Knowledge

Stark effect

Source 📝

973: 2608: 104: 20: 701: 1433: 2277: 2855: 275:) of the 2s and 2p states where the electron tends to be to the left, which will acquire a lower energy, and other hybrid orbitals where the electron tends to be to the right, which will acquire a higher energy. Therefore, the formerly degenerate energy levels will split into slightly lower and slightly higher energy levels. 1219: 1585: 3032:
of finite width. These resonances may decay in finite time via field ionization. For low lying states and not too strong fields the decay times are so long, however, that for all practical purposes the system can be regarded as bound. For highly excited states and/or very strong fields ionization may
240:
An electric field pointing from left to right, for example, tends to pull nuclei to the right and electrons to the left. In another way of viewing it, if an electronic state has its electron disproportionately to the left, its energy is lowered, while if it has the electron disproportionately to the
219:
discussed at length the Stark effect in his third paper on quantum theory (in which he introduced his perturbation theory), once in the manner of the 1916 work of Epstein (but generalized from the old to the new quantum theory) and once by his (first-order) perturbation approach. Finally, Epstein
968:{\displaystyle V_{\mathrm {int} }\approx \phi (\mathbf {0} )\int _{\mathcal {V}}\rho (\mathbf {r} )d^{3}r-\sum _{i=1}^{3}F_{i}\int _{\mathcal {V}}\rho (\mathbf {r} )r_{i}d^{3}r\equiv q\phi (\mathbf {0} )-\sum _{i=1}^{3}\mu _{i}F_{i}=q\phi (\mathbf {0} )-{\boldsymbol {\mu }}\cdot \mathbf {F} ,} 175:
performed classical mechanical calculations of quasi-elastically bound electrons in an electric field. By using experimental indices of refraction he gave an estimate of the Stark splittings. This estimate was a few orders of magnitude too low. Not deterred by this prediction, Stark undertook
2272: 1074:
Turning now to quantum mechanics an atom or a molecule can be thought of as a collection of point charges (electrons and nuclei), so that the second definition of the dipole applies. The interaction of atom or molecule with a uniform external field is described by the operator
2617: 2603:{\displaystyle E_{k}^{(2)}=\sum _{k'\neq k}{\frac {\langle \psi _{k}^{0}|V_{\mathrm {int} }|\psi _{k^{\prime }}^{0}\rangle \langle \psi _{k'}^{0}|V_{\mathrm {int} }|\psi _{k}^{0}\rangle }{E_{k}^{(0)}-E_{k'}^{(0)}}}\equiv -{\frac {1}{2}}\sum _{i,j=1}^{3}\alpha _{ij}F_{i}F_{j}} 1646:
have opposite parity (obtain plus and minus under inversion), because only functions of opposite parity give non-vanishing matrix elements. Degenerate zeroth-order states of opposite parity occur for excited hydrogen-like (one-electron) atoms or Rydberg states. Neglecting
2980: 481: 2068:. The first-order perturbation matrix on basis of the unperturbed rigid rotor function is non-zero and can be diagonalized. This gives shifts and splittings in the rotational spectrum. Quantitative analysis of these Stark shift yields the permanent 1464: 668: 1870: 220:
reconsidered the linear and quadratic Stark effect from the point of view of the new quantum theory. He derived equations for the line intensities which were a decided improvement over Kramers's results obtained by the old quantum theory.
2045: 584: 2086: 1428:{\displaystyle (\mathbf {V} _{\mathrm {int} })_{kl}=\langle \psi _{k}^{0}|V_{\mathrm {int} }|\psi _{l}^{0}\rangle =-\mathbf {F} \cdot \langle \psi _{k}^{0}|{\boldsymbol {\mu }}|\psi _{l}^{0}\rangle ,\qquad k,l=1,\ldots ,g.} 1130: 3212:
Intensities of Spectral Lines. On the Application of the Quantum Theory to the Problem of Relative Intensities of the Components of the Fine Structure and of the Stark Effect of the Lines of the Hydrogen
1058:
this is no longer true. Nevertheless, it is often justified to omit it in this case, too. Indeed, the Stark effect is observed in spectral lines, which are emitted when an electron "jumps" between two
2871: 389: 85:. Although initially coined for the static case, it is also used in the wider context to describe the effect of time-dependent electric fields. In particular, the Stark effect is responsible for the 1735: 1202: 2850:{\displaystyle \alpha _{ij}=-2\sum _{k'\neq k}{\frac {\langle \psi _{k}^{0}|\mu _{i}|\psi _{k'}^{0}\rangle \langle \psi _{k'}^{0}|\mu _{j}|\psi _{k}^{0}\rangle }{E_{k}^{(0)}-E_{k'}^{(0)}}}.} 1784: 1459: 384: 326: 1930: 589: 494: 1015: 696: 350: 1644: 3010: 227:
theory of the atom, higher-order corrections are not. Measurements of the Stark effect under high field strengths confirmed the correctness of the new quantum theory.
