants of motion are said to be in 196: 2435:{\displaystyle \mathbf {L} =\mathbf {x} \times \mathbf {v} } 2372:
has constants of motion other than the energy. By contrast,
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for an object moving at a constant speed in one dimension.
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For an arbitrary state of a Quantum Mechanical system, if
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equals minus its partial derivative with respect to time
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corresponding to the constants of motion. For example,
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Taking the time derivative of the expectation value of
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are constants of motion, so is their Poisson bracket
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corresponds to a constant of motion, often called a
215:. The converse is also true; every symmetry of the 2671: 2676: 2569: 2513: 2434: 2352: 2196: 2147: 1966:{\displaystyle {\frac {d}{dt}}\langle Q\rangle =0} 1965: 1918: 1884:is an eigenfunction of Hamiltonian, then even if 1876: 1855:{\displaystyle {\frac {d}{dt}}\langle Q\rangle =0} 1854: 1803: 1743: 1569: 891: 827: 768: 717: 497: 465: 445: 418: 349: 329: 242: 2197:{\displaystyle H|\psi \rangle =E|\psi \rangle \,} 2699: 2647:. Princeton University Press. 27 January 2008. 2644:Binney, J. and Tremaine, S.: Galactic Dynamics 2616: 2585:In order to extract physical information from 2363: 788:which depends on position, momentum and time, 2325: 2303: 2294: 2272: 2236: 2230: 2190: 2173: 2142: 2098: 2074: 2036: 2012: 2006: 1954: 1948: 1843: 1837: 1737: 1698: 1692: 1654: 1628: 1606: 604: 582: 492: 480: 410: 398: 321: 309: 2679:Introduction to Quantum Mechanics (2nd ed.) 129:Methods for identifying constants of motion 1815:is not explicitly dependent on time, then 2193: 1740: 765: 714: 159:Another approach is to recognize that a 152:adopts recognizable functional forms in 539: 14: 2700: 784:Say there is some observable quantity 433:, which states that if two quantities 2387: 2580: 2376:is the only constant of motion in a 100:of the motion can be derived as the 548:will be a constant of motion if it 207:results from the invariance of the 191:results from the invariance of the 179:results from the invariance of the 24: 2497: 868: 860: 383: 375: 297: 289: 25: 2719: 2617:Landau, L.; Lifshitz, E. (1960). 2258: 2092: 2030: 1648: 1471: 1415: 1324: 1266: 1173: 854: 622: 49:, the natural consequence of the 2504: 2464: 2456: 2428: 2420: 2412: 1581: 205:conservation of angular momentum 96:. In fortunate cases, even the 2621:. Pergamon Press. p. 135. 