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Rarita–Schwinger equation

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1496: 1212: 1491:{\displaystyle \delta {\mathcal {L}}_{RS}=\delta {\bar {\psi }}_{\mu }\gamma ^{\mu \nu \rho }\partial _{\nu }\psi _{\rho }+{\bar {\psi }}_{\mu }\gamma ^{\mu \nu \rho }\partial _{\nu }\delta \psi _{\rho }=\delta {\bar {\psi }}_{\mu }\gamma ^{\mu \nu \rho }\partial _{\nu }\psi _{\rho }-\partial _{\nu }{\bar {\psi }}_{\mu }\gamma ^{\mu \nu \rho }\delta \psi _{\rho }+{\text{ boundary terms}}} 771: 2017: 183: 1878: 1606: 623: 1051: 2201: 901: 374: 1174: 1889: 1714: 74: 1768: 2211:
leads to equation with solutions representing wavefronts, some of which propagate faster than light. In other words, the field then suffers from acausal, superluminal propagation; consequently, the
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in interaction with electromagnetism is essentially flawed. In extended supergravity, though, Das and Freedman have shown that local supersymmetry solves this problem.
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Velo, Giorgio; Zwanzinger, Daniel (1969-12-25). "Noncausality and Other Defects of Interaction Lagrangians for Particles with Spin One and Higher".
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Velo, Giorgio; Zwanziger, Daniel (1969-10-25). "Propagation and Quantization of Rarita-Schwinger Waves in an External Electromagnetic Potential".
2012:{\displaystyle \psi _{0}=\kappa ,\quad \psi _{i}=\psi _{i}^{TT}+{\frac {\gamma ^{j}\partial _{j}}{\nabla ^{2}}}\gamma _{0}\partial _{i}\kappa ,} 306: 1089: 1660: 178:{\displaystyle \left(\epsilon ^{\mu \kappa \rho \nu }\gamma _{5}\gamma _{\kappa }\partial _{\rho }-im\sigma ^{\mu \nu }\right)\psi _{\nu }=0} 567: 1873:{\displaystyle \gamma ^{\nu }{\partial }_{\nu }\psi _{\mu }=0,\quad \partial ^{\mu }\psi _{\mu }=0,\quad \gamma ^{\mu }\psi _{\mu }=0.} 1601:{\displaystyle \delta {\mathcal {L}}_{RS}=2\delta {\bar {\psi }}_{\mu }\gamma ^{\mu \nu \rho }\partial _{\nu }\psi _{\rho },} 399: 2604: 2584: 906: 610: 2124:
As in the case of the Dirac equation, electromagnetic interaction can be added by promoting the partial derivative to
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The massless Rarita–Schwinger equation has a fermionic gauge symmetry: is invariant under the gauge transformation
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using the Majorana flip properties we see that the second and first terms on the RHS are equal, concluding that
1046:{\displaystyle {\mathcal {L}}_{RS}={\bar {\psi }}_{\mu }\gamma ^{\mu \nu \rho }\partial _{\nu }\psi _{\rho },} 499:
with additional components compared to the four component spinor in the Dirac equation. It corresponds to the
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Kobayashi, M.; Shamaly, A. (1978-04-15). "Minimal electromagnetic coupling for massive spin-two fields".
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Rarita, William; Schwinger, Julian (1941-07-01). "On a Theory of Particles with Half-Integral Spin".
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we thus see that the equation of motion for a massless Majorana Rarita–Schwinger spinor reads:
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The gauge symmetry of the massless Rarita-Schwinger equation allows the choice of the gauge
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The current description of massive, higher spin fields through either Rarita–Schwinger or
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Freedman, D. Z.; Das, A. (1977). "Gauge internal symmetry in extended supergravity".