3088: 203:, with corrections for relativistic kinetic energy and coupling between electron spin and orbital motion. The first quantum mechanical treatment (in the framework of 1439:= 1 (as is often the case for electronic states of molecules) the first-order energy becomes proportional to the expectation (average) value of the dipole operator 1910: 1890: 1779: 1755: 1580:{\displaystyle E^{(1)}=-\mathbf {F} \cdot \langle \psi _{1}^{0}|{\boldsymbol {\mu }}|\psi _{1}^{0}\rangle =-\mathbf {F} \cdot \langle {\boldsymbol {\mu }}\rangle .} 3024:
The perturbative treatment of the Stark effect has some problems. In the presence of an electric field, states of atoms and molecules that were previously bound (
1052: 1078: 993: 3346: 3108:
Courtney, Michael; Neal Spellmeyer; Hong Jiao; Daniel Kleppner (1995). "Classical, semiclassical, and quantum dynamics of lithium in an electric field".
1054:), so the first, monopole, term in the expression above is identically zero. This is also the case for a neutral atom or molecule. However, for an 93:. For most spectral lines, the Stark effect is either linear (proportional to the applied electric field) or quadratic with a high accuracy. 1662: 2267:{\displaystyle H^{(0)}\psi _{k}^{0}=E_{k}^{(0)}\psi _{k}^{0},\quad k=0,1,\ldots ,\quad E_{0}^{(0)}<E_{1}^{(0)}\leq E_{2}^{(0)},\dots } 1604:. Atoms and molecules possessing inversion symmetry do not have a (permanent) dipole moment and hence do not show a linear Stark effect. 1066:
of the radiator but not its charge, the effects of the monopole interaction on the initial and final states exactly cancel each other.
3288: 223:
While the first-order-perturbation (linear) Stark effect in hydrogen is in agreement with both the old Bohr–Sommerfeld model and the
2868:(which is often justified — unless extremely weak electric fields are considered), the polarizability tensor of atoms is isotropic, 1920: 491:
converges fast, so only a few first terms give an accurate approximation. Namely, keeping only the zero- and first-order terms,
1923:(but not for linear and asymmetric molecules). In first approximation a molecule may be seen as a rigid rotor. A symmetric top 3455: 3428: 3406: 3380: 3356: 156:. The discovery of this effect contributed importantly to the development of quantum theory and Stark was awarded with the 1151: 3171:(Observations of the effect of the electric field on spectral lines I. Transverse effect), Annalen der Physik, vol. 54: 2975:{\displaystyle \alpha _{ij}\equiv \alpha _{0}\delta _{ij}\Longrightarrow E^{(2)}=-{\frac {1}{2}}\alpha _{0}F^{2}.} 476:{\displaystyle V_{\mathrm {int} }=\int _{\mathcal {V}}\rho (\mathbf {r} )\phi (\mathbf {r} )\,d^{3}\mathbf {r} .} 3219:(On the influence of an electric field on the fine structure of hydrogen lines), Zeitschrift fĂŒr Physik, vol. 119:= 0. Note how a complicated pattern of the energy levels emerges as the electric field increases, not unlike 3236:(On the hydrogen spectrum from the point of view of the new quantum mechanics). Zeitschrift fĂŒr Physik, vol. 3068: 96:
The Stark effect can be observed both for emission and absorption lines. The latter is sometimes called the
2081: 663:{\textstyle F_{i}\equiv -\left.\left({\frac {\partial \phi }{\partial r_{i}}}\right)\right|_{\mathbf {0} }} 1442: 3460: 2080:
As stated, the quadratic Stark effect is described by second-order perturbation theory. The zeroth-order
358: 300: 3289:"Locally Excited State-Charge Transfer State Coupled Dyes as Optically Responsive Neuron Firing Probes" 3078: 248:, because the electron is more distant from the nucleus, so it travels farther left and farther right. 148:, who discovered it in 1913. It was independently discovered in the same year by the Italian physicist 3287:
Sirbu, Dumitru; Butcher, John B.; Waddell, Paul G.; Andras, Peter; Benniston, Andrew C. (2017-09-18).
998: 353: 1865:{\displaystyle 16=1+3+5+7\;\;\Longrightarrow \;\;n=4\;{\text{contains}}\;s\oplus p\oplus d\oplus f.} 677: 331: 3175:, pp. 965–983 (1914). Published earlier (1913) in Sitzungsberichten der Kgl. Preuss. Akad. d. Wiss. 3063: 1617: 35: 3450: 2988: 487:
and quantum-mechanically alike. If the potential varies weakly over the charge distribution, the
252: 196: 86: 46: 28: 2069: 157: 199:
derived formulas for intensities of spectral transitions. Kramers also included the effect of
3465: 3046: 272: 268: 1614:
for systems with an inversion center it is necessary that some of the unperturbed functions
3117: 1895: 1875: 1764: 1740: 1208:= 1). According to perturbation theory the first-order energies are the eigenvalues of the 176:
measurements on excited states of the hydrogen atom and succeeded in observing splittings.