1980: 189:conservation of linear momentum 87: 2635: 2610: 2549: 2531: 2508: 2500: 2468: 2452: 2318: 2310: 2287: 2279: 2183: 2166: 2135: 2105: 2067: 2043: 1730: 1705: 1685: 1661: 1621: 1613: 822: 804: 744: 732: 597: 589: 195:under shifts in the origin of 183:under shifts in the origin of 13: 1: 2604: 2570:{\displaystyle C(x,v,t)=x-vt} 779: 776:is the commutator relation. 64:). Common examples include 7: 2364:Relevance for quantum chaos 1919:{\displaystyle \left\neq 0} 112:shows that the torque-free 60:(which would require extra 10: 2724: 1926:it is still the case that 1756: 837:And also, that there is a 828:{\displaystyle Q=Q(x,p,t)} 429:Another useful result is 146:Hamilton–Jacobi equations 82:inverse-square force laws 78:Laplace–Runge–Lenz vector 2589:, one either constructs 1977:is independent of time. 769:{\displaystyle =HQ-QH\,} 512:degrees of freedom, and 2595:first class constraints 1804:{\displaystyle \left=0} 544:An observable quantity 524:with each other. For a 498:{\displaystyle \{A,B\}} 2571: 2515: 2436: 2354: 2198: 2149: 1967: 1920: 1878: 1856: 1805: 1745: 1571: 893: 843:Schrödinger's equation 829: 770: 719: 499: 467: 447: 420: 351: 331: 244: 201:translational symmetry 177:conservation of energy 154:orthogonal coordinates 110:Poinsot's construction 2572: 2516: 2437: 2378:non-integrable system 2355: 2199: 2150: 1968: 1921: 1879: 1877:{\displaystyle \psi } 1857: 1806: 1746: 1572: 894: 830: 771: 720: 500: 468: 448: 421: 352: 332: 245: 2525: 2446: 2408: 2208: 2159: 1988: 1930: 1888: 1868: 1819: 1773: 1588: 913: 905:requires use of the 848: 792: 729: 564: 540:In quantum mechanics 477: 457: 437: 369: 341: 254: 234: 2708:Classical mechanics 2673:Griffiths, David J. 2398:integrals of motion 1769:commute, i.e. if 94:equations of motion 51:equations of motion 2567: 2511: 2432: 2388:Integral of motion 2350: 2348: 2194: 2145: 1963: 1916: 1874: 1852: 1801: 1741: 1567: 1565: 889: 825: 766: 715: 534:conserved quantity 495: 463: 443: 416: 347: 337:which occurs when 327: 240: 161:conserved quantity 33:constant of motion 2683:. Prentice Hall. 2581:Dirac observables 2482: 2370:integrable system 2262: 2228: 2096: 2034: 2004: 1946: 1835: 1754: 1753: 1727: 1652: 1604: 1550: 1475: 1419: 1390: 1328: 1270: 1241: 1177: 1133: 1085: 1021: 966: 933: 909:, and results in 875: 701: 626: 580: 518:integrable system 466:{\displaystyle B} 446:{\displaystyle A} 431:Poisson's theorem 390: 350:{\displaystyle A} 304: 281: 243:{\displaystyle A} 173:Noether's theorem 163:corresponds to a 139:experimental data 62:constraint forces 37:physical quantity 16:(Redirected from 2715: 2694: 2682: 2665: 2664: 2662: 2661: 2639: 2633: 2632: 2614: 2576: 2574: 2573: 2568: 2520: 2518: 2517: 2512: 2507: 2493: 2492: 2483: 2475: 2467: 2459: 2441: 2439: 2438: 2433: 2431: 2423: 2415: 2359: 2357: 2356: 2351: 2349: 2336: 2332: 2328: 2321: 2313: 2290: 2282: 2263: 2261: 2250: 2229: 2227: 2216: 2203: 2201: 2200: 2195: 2186: 2169: 2154: 2152: 2151: 2146: 2138: 2133: 2129: 2108: 2097: 2095: 2084: 2070: 2065: 2061: 2046: 