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To obtain the equations of motion we vary the Lagrangian with respect to the fields
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In 1969, Velo and Zwanziger showed that the Rarita–Schwinger Lagrangian coupled to
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Consider a massless Rarita–Schwinger field described by the Lagrangian density
896:{\displaystyle \psi _{\mu }\rightarrow \psi _{\mu }+\partial _{\mu }\epsilon } 2562: 2554: 2525: 2517: 2488: 2480: 2436: 2327: 947:"Weyl" and "Majorana" versions of the Rarita–Schwinger equation also exist. 837: 2341:
Das, A.; Freedman, D. Z. (1976). "Gauge quantization for spin-3/2 fields".
2428: 2269:"Massless Rarita-Schwinger equations: Half and three halves spin solution" 369:{\displaystyle \gamma _{5}=i\gamma _{0}\gamma _{1}\gamma _{2}\gamma _{3}} 1169:{\displaystyle \gamma ^{\mu \nu \rho }\equiv {\frac {1}{3!}}\gamma ^{}.} 1709:{\displaystyle \gamma ^{\mu \nu \rho }\partial _{\nu }\psi _{\rho }=0.} 50: 2248:
S. Weinberg, "The quantum theory of fields", Vol. 3, Cambridge p. 335
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S. Weinberg, "The quantum theory of fields", Vol. 1, Cambridge p. 232
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S. Weinberg, "The quantum theory of fields", Vol. 3, Cambridge p. 335
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satisfies the massless Dirac equation, therefore carrying spin 1/2.
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for spin-1/2 fermions. This equation was first introduced by
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in a four-dimensional flat spacetime. It is similar to the
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is an arbitrary spinor field. This is simply the local
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Pierre Ramond - Field theory, a Modern Primer - p.40
929:{\displaystyle \epsilon \equiv \epsilon _{\alpha }} 2195: 2096: 2076: 2041: 2011: 1872: 1754: 1708: 1646: 1600: 1490: 1198: 1168: 1075: 1045: 928: 895: 795: 765: 487: 460: 388: 368: 295: 247: 216: 177: 2541:(8). American Physical Society (APS): 2179–2181. 2504:(5). American Physical Society (APS): 2218–2222. 2467:(5). American Physical Society (APS): 1337–1341. 217:{\displaystyle \epsilon ^{\mu \kappa \rho \nu }} 2116:formalisms is afflicted with several maladies. 1883:A solution with spins 1/2 and 3/2 is given by: 810:This equation controls the propagation of the 2310:Deser, S.; Kay, J. H.; Stelle, K. S. (1977). 2084:is doubly transverse, carrying spin 3/2, and 1056:where the sum over spin indices is implicit, 844:with spin 3/2 has been found experimentally. 