2040:{\displaystyle |JKM\rangle =(D_{MK}^{J})^{*}\quad {\text{with}}\quad M,K=-J,-J+1,\dots ,J} 216: 8: 2865: 1133: 1031: 579:{\displaystyle \phi (\mathbf {r} )\approx \phi (\mathbf {0} )-\sum _{i=1}^{3}r_{i}F_{i},} 488: 284: 191:
were independently able to derive equations for the linear and quadratic Stark effect in
184: 3121: 3395: 3370: 3083: 3073: 978: 188: 180: 120: 3201:
K. Schwarzschild, Sitzungsberichten der Kgl. Preuss. Akad. d. Wiss. April 1916, p. 548
3169:
Beobachtungen ĂŒber den Effekt des elektrischen Feldes auf Spektrallinien I. Quereffekt
3424: 3402: 3376: 3352: 3319: 3311: 3217:Über den Einfluß eines elektrischen Feldes auf die Feinstruktur der Wasserstofflinien 3133: 3025: 1063: 484: 224: 204: 149: 58: 81:, where a spectral line is split into several components due to the presence of the 23:
Computed energy level spectrum of hydrogen as a function of the electric field near
3303: 3125: 1601: 1018: 208: 128: 124: 90: 3341: 2065: 290: 168: 244:
Other things being equal, the effect of the electric field is greater for outer
3107: 2611: 1648: 294: 264: 260: 245: 212: 200: 172: 145: 82: 74: 50: 1757:
is the azimuthal (angular momentum) quantum number. For instance, the excited
3444: 3315: 3129: 3058: 164: 78: 70: 3323: 3307: 3154:(On the electric analogue of the Zeeman effect), Annalen der Physik, vol. 3034: 1125:{\displaystyle V_{\mathrm {int} }=-\mathbf {F} \cdot {\boldsymbol {\mu }}.} 132: 108: 3137: 1924: 1059: 3271:
The Stark Effect from the Point of View of Schroedinger's Quantum Theory
2982:
For some molecules this expression is a reasonable approximation, too.
256: 3234:Über dass Wasserstoffspektrum vom Standpunkt der neuen Quantenmechanik 3029: 1593:
of the first rank), the diagonal elements of the perturbation matrix
1148:-fold degenerate state with orthonormal zeroth-order state functions 3045:
The Stark effect is at the basis of the spectral shift measured for
1028:
Classical macroscopic objects are usually neutral or quasi-neutral (
1132:
This operator is used as a perturbation in first- and second-order
192: 1919:
The first-order Stark effect occurs in rotational transitions of
1590: 1022: 3016:
positive, i.e., the quadratic Stark shift is always negative.
297:. The interaction energy of a continuous charge distribution 89:(Stark broadening) of spectral lines by charged particles in 3388:(Chapter 17 provides a comprehensive treatment, as of 1935.) 100:, but this term is no longer used in the modern literature. 611: 289:
The Stark effect originates from the interaction between a
3368: 103: 73:
of atoms and molecules due to the presence of an external
19: 3286: 1136:
to account for the first- and second-order Stark effect.
1055: 111:-level spectrum as a function of the electric field near 1651:
effects, such a state with the principal quantum number
3340: 3033:
have to be accounted for. (See also the article on the
2274:
is assumed to be solved. The perturbation theory gives
259:, an electron has the same energy whether it is in the 1730:{\displaystyle n^{2}=\sum _{\ell =0}^{n-1}(2\ell +1),} 592: 53:
breaks the degeneracy. Energy levels can cross due to
2991: 2874: 2620: 2280: 2089: 1933: 1912:
are odd under parity. Hence hydrogen-like atoms with
1898: 1878: 1787: 1767: 1743: 1665: 1620: 1467: 1445: 1222: 1154: 1081: 1034: 1001: 981: 704: 680: 497: 392: 361: 334: 303: 267:
states. However, in an electric field, there will be
3049:
used for imaging of the firing activity of neurons.
3347:
A History of the Theories of Aether and Electricity