2035: 2033: 2022: 2005: 2003: 1992: 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851: 844: 840: 839:wave function 835: 819: 816: 813: 810: 807: 801: 798: 795: 777: 762: 759: 756: 753: 750: 747: 741: 738: 735: 710: 707: 704: 697: 694: 689: 686: 679: 676: 673: 669: 665: 662: 659: 654: 650: 647: 644: 640: 635: 632: 629: 619: 615: 610: 607: 601: 593: 585: 576: 573: 569: 559: 555: 551: 547: 537: 535: 531: 527: 526:closed system 523: 519: 515: 511: 506: 489: 486: 483: 460: 440: 432: 413: 407: 404: 401: 395: 392: 386: 378: 364: 360: 344: 324: 318: 315: 312: 306: 300: 292: 283: 277: 274: 269: 266: 260: 257: 237: 229: 226: 222: 218: 214: 210: 206: 202: 198: 194: 190: 186: 182: 178: 174: 170: 166: 162: 158: 155: 151: 147: 143: 140: 136: 135: 134: 126: 124: 119: 115: 111: 107: 103: 99: 95: 85: 83: 79: 75: 71: 67: 63: 59: 57: 52: 48: 46: 41: 38: 34: 30: 19: 2678: 2658:. Retrieved 2643: 2637: 2618: 2612: 2584: 2401: 2397: 2391: 2367: 1984: 1863: 1760: 1579:So finally, 1578: 907:product rule 900: 841:which obeys 836: 783: 557: 545: 543: 513: 509: 507: 430: 428: 224: 220: 200: 132: 102:intersection 91: 88:Applications 55: 45:mathematical 44: 32: 26: 2599:gauge orbit 2394:phase-space 554:Hamiltonian 363:Hamiltonian 230:A quantity 150:Hamiltonian 106:isosurfaces 2660:2011-05-05 2605:References 1981:Derivation 780:Derivation 530:Lagrangian 522:involution 217:Lagrangian 209:Lagrangian 193:Lagrangian 181:Lagrangian 169:Lagrangian 118:rigid body 98:trajectory 58:constraint 47:constraint 2619:Mechanics 2559:− 2498:Φ 2425:× 2382:quantized 2326:⟩ 2323:ψ 2307:ψ 2304:⟨ 2298:− 2295:⟩ 2292:ψ 2276:ψ 2273:⟨ 2259:ℏ 2247:− 2237:⟩ 2231:⟨ 2191:⟩ 2188:ψ 2174:⟩ 2171:ψ 2143:⟩ 2140:ψ 2121:− 2102:ψ 2099:⟨ 2093:ℏ 2081:− 2075:⟩ 2072:ψ 2040:ψ 2037:⟨ 2031:ℏ 2019:− 2013:⟩ 2007:⟨ 1973:provided 1955:⟩ 1949:⟨ 1911:≠ 1872:ψ 1844:⟩ 1838:⟨ 1738:⟩ 1735:ψ 1702:ψ 1699:⟨ 1693:⟩ 1690:ψ 1658:ψ 1655:⟨ 1649:ℏ 1638:− 1629:⟩ 1626:ψ 1610:ψ 1607:⟨ 1557:ψ 1526:ψ 1512:ψ 1482:ψ 1472:ℏ 1460:− 1443:ψ 1426:ψ 1416:ℏ 1397:ψ 1366:ψ 1352:ψ 1335:ψ 1325:ℏ 1313:− 1295:ψ 1277:ψ 1267:ℏ 1248:ψ 1217:ψ 1203:ψ 1188:ψ 1174:ℏ 1162:− 1140:ψ 1106:ψ 1092:ψ 1061:ψ 1047:ψ 1028:ψ 987:ψ 973:ψ 884:ψ 869:∂ 864:ψ 861:∂ 855:ℏ 757:− 708:ψ 677:ψ 663:ψ 633:ψ 623:ℏ 611:− 605:⟩ 602:ψ 586:ψ 583:⟨ 552:with the 396:− 384:∂ 376:∂ 361:with the 298:∂ 290:∂ 213:rotations 123:mechanics 40:conserved 29:mechanics 2702:Category 2675:(2004). 1560:⟩ 1523:⟨ 1515:⟩ 1479:⟨ 1446:⟩ 1423:⟨ 1400:⟩ 1363:⟨ 1355:⟩ 1332:⟨ 1299:⟩ 1274:⟨ 1251:⟩ 1214:⟨ 1206:⟩ 1181:⟨ 1143:⟩ 1103:⟨ 1095:⟩ 1058:⟨ 1050:⟩ 1025:⟨ 990:⟩ 970:⟨ 943:⟩ 937:⟨ 711:⟩ 674:⟨ 666:⟩ 630:⟨ 550:commutes 165:symmetry 114:rotation 76:and the 56:physical 2155:Since 1864:But if 1757:Comment 225:current 167:of the 2687:  2651:  2625:  2374:energy 725:where 211:under 203:) and 66:energy 2400:, or 2204:then 197:space 116:of a 80:(for 35:is a 2685:ISBN 2649:ISBN 2623:ISBN 1811:and 1765:and 453:and 185:time 144:The 31:, a 536:). 