8: 1755:{\displaystyle \gamma ^{\mu }\psi _{\mu }=0} 1647:{\displaystyle \delta {\mathcal {L}}_{RS}=0} 2415:(1). American Physical Society (APS): 61. 1611:plus unimportant boundary terms. Imposing 652: 609:This field equation can be derived as the 2312:"Hamiltonian Formulation of Supergravity" 2294: 2284: 2187: 2168: 2155: 2142: 2136: 2089: 2065: 2060: 2054: 2033: 2027: 1997: 1987: 1975: 1964: 1954: 1947: 1935: 1930: 1917: 1897: 1891: 1858: 1848: 1828: 1818: 1798: 1788: 1783: 1776: 1770: 1740: 1730: 1724: 1694: 1684: 1668: 1662: 1629: 1623: 1622: 1616: 1589: 1579: 1563: 1553: 1542: 1541: 1522: 1516: 1515: 1509: 1483: 1474: 1455: 1445: 1434: 1433: 1426: 1413: 1403: 1387: 1377: 1366: 1365: 1352: 1339: 1323: 1313: 1302: 1301: 1291: 1281: 1265: 1255: 1244: 1243: 1227: 1221: 1220: 1214: 1190: 1184: 1154: 1144: 1131: 1112: 1097: 1091: 1067: 1061: 1034: 1024: 1008: 998: 987: 986: 973: 967: 966: 963: 920: 908: 884: 871: 858: 852: 787: 781: 757: 739: 720: 710: 700: 681: 666: 655: 654: 640: 628: 627: 625: 479: 473: 449: 436: 419: 407: 401: 381: 360: 350: 340: 330: 314: 308: 264: 239: 233: 199: 193: 163: 145: 126: 116: 106: 87: 76: 68:In modern notation it can be written as: 951:Equations of motion in the massless case 2223: 613:corresponding to the Rarita–Schwinger 944:, and the field must be a gravitino. 7: 2267:Valenzuela, M.; Zanelli, J. (2024). 27:Field equation for spin-3/2 fermions 568:representation of the Lorentz group 2165: 2139: 2030: 1994: 1972: 1961: 1815: 1784: 1681: 1576: 1423: 1400: 1336: 1278: 1021: 881: 717: 123: 25: 814:of composite objects such as the 248:{\displaystyle \gamma _{\kappa }} 1912: 1843: 1813: 296:{\displaystyle \kappa =0,1,2,3} 2595:Partial differential equations 2580:Eponymous equations of physics 2449:Particle physics and cosmology 2148: 2077:{\displaystyle \psi _{i}^{TT}} 1547: 1439: 1371: 1307: 1249: 1158: 1132: 992: 864: 660: 455: 429: 1: 2296:10.21468/SciPostPhys.16.3.065 1762:, reducing the equations to: 611:Euler–Lagrange equation 2391:10.1016/0550-3213(77)90041-4 2363:10.1016/0550-3213(76)90589-7 1199:{\displaystyle \psi _{\mu }} 1076:{\displaystyle \psi _{\mu }} 796:{\displaystyle \psi _{\mu }} 488:{\displaystyle \psi _{\nu }} 2042:{\displaystyle \nabla ^{2}} 2621: 2126:gauge covariant derivative 2049:is the spatial Laplacian, 1083:are Majorana spinors, and 836:) or for the conjectural 2108:Drawbacks of the equation 36:Rarita–Schwinger equation 18:Rarita-Schwinger equation 2555:10.1103/physrevd.17.2179 2518:10.1103/physrev.188.2218 2481:10.1103/physrev.186.1337 2328:10.1103/PhysRevD.16.2448 2120:Superluminal propagation 2097:{\displaystyle \kappa } 2197: 2098: 2078: 2043: 2013: 1874: 1756: 1710: 1648: 1602: 1492: 1200: 1170: 1077: 1047: 