1197:{\displaystyle \psi _{1}^{0},\ldots ,\psi _{g}^{0}} 1062:. Since such a transition only alters the internal 3394: 3004: 2974: 2849: 2602: 2266: 2039: 1904: 1884: 1864: 1773: 1749: 1729: 1638: 1579: 1453: 1427: 1196: 1124: 1046: 1009: 987: 967: 690: 662: 578: 475: 378: 344: 320: 3152:Ueber das Elektrische Analogon des Zeemaneffectes 3442: 2051:+1)-fold degenerate energy for |K| > 0 and (2 1589:Because the electric dipole moment is a vector ( 293:distribution (atom or molecule) and an external 3265: 3263: 152:, and in Italy it is thus sometimes called the 144:The effect is named after the German physicist 1144:Let the unperturbed atom or molecule be in a 3392: 3260: 2786: 2728: 2725: 2667: 2466: 2400: 2397: 2329: 1948: 1892:are even under parity, while those with odd 1571: 1563: 1546: 1498: 1388: 1340: 1323: 1262: 3418: 3101: 3028:), become formally (non-square-integrable) 77:. It is the electric-field analogue of the 16:Spectral line splitting in electrical field 3369:E. U. Condon & G. H. Shortley (1935). 1837: 1831: 1821: 1820: 1816: 1815: 1017:are, respectively, the total charge (zero 251:The Stark effect can lead to splitting of 2055:+1)-fold degenerate energy for K=0. Here 454: 102: 18: 1567: 1522: 1447: 1364: 1115: 950: 586:where we introduced the electric field 3443: 1204:. (Non-degeneracy is the special case 1069: 278: 3436:(Stark effect for rotating molecules) 3349:. II. The Modern Theories (1800-1950) 1916:>1 show first-order Stark effect. 1607:In order to obtain a non-zero matrix 1600:vanish between states with a certain 698:. Therefore, the interaction becomes 3210:H. A. Kramers, Roy. Danish Academy, 3089:Stark effect in semiconductor optics 1454:{\displaystyle {\boldsymbol {\mu }}} 3364:(Early history of the Stark effect) 379:{\displaystyle \phi (\mathbf {r} )} 321:{\displaystyle \rho (\mathbf {r} )} 13: 3334: 3251:Quantisierung als Eigenwertproblem 2861:gives the quadratic Stark effect. 2440: 2437: 2434: 2385: 2364: 2361: 2358: 1872:The one-electron states with even 1297: 1294: 1291: 1240: 1237: 1234: 1094: 1091: 1088: 819: 746: 717: 714: 711: 683: 628: 620: 420: 405: 402: 399: 337: 328:, confined within a finite volume 179:By the use of the Bohr–Sommerfeld 14: 3477: 3351:. American Institute of Physics. 1761:= 4 state contains the following 69:is the shifting and splitting of 1927:has the unperturbed eigenstates 1556: 1491: 1333: 1228: 1107: 958: 939: 875: 832: 759: 733: 654: 522: 505: 466: 447: 433: 369: 311: 3280: 3040: 2188: 2163: 2075: 2072:of the symmetric top molecule. 1991: 1985: 1394: 1010:{\displaystyle \mathbf {\mu } } 3375:. Cambridge University Press. 3296:Chemistry - A European Journal 3243: 3226: 3204: 3195: 3178: 3161: 3144: 2928: 2922: 2914: 2836: 2830: 2807: 2801: 2767: 2752: 2701: 2686: 2516: 2510: 2487: 2481: 2447: 2424: 2371: 2348: 2297: 2291: 2253: 2247: 2229: 2223: 2205: 2199: 2140: 2134: 2101: 2095: 1976: 1954: 1935: 1817: 1721: 1706: 1527: 1517: 1479: 1473: 1369: 1359: 1304: 1281: 1247: 1223: 1139: 943: 935: 879: 871: 836: 828: 763: 755: 737: 729: 691:{\displaystyle {\mathcal {V}}} 526: 518: 509: 501: 451: 443: 437: 429: 373: 365: 345:{\displaystyle {\mathcal {V}}} 315: 307: 1: 3186:Zur Theorie des Starkeffektes 3094: 3069:Quantum-confined Stark effect 1639:{\displaystyle \psi _{i}^{0}} 1216:matrix with general element 241:right, its energy is raised. 3456:Foundational quantum physics 3372:The Theory of Atomic Spectra 1025:of the charge distribution. 230: 7: 3401:. Springer-Verlag, Berlin. 