357:'s 223:or 104:of 84:). 27:In 2704:: 556:, 505:. 187:, 171:. 125:. 72:, 68:, 2693:. 2663:. 2631:. 2565:t 2562:v 2556:x 2553:= 2550:) 2547:t 2544:, 2541:v 2538:, 2535:x 2532:( 2529:C 2509:) 2505:x 2501:( 2495:+ 2490:2 2486:v 2480:2 2477:1 2472:= 2469:) 2465:v 2461:, 2457:x 2453:( 2450:H 2429:v 2421:x 2417:= 2413:L 2344:0 2341:= 2330:) 2319:| 2315:Q 2311:| 2301:E 2288:| 2284:Q 2280:| 2270:E 2266:( 2256:i 2252:1 2244:= 2234:Q 2225:t 2222:d 2218:d 2184:| 2180:E 2177:= 2167:| 2163:H 2136:| 2131:) 2127:H 2124:Q 2118:Q 2115:H 2111:( 2106:| 2090:i 2086:1 2078:= 2068:| 2063:] 2059:Q 2056:, 2053:H 2049:[ 2044:| 2028:i 2024:1 2016:= 2010:Q 2001:t 1998:d 1994:d 1975:Q 1961:0 1958:= 1952:Q 1943:t 1940:d 1936:d 1914:0 1907:] 1903:Q 1900:, 1897:H 1893:[ 1850:0 1847:= 1841:Q 1832:t 1829:d 1825:d 1813:Q 1799:0 1796:= 1792:] 1788:Q 1785:, 1782:H 1778:[ 1767:Q 1763:H 1731:| 1724:t 1721:d 1716:Q 1713:d 1706:| 1696:+ 1686:| 1681:] 1677:Q 1674:, 1671:H 1667:[ 1662:| 1646:i 1641:1 1632:= 1622:| 1618:Q 1614:| 1601:t 1598:d 1594:d 1554:| 1547:t 1544:d 1539:Q 1536:d 1529:| 1519:+ 1509:| 1504:] 1500:Q 1497:, 1494:H 1490:[ 1485:| 1469:i 1465:1 1457:= 1440:| 1436:H 1433:Q 1429:| 1413:i 1409:1 1404:+ 1394:| 1387:t 1384:d 1379:Q 1376:d 1369:| 1359:+ 1349:| 1345:Q 1342:H 1338:| 1322:i 1318:1 1310:= 1292:H 1288:| 1284:Q 1280:| 1264:i 1260:1 1255:+ 1245:| 1238:t 1235:d 1230:Q 1227:d 1220:| 1210:+ 1200:| 1196:Q 1192:| 1185:H 1171:i 1167:1 1159:= 1148:) 1137:| 1130:t 1127:d 1123:d 1117:( 1113:Q 1109:| 1099:+ 1089:| 1082:t 1079:d 1074:Q 1071:d 1064:| 1054:+ 1044:| 1040:Q 1036:) 1031:| 1018:t 1015:d 1011:d 1005:( 1001:= 984:| 980:Q 976:| 963:t 960:d 956:d 951:= 940:Q 930:t 927:d 923:d 903:Q 887:. 881:H 878:= 872:t 852:i 823:) 820:t 817:, 814:p 811:, 808:x 805:( 802:Q 799:= 796:Q 786:Q 763:H 760:Q 754:Q 751:H 748:= 745:] 742:Q 739:, 736:H 733:[ 705:| 698:t 695:d 690:Q 687:d 680:| 670:+ 660:| 655:] 651:Q 648:, 645:H 641:[ 636:| 620:i 616:1 608:= 598:| 594:Q 590:| 577:t 574:d 570:d 558:H 546:Q 528:( 514:n 510:n 493:} 490:B 487:, 484:A 481:{ 461:B 441:A 414:. 411:} 408:H 405:, 402:A 399:{ 393:= 387:t 379:A 345:A 325:, 322:} 319:H 316:, 313:A 310:{ 307:+ 301:t 293:A 284:= 278:t 275:d 270:A 267:d 261:= 258:0 238:A 227:. 199:( 156:. 20:)

Index

First integral
mechanics
physical quantity
conserved
mathematical constraint
equations of motion
physical constraint
constraint forces
energy
linear momentum
angular momentum
Laplace–Runge–Lenz vector
inverse-square force laws
equations of motion
trajectory
intersection
isosurfaces
Poinsot's construction
rotation
rigid body
mechanics
experimental data
Hamilton–Jacobi equations
Hamiltonian
orthogonal coordinates
conserved quantity
symmetry
Lagrangian
Noether's theorem
conservation of energy

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