930: 897: 797: 767: 489: 462: 390: 370: 297: 249: 218: 179: 2429:10.1103/physrev.60.61 2198: 2099: 2079: 2044: 2014: 1875: 1757: 1711: 1649: 1603: 1493: 1201: 1171: 1078: 1048: 931: 898: 798: 768: 490: 463: 391: 371: 298: 250: 219: 180: 2605:Mathematical physics 2585:Quantum field theory 2135: 2088: 2053: 2026: 1890: 1769: 1723: 1661: 1615: 1508: 1485: boundary terms 1213: 1183: 1090: 1060: 962: 907: 851: 780: 776:where the bar above 624: 472: 400: 380: 307: 263: 232: 192: 75: 2547:1978PhRvD..17.2179K 2510:1969PhRv..188.2218V 2473:1969PhRv..186.1337V 2421:1941PhRv...60...61R 2383:1977NuPhB.120..221F 2355:1976NuPhB.114..271D 2073: 1943: 842:elementary particle 495:is a vector-valued 32:theoretical physics 2193: 2094: 2074: 2056: 2039: 2009: 1926: 1870: 1752: 1706: 1644: 1598: 1488: 1196: 1166: 1073: 1043: 926: 893: 793: 763: 650: 485: 458: 386: 366: 293: 245: 226:Levi-Civita symbol 214: 175: 2535:Physical Review D 2371:Nuclear Physics B 2343:Nuclear Physics B 1981: 1550: 1486: 1442: 1374: 1310: 1252: 1125: 995: 663: 649: 570:, or rather, its 427: 389:{\displaystyle m} 16:(Redirected from 2612: 2566: 2529: 2492: 2447:, Squires E.J., 2443:Collins P.D.B., 2440: 2395: 2394: 2366: 2338: 2332: 2331: 2322:(8): 2448–2455. 2307: 2301: 2300: 2298: 2288: 2264: 2258: 2255: 2249: 2246: 2240: 2237: 2231: 2228: 2209:electromagnetism 2202: 2200: 2199: 2194: 2192: 2191: 2173: 2172: 2160: 2159: 2147: 2146: 2103: 2101: 2100: 2095: 2083: 2081: 2080: 2075: 2072: 2064: 2048: 2046: 2045: 2040: 2038: 2037: 2018: 2016: 2015: 2010: 2002: 2001: 1992: 1991: 1982: 1980: 1979: 1970: 1969: 1968: 1959: 1958: 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413: 410: 406: 385: 363: 359: 353: 349: 343: 339: 333: 329: 325: 322: 317: 313: 292: 289: 286: 283: 280: 277: 274: 271: 268: 257:Dirac matrices 242: 238: 211: 208: 205: 202: 198: 186: 185: 174: 171: 166: 162: 157: 151: 148: 144: 140: 137: 134: 129: 125: 119: 115: 109: 105: 99: 96: 93: 90: 86: 81: 59:William Rarita 55:Dirac equation 43:field equation 26: 24: 14: 13: 10: 9: 6: 4: 3: 2: 2617: 2606: 2603: 2601: 2598: 2596: 2593: 2591: 2588: 2586: 2583: 2581: 2578: 2577: 2575: 2564: 2560: 2556: 2552: 2548: 2544: 2540: 2536: 2531: 2527: 2523: 2519: 2515: 2511: 2507: 2503: 2499: 2494: 2490: 2486: 2482: 2478: 2474: 2470: 2466: 2462: 2457: 2454: 2450: 2446: 2442: 2438: 2434: 2430: 2426: 2422: 2418: 2414: 2410: 2405: 2404: 2400: 2392: 2388: 2384: 2380: 2376: 2372: 2364: 2360: 2356: 2352: 2348: 2344: 2337: 2334: 2329: 2325: 2321: 2317: 2313: 2306: 2303: 2297: 2292: 2287: 2282: 2278: 2274: 2270: 2263: 2260: 2254: 2251: 2245: 2242: 2236: 2233: 2227: 2224: 2218: 2216: 2214: 2210: 2188: 2184: 2180: 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1191: 