3253:, Annalen der Physik, vol. 3188:, Annalen der Physik, vol. 3052: 3019: 3005:{\displaystyle \alpha _{0}} 2610:with the components of the 235: 10: 3482: 3421:Molecular Rotation Spectra 3397:Theoretical Atomic Physics 282: 139: 483:This expression is valid 163:Inspired by the magnetic 3414:(Stark effect for atoms) 3257:Issue 13, 437–490 (1926) 3130:10.1103/PhysRevA.51.3604 253:degenerate energy levels 3342:Edmond Taylor Whittaker 3273:, Physical Review, vol 1921:symmetric top molecules 674:to be somewhere within 670:and assumed the origin 354:electrostatic potential 29:magnetic quantum number 3308:10.1002/chem.201703366 3079:Inglis–Teller equation 3047:voltage-sensitive dyes 3006: 2976: 2851: 2604: 2566: 2268: 2070:electric dipole moment 2041: 1906: 1886: 1866: 1775: 1751: 1731: 1705: 1640: 1581: 1455: 1429: 1198: 1126: 1048: 1011: 989: 969: 905: 802: 692: 664: 580: 552: 477: 380: 346: 322: 273:quantum superpositions 255:. For example, in the 181:("old") quantum theory 171:'s explanation of it, 158:Nobel Prize in Physics 136: 62: 3393:H. Friedrich (1990). 3223:, pp. 199–223 (1920) 3158:, pp. 197–208 (1901). 3007: 2985:For the ground state 2977: 2852: 2612:polarizability tensor 2605: 2540: 2269: 2064:is an element of the 2042: 1907: 1905:{\displaystyle \ell } 1887: 1885:{\displaystyle \ell } 1867: 1776: 1774:{\displaystyle \ell } 1752: 1750:{\displaystyle \ell } 1732: 1679: 1659:-fold degenerate and 1641: 1582: 1456: 1430: 1199: 1127: 1049: 1012: 990: 970: 885: 782: 693: 665: 581: 532: 478: 381: 347: 323: 154:Stark–Lo Surdo effect 106: 55:underlying symmetries 22: 3419:H. W. Kroto (1992). 3277:, pp. 695–710 (1926) 3192:, pp. 489–520 (1916) 3064:Autler–Townes effect 2989: 2872: 2618: 2278: 2087: 1931: 1896: 1876: 1785: 1765: 1741: 1663: 1618: 1465: 1443: 1220: 1152: 1079: 1032: 999: 979: 702: 678: 590: 495: 390: 359: 332: 301: 263:state or any of the 195:. Four years later, 167:, and especially by 98:inverse Stark effect 49:; application of an 47:degenerate sublevels 3423:. Dover, New York. 3302:(58): 14639–14649. 3122:1995PhRvA..51.3604C 2866:hyperfine structure 2840: 2811: 2785: 2750: 2724: 2684: 2520: 2491: 2465: 2422: 2396: 2346: 2301: 2257: 2233: 2209: 2159: 2144: 2120: 1974: 1635: 1545: 1515: 1387: 1357: 1322: 1279: 1193: 1169: 1134:perturbation theory 1070:Perturbation theory 1047:{\displaystyle q=0} 489:multipole expansion 352:, with an external 285:Multipole expansion 279:Multipole expansion 87:pressure broadening 3461:Physical phenomena 3084:Electric field NMR 3074:Stark spectroscopy 3002: 2972: 2847: 2815: 2791: 2771: 2731: 2705: 2670: 2663: 2600: 2495: 2471: 2451: 2403: 2375: 2332: 2325: 2281: 2264: 2237: 2213: 2189: 2145: 2124: 2106: 2037: 1957: 1902: 1882: 1862: 1771: 1747: 1727: 1636: 1621: 1577: 1531: 1501: 1451: 1425: 1373: 1343: 1308: 1265: 1194: 1179: 1155: 1122: 1064:degrees of freedom 1044: 1007: 985: 965: 688: 660: 576: 473: 376: 342: 318: 225:quantum-mechanical 189:Karl Schwarzschild 160:in the year 1919. 137: 63: 3430:978-0-486-67259-5 3408:978-0-387-54179-2 3382:978-0-521-09209-8 3358:978-0-88318-523-0 3110:Physical Review A 3026:square-integrable 2947: 2842: 2643: 2538: 2522: 2305: 1989: 1835: 988:{\displaystyle q} 642: 217:Erwin Schrödinger 205:Werner Heisenberg 150:Antonino Lo Surdo 129:dynamical systems 59:Coulomb potential 57:of motion in the 3473: 3434: 3412: 3400: 3386: 3362: 3328: 3327: 3293: 3284: 3278: 3267: 3258: 3249:E. Schrödinger, 3247: 3241: 3230: 3224: 3215:, p. 287 (1919); 3208: 3202: 3199: 3193: 3182: 3176: 3165: 3159: 3148: 3142: 3141: 3116:(5): 3604–3620. 