1187: 1163: 1155: 1151: 1145: 1141: 1135: 1128: 1121: 1118: 1114: 1109: 1104: 1101: 1098: 1094: 1086: 1085: 1084: 1068: 1064: 1040: 1035: 1031: 1025: 1015: 1012: 1009: 1005: 999: 989: 982: 977: 974: 958: 957: 956: 950: 948: 945: 943: 939: 938:supersymmetry 921: 917: 913: 910: 890: 885: 877: 872: 868: 859: 855: 845: 843: 840:. So far, no 839: 817: 816:delta baryons 813: 812:wave function 808: 806: 805:Dirac adjoint 788: 784: 758: 754: 749: 743: 740: 736: 732: 729: 726: 721: 711: 707: 701: 697: 691: 688: 685: 682: 678: 673: 667: 657: 646: 643: 637: 634: 620: 619: 618: 616: 612: 607: 569: 498: 480: 476: 450: 446: 442: 437: 433: 424: 421: 416: 411: 408: 404: 396:is the mass, 383: 361: 357: 351: 347: 341: 337: 331: 327: 323: 320: 315: 311: 290: 287: 284: 281: 278: 275: 272: 269: 266: 258: 240: 236: 227: 209: 206: 203: 200: 196: 172: 169: 164: 160: 155: 149: 146: 142: 138: 135: 132: 127: 117: 113: 107: 103: 97: 94: 91: 88: 84: 79: 71: 70: 69: 66: 64: 60: 56: 52: 48: 44: 41: 37: 33: 19: 2538: 2534: 2501: 2497: 2464: 2460: 2452: 2448: 2412: 2408: 2374: 2370: 2346: 2342: 2336: 2319: 2316:Phys. Rev. D 2315: 2305: 2276: 2273:SciPost Phys 2272: 2262: 2253: 2244: 2235: 2226: 2213:quantization 2206: 2123: 2111: 2021: 1882: 1718: 1610: 1500: 1178: 1055: 954: 946: 942:supergravity 846: 809: 803:denotes the 775: 608: 187: 67: 40:relativistic 35: 29: 2453:Section 1.6 2445:Martin A.D. 2114:Fierz–Pauli 549:, 0) ⊕ (0, 2574:Categories 2377:(2): 221. 2349:(2): 271. 2286:2305.00106 2279:(3): 065. 2219:References 615:Lagrangian 2563:0556-2821 2526:0031-899X 2489:0031-899X 2437:0031-899X 2189:μ 2175:− 2170:μ 2166:∂ 2157:μ 2149:→ 2144:μ 2140:∂ 2092:κ 2058:ψ 2031:∇ 2004:κ 1995:∂ 1985:γ 1973:∇ 1962:∂ 1952:γ 1928:ψ 1915:ψ 1907:κ 1895:ψ 1860:μ 1856:ψ 1850:μ 1846:γ 1830:μ 1826:ψ 1820:μ 1816:∂ 1800:μ 1796:ψ 1790:ν 1785:∂ 1778:ν 1774:γ 1742:μ 1738:ψ 1732:μ 1728:γ 1696:ρ 1692:ψ 1686:ν 1682:∂ 1676:ρ 1673:ν 1670:μ 1666:γ 1619:δ 1591:ρ 1587:ψ 1581:ν 1577:∂ 1571:ρ 1568:ν 1565:μ 1561:γ 1555:μ 1548:¯ 1545:ψ 1538:δ 1512:δ 1476:ρ 1472:ψ 1468:δ 1463:ρ 1460:ν 1457:μ 1453:γ 1447:μ 1440:¯ 1437:ψ 1428:ν 1424:∂ 1420:− 1415:ρ 1411:ψ 1405:ν 1401:∂ 1395:ρ 1392:ν 1389:μ 1385:γ 1379:μ 1372:¯ 1369:ψ 1362:δ 1354:ρ 1350:ψ 1346:δ 1341:ν 1337:∂ 1331:ρ 1328:ν 1325:μ 1321:γ 1315:μ 1308:¯ 1305:ψ 1293:ρ 1289:ψ 1283:ν 1279:∂ 1273:ρ 1270:ν 1267:μ 1263:γ 1257:μ 1250:¯ 1247:ψ 1240:δ 1217:δ 1192:μ 1188:ψ 1156:ρ 1152:γ 1146:ν 1142:γ 1136:μ 1129:γ 1110:≡ 1105:ρ 1102:ν 1099:μ 1095:γ 1069:μ 1065:ψ 1036:ρ 1032:ψ 1026:ν 1022:∂ 1016:ρ 1013:ν 1010:μ 1006:γ 1000:μ 993:¯ 990:ψ 922:α 918:ϵ 914:≡ 911:ϵ 891:ϵ 886:μ 882:∂ 873:μ 869:ψ 865:→ 860:μ 856:ψ 838:gravitino 789:μ 785:ψ 759:ν 755:ψ 744:ν 741:μ 737:σ 727:− 722:ρ 718:∂ 712:κ 708:γ 698:γ 692:ν 689:ρ 686:κ 683:μ 679:ϵ 668:μ 661:¯ 658:ψ 638:− 481:ν 477:ψ 451:ν 447:γ 438:μ 434:γ 417:≡ 412:ν 409:μ 405:σ 358:γ 348:γ 338:γ 328:γ 312:γ 267:κ 241:κ 237:γ 210:ν 207:ρ 204:κ 201:μ 197:ϵ 165:ν 161:ψ 150:ν 147:μ 143:σ 133:− 128:ρ 124:∂ 118:κ 114:γ 104:γ 98:ν 95:ρ 92:κ 89:μ 85:ϵ 65:in 1941. 