3105: 3011: 3009: 3008: 3003: 3001: 3000: 2981: 2979: 2978: 2973: 2968: 2967: 2958: 2957: 2948: 2940: 2932: 2931: 2913: 2912: 2900: 2899: 2887: 2886: 2856: 2854: 2853: 2848: 2843: 2841: 2839: 2828: 2827: 2810: 2799: 2789: 2784: 2779: 2770: 2765: 2764: 2755: 2749: 2744: 2743: 2723: 2718: 2717: 2704: 2699: 2698: 2689: 2683: 2678: 2665: 2662: 2655: 2633: 2632: 2609: 2607: 2606: 2601: 2599: 2598: 2589: 2588: 2579: 2578: 2565: 2560: 2539: 2531: 2523: 2521: 2519: 2508: 2507: 2490: 2479: 2469: 2464: 2459: 2450: 2445: 2444: 2443: 2427: 2421: 2416: 2415: 2395: 2390: 2389: 2388: 2374: 2369: 2368: 2367: 2351: 2345: 2340: 2327: 2324: 2317: 2300: 2289: 2273: 2271: 2270: 2265: 2256: 2245: 2232: 2221: 2208: 2197: 2158: 2153: 2143: 2132: 2119: 2114: 2105: 2104: 2046: 2044: 2043: 2038: 1990: 1987: 1984: 1983: 1973: 1968: 1938: 1911: 1909: 1908: 1903: 1891: 1889: 1888: 1883: 1871: 1869: 1868: 1863: 1836: 1833: 1780: 1778: 1777: 1772: 1756: 1754: 1753: 1748: 1736: 1734: 1733: 1728: 1704: 1693: 1675: 1674: 1645: 1643: 1642: 1637: 1634: 1629: 1586: 1584: 1583: 1578: 1570: 1559: 1544: 1539: 1530: 1525: 1520: 1514: 1509: 1494: 1483: 1482: 1460: 1458: 1457: 1452: 1450: 1434: 1432: 1431: 1426: 1386: 1381: 1372: 1367: 1362: 1356: 1351: 1336: 1321: 1316: 1307: 1302: 1301: 1300: 1284: 1278: 1273: 1258: 1257: 1245: 1244: 1243: 1231: 1203: 1201: 1200: 1195: 1192: 1187: 1168: 1163: 1131: 1129: 1128: 1123: 1118: 1110: 1099: 1098: 1097: 1053: 1051: 1050: 1045: 1016: 1014: 1013: 1008: 1006: 994: 992: 991: 986: 974: 972: 971: 966: 961: 953: 942: 925: 924: 915: 914: 904: 899: 878: 858: 857: 848: 847: 835: 824: 823: 822: 812: 811: 801: 796: 775: 774: 762: 751: 750: 749: 736: 722: 721: 720: 697: 695: 694: 689: 687: 686: 669: 667: 666: 661: 659: 658: 657: 651: 647: 643: 641: 640: 639: 626: 618: 602: 601: 585: 583: 582: 577: 572: 571: 562: 561: 551: 546: 525: 508: 482: 480: 479: 474: 469: 464: 463: 450: 436: 425: 424: 423: 410: 409: 408: 385: 383: 382: 377: 372: 351: 349: 348: 343: 341: 340: 327: 325: 324: 319: 314: 209:matrix mechanics 3481: 3480: 3476: 3475: 3474: 3472: 3471: 3470: 3441: 3440: 3431: 3409: 3383: 3359: 3337: 3335:Further reading 3332: 3331: 3291: 3285: 3281: 3269:P. S. Epstein, 3268: 3261: 3248: 3244: 3231: 3227: 3209: 3205: 3200: 3196: 3184:P. S. Epstein, 3183: 3179: 3166: 3162: 3149: 3145: 3106: 3102: 3097: 3055: 3043: 3022: 2996: 2992: 2990: 2987: 2986: 2963: 2959: 2953: 2949: 2939: 2921: 2917: 2905: 2901: 2895: 2891: 2879: 2875: 2873: 2870: 2869: 2864:Neglecting the 2829: 2820: 2819: 2800: 2795: 2790: 2780: 2775: 2766: 2760: 2756: 2751: 2745: 2736: 2735: 2719: 2710: 2709: 2700: 2694: 2690: 2685: 2679: 2674: 2666: 2664: 2648: 2647: 2625: 2621: 2619: 2616: 2615: 2594: 2590: 2584: 2580: 2571: 2567: 2561: 2544: 2530: 2509: 2500: 2499: 2480: 2475: 2470: 2460: 2455: 2446: 2433: 2432: 2428: 2423: 2417: 2408: 2407: 2391: 2384: 2380: 2379: 2370: 2357: 2356: 2352: 2347: 2341: 2336: 2328: 2326: 2310: 2309: 2290: 2285: 2279: 2276: 2275: 2246: 2241: 2222: 2217: 2198: 2193: 2154: 2149: 2133: 2128: 2115: 2110: 2094: 2090: 2088: 2085: 2084: 2078: 2066:Wigner D-matrix 2063: 1986: 1979: 1975: 1969: 1961: 1934: 1932: 1929: 1928: 1897: 1894: 1893: 1877: 1874: 1873: 1832: 1786: 1783: 1782: 1766: 1763: 1762: 1742: 1739: 1738: 1694: 1683: 1670: 1666: 1664: 1661: 1660: 1630: 1625: 1619: 1616: 1615: 1613: 1599: 1566: 1555: 1540: 1535: 1526: 1521: 1516: 1510: 1505: 1490: 1472: 1468: 1466: 1463: 1462: 1446: 1444: 1441: 1440: 1382: 1377: 1368: 1363: 1358: 1352: 1347: 1332: 1317: 1312: 1303: 1290: 1289: 1285: 1280: 1274: 1269: 1250: 1246: 1233: 1232: 1227: 1226: 1221: 1218: 1217: 1188: 1183: 1164: 1159: 1153: 1150: 1149: 1142: 1114: 1106: 1087: 1086: 1082: 1080: 1077: 1076: 1072: 1033: 1030: 1029: 1002: 1000: 997: 996: 980: 977: 976: 957: 949: 938: 920: 916: 910: 906: 900: 889: 874: 853: 849: 843: 839: 831: 818: 817: 813: 807: 803: 797: 786: 770: 766: 758: 745: 744: 740: 732: 710: 709: 705: 703: 700: 699: 682: 681: 679: 676: 675: 653: 652: 635: 631: 627: 619: 617: 613: 610: 609: 597: 593: 591: 588: 587: 567: 563: 557: 553: 547: 536: 521: 504: 496: 493: 492: 465: 459: 455: 446: 432: 419: 418: 414: 398: 397: 393: 391: 388: 387: 368: 360: 357: 356: 336: 335: 333: 330: 329: 310: 302: 299: 298: 287: 281: 269:hybrid orbitals 246:electron shells 238: 233: 197:Hendrik Kramers 169:Hendrik Lorentz 142: 17: 12: 11: 5: 3479: 3469: 3468: 3463: 3458: 3453: 3451:Atomic physics 3439: 3438: 3429: 3416: 3407: 3390: 3381: 3366: 3357: 3336: 3333: 3330: 3329: 3279: 3259: 3242: 3225: 3203: 3194: 3177: 3160: 3143: 3099: 3098: 3096: 3093: 3092: 3091: 3086: 3081: 3076: 3071: 3066: 3061: 3054: 3051: 3042: 3039: 3021: 3018: 2999: 2995: 2971: 2966: 2962: 2956: 2952: 2946: 2943: 2938: 2935: 2930: 2927: 2924: 2920: 2916: 2911: 2908: 2904: 2898: 2894: 2890: 2885: 2882: 2878: 2846: 2838: 2835: 2832: 2826: 2823: 2818: 2814: 2809: 2806: 2803: 2798: 2794: 2788: 2783: 2778: 2774: 2769: 2763: 2759: 2754: 2748: 2742: 2739: 2734: 2730: 2727: 2722: 2716: 2713: 2708: 2703: 2697: 2693: 2688: 2682: 2677: 2673: 2669: 2661: 2658: 2654: 2651: 2646: 2642: 2639: 2636: 2631: 2628: 2624: 2597: 2593: 2587: 2583: 2577: 2574: 2570: 2564: 2559: 2556: 2553: 2550: 2547: 2543: 2537: 2534: 2529: 2526: 2518: 2515: 2512: 2506: 2503: 2498: 2494: 2489: 2486: 2483: 2478: 2474: 2468: 2463: 2458: 2454: 2449: 2442: 2439: 2436: 2431: 2426: 2420: 2414: 2411: 2406: 2402: 2399: 2394: 2387: 2383: 2378: 2373: 2366: 2363: 2360: 2355: 2350: 2344: 2339: 2335: 2331: 2323: 2320: 2316: 2313: 2308: 2304: 2299: 2296: 2293: 2288: 2284: 2263: 2260: 2255: 2252: 2249: 2244: 2240: 2236: 2231: 2228: 2225: 2220: 2216: 2212: 2207: 2204: 2201: 2196: 2192: 2187: 2184: 2181: 2178: 2175: 2172: 2169: 2166: 2162: 2157: 2152: 2148: 2142: 2139: 2136: 2131: 2127: 2123: 2118: 2113: 2109: 2103: 2100: 2097: 2093: 2077: 2074: 2059: 2036: 2033: 2030: 2027: 2024: 2021: 2018: 2015: 2012: 2009: 2006: 2003: 2000: 1997: 1994: 1982: 1978: 1972: 1967: 1964: 1960: 1956: 1953: 1950: 1947: 1944: 1941: 1937: 1901: 1881: 1861: 1858: 1855: 1852: 1849: 1846: 1843: 1840: 1830: 1827: 1824: 1819: 1814: 1811: 1808: 1805: 1802: 1799: 1796: 1793: 1790: 1770: 1746: 1726: 1723: 1720: 1717: 1714: 1711: 1708: 1703: 1700: 1697: 1692: 1689: 1686: 1682: 1678: 1673: 1669: 1649:fine-structure 1633: 1628: 1624: 1611: 1597: 1576: 1573: 1569: 1565: 1562: 1558: 1554: 1551: 1548: 1543: 1538: 1534: 1529: 1524: 1519: 1513: 1508: 1504: 1500: 1497: 1493: 1489: 1486: 1481: 1478: 1475: 1471: 1449: 1424: 1421: 1418: 1415: 1412: 1409: 1406: 1403: 1400: 1397: 1393: 1390: 1385: 1380: 1376: 1371: 1366: 1361: 1355: 1350: 1346: 1342: 1339: 1335: 1331: 1328: 1325: 1320: 1315: 1311: 1306: 1299: 1296: 1293: 1288: 1283: 1277: 1272: 1268: 1264: 1261: 1256: 1253: 1249: 1242: 1239: 1236: 1230: 1225: 1191: 1186: 1182: 1178: 1175: 1172: 1167: 1162: 1158: 1141: 1138: 1121: 1117: 1113: 1109: 1105: 1102: 1096: 1093: 1090: 1085: 1071: 1068: 1043: 1040: 1037: 1005: 984: 964: 960: 956: 952: 948: 945: 941: 937: 934: 931: 928: 923: 919: 913: 909: 903: 898: 895: 892: 888: 884: 881: 877: 873: 870: 867: 864: 861: 856: 852: 846: 842: 838: 834: 830: 827: 821: 816: 810: 806: 800: 795: 792: 789: 785: 781: 778: 773: 769: 765: 761: 757: 754: 748: 743: 739: 735: 731: 728: 725: 719: 716: 713: 708: 685: 656: 650: 646: 638: 634: 630: 625: 622: 616: 612: 608: 605: 600: 596: 575: 570: 566: 560: 556: 550: 545: 542: 539: 535: 531: 528: 524: 520: 517: 514: 511: 507: 503: 500: 472: 468: 462: 458: 453: 449: 445: 442: 439: 435: 431: 428: 422: 417: 413: 407: 404: 401: 396: 375: 371: 367: 364: 339: 317: 313: 309: 306: 295:electric field 283:Main article: 280: 277: 237: 234: 232: 229: 213:Wolfgang Pauli 201:fine structure 173:Woldemar Voigt 146:Johannes Stark 141: 138: 83:magnetic field 75:electric field 71:spectral lines 51:electric field 15: 9: 6: 4: 3: 2: 3478: 3467: 3464: 3462: 3459: 3457: 3454: 3452: 3449: 3448: 3446: 3437: 3432: 3426: 3422: 