2600:Fermions 903:, where 51:fermions 2590:Spinors 2543:Bibcode 2506:Bibcode 2469:Bibcode 2417:Bibcode 2401:Sources 2379:Bibcode 2351:Bibcode 2022:where 602:⁠ 590:⁠ 586:⁠ 574:⁠ 563:⁠ 551:⁠ 547:⁠ 535:⁠ 531:⁠ 519:⁠ 515:⁠ 503:⁠ 224:is the 38:is the 2561:  2524:  2487:  2435:  827:Δ 606:part. 533:) ⊗ (( 497:spinor 468:, and 303:) and 259:(with 188:where 34:, the 2281:arXiv 588:) ⊕ ( 49:-3/2 2559:ISSN 2522:ISSN 2485:ISSN 2433:ISSN 604:, 1) 572:(1, 255:are 61:and 47:spin 2551:doi 2514:doi 2502:188 2477:doi 2465:186 2425:doi 2387:doi 2375:120 2359:doi 2347:114 2324:doi 2291:doi 940:of 45:of 30:In 2576:: 2557:. 2549:. 2539:17 2537:. 2520:. 2512:. 2500:. 2483:. 2475:. 2463:. 2431:. 2423:. 2413:60 2411:. 2385:. 2373:. 2367:; 2357:. 2345:. 2320:16 2318:. 2314:. 2289:. 2277:16 2275:. 2271:. 2128:: 1868:0. 1704:0. 807:. 617:: 565:)) 517:, 376:, 228:, 2565:. 2553:: 2545:: 2528:. 2516:: 2508:: 2491:. 2479:: 2471:: 2455:. 2439:. 2427:: 2419:: 2393:. 2389:: 2381:: 2365:. 2361:: 2353:: 2330:. 2326:: 2299:. 2293:: 2283:: 2203:. 2185:A 2181:e 2178:i 2162:= 2153:D 2070:T 2067:T 2062:i 2035:2 2007:, 1999:i 1989:0 1977:2 1966:j 1956:j 1945:+ 1940:T 1937:T 1932:i 1924:= 1919:i 1910:, 1904:= 1899:0 1865:= 1841:, 1838:0 1835:= 1811:, 1808:0 1805:= 1750:0 1747:= 1701:= 1642:0 1639:= 1634:S 1631:R 1625:L 1596:, 1535:2 1532:= 1527:S 1524:R 1518:L 1481:+ 1359:= 1298:+ 1237:= 1232:S 1229:R 1223:L 1164:. 1159:] 1133:[ 1122:! 1119:3 1115:1 1041:, 983:= 978:S 975:R 969:L 878:+ 818:( 750:) 733:m 730:i 702:5 674:( 647:2 644:1 635:= 630:L 599:2 596:/ 593:1 583:2 580:/ 577:1 560:2 557:/ 554:1 544:2 541:/ 538:1 528:2 525:/ 522:1 512:2 509:/ 506:1 501:( 456:] 443:, 430:[ 425:2 422:i 384:m 362:3 352:2 342:1 332:0 324:i 321:= 316:5 291:3 288:, 285:2 282:, 279:1 276:, 273:0 270:= 173:0 170:= 156:) 139:m 136:i 108:5 80:( 20:)

Index

Rarita-Schwinger equation
theoretical physics
relativistic
field equation
spin
fermions
Dirac equation
William Rarita
Julian Schwinger
Levi-Civita symbol
Dirac matrices
spinor
representation of the Lorentz group
Euler–Lagrange equation
Lagrangian
Dirac adjoint
wave function
delta baryons
gravitino
elementary particle
supersymmetry
supergravity
Fierz–Pauli
gauge covariant derivative
electromagnetism
quantization
"Massless Rarita-Schwinger equations: Half and three halves spin solution"
arXiv
2305.00106
doi

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