3417: 3415: 3410: 3404: 3399: 3398: 3391: 3389: 3384: 3378: 3374: 3373: 3367: 3365: 3360: 3354: 3350: 3348: 3343: 3339: 3338: 3325: 3321: 3317: 3313: 3309: 3305: 3301: 3297: 3290: 3283: 3276: 3272: 3266: 3264: 3256: 3252: 3246: 3240:p. 336 (1926) 3239: 3235: 3229: 3222: 3218: 3214: 3207: 3198: 3191: 3187: 3181: 3174: 3170: 3164: 3157: 3153: 3147: 3139: 3135: 3131: 3127: 3123: 3119: 3115: 3111: 3104: 3100: 3090: 3087: 3085: 3082: 3080: 3077: 3075: 3072: 3070: 3067: 3065: 3062: 3060: 3059:Zeeman effect 3057: 3056: 3050: 3048: 3038: 3036: 3031: 3027: 3017: 3015: 2997: 2993: 2983: 2969: 2964: 2960: 2954: 2950: 2944: 2941: 2936: 2933: 2925: 2918: 2909: 2906: 2902: 2896: 2892: 2888: 2883: 2880: 2876: 2867: 2862: 2860: 2844: 2833: 2824: 2821: 2816: 2812: 2804: 2796: 2792: 2781: 2776: 2772: 2761: 2757: 2746: 2740: 2737: 2732: 2720: 2714: 2711: 2706: 2695: 2691: 2680: 2675: 2671: 2659: 2656: 2652: 2649: 2644: 2640: 2637: 2634: 2629: 2626: 2622: 2614:α defined by 2613: 2595: 2591: 2585: 2581: 2575: 2572: 2568: 2562: 2557: 2554: 2551: 2548: 2545: 2541: 2535: 2532: 2527: 2524: 2513: 2504: 2501: 2496: 2492: 2484: 2476: 2472: 2461: 2456: 2452: 2429: 2418: 2412: 2409: 2404: 2392: 2381: 2376: 2353: 2342: 2337: 2333: 2321: 2318: 2314: 2311: 2306: 2302: 2294: 2286: 2282: 2261: 2258: 2250: 2242: 2238: 2234: 2226: 2218: 2214: 2210: 2202: 2194: 2190: 2185: 2182: 2179: 2176: 2173: 2170: 2167: 2164: 2160: 2155: 2150: 2146: 2137: 2129: 2125: 2121: 2116: 2111: 2107: 2098: 2091: 2083: 2073: 2071: 2067: 2062: 2058: 2054: 2050: 2034: 2031: 2028: 2025: 2022: 2019: 2016: 2013: 2010: 2007: 2004: 2001: 1998: 1995: 1992: 1980: 1970: 1965: 1962: 1958: 1951: 1945: 1942: 1939: 1926: 1922: 1917: 1915: 1899: 1879: 1859: 1856: 1853: 1850: 1847: 1844: 1841: 1838: 1828: 1825: 1822: 1812: 1809: 1806: 1803: 1800: 1797: 1794: 1791: 1788: 1768: 1760: 1744: 1724: 1718: 1715: 1712: 1709: 1701: 1698: 1695: 1690: 1687: 1684: 1680: 1676: 1671: 1667: 1658: 1654: 1650: 1631: 1626: 1622: 1610: 1605: 1603: 1596: 1592: 1587: 1574: 1560: 1552: 1549: 1541: 1536: 1532: 1511: 1506: 1502: 1495: 1487: 1484: 1476: 1469: 1438: 1422: 1419: 1416: 1413: 1410: 1407: 1404: 1401: 1398: 1395: 1391: 1383: 1378: 1374: 1353: 1348: 1344: 1337: 1329: 1326: 1318: 1313: 1309: 1286: 1275: 1270: 1266: 1259: 1254: 1251: 1215: 1211: 1207: 1189: 1184: 1180: 1176: 1173: 1170: 1165: 1160: 1156: 1147: 1137: 1135: 1119: 1111: 1103: 1100: 1083: 1067: 1065: 1061: 1057: 1041: 1038: 1035: 1026: 1024: 1023:dipole moment 1020: 1003: 982: 962: 954: 946: 932: 929: 926: 921: 917: 911: 907: 901: 896: 893: 890: 886: 882: 868: 865: 862: 859: 854: 850: 844: 840: 825: 814: 808: 804: 798: 793: 790: 787: 783: 779: 776: 771: 767: 752: 741: 726: 723: 706: 673: 648: 644: 636: 632: 623: 614: 606: 603: 598: 594: 573: 568: 564: 558: 554: 548: 543: 540: 537: 533: 529: 515: 512: 498: 490: 486: 470: 460: 456: 440: 426: 415: 411: 394: 362: 355: 304: 296: 292: 286: 276: 274: 271:(also called 270: 266: 262: 258: 254: 249: 247: 242: 228: 226: 221: 218: 214: 210: 206: 202: 198: 194: 190: 186: 182: 177: 174: 170: 166: 165:Zeeman effect 161: 159: 155: 151: 147: 134: 130: 127:in classical 126: 125:closed orbits 122: 118: 114: 110: 105: 101: 99: 94: 92: 88: 84: 80: 79:Zeeman effect 76: 72: 68: 60: 56: 52: 48: 44: 40: 38: 33: 30: 26: 21: 3466:Spectroscopy 3435: 3420: 3413: 3396: 3387: 3371: 3363: 3345: 3299: 3295: 3282: 3274: 3270: 3254: 3250: 3245: 3237: 3233: 3228: 3220: 3216: 3211: 3206: 3197: 3189: 3185: 3180: 3172: 3168: 3163: 3155: 3151: 3146: 3113: 3109: 3103: 3044: 3041:Applications 3035:Rydberg atom 3023: 3013: 2984: 2863: 2858: 2082:eigenproblem 2079: 2076:Second order 2060: 2056: 2052: 2048: 1918: 1913: 1758: 1656: 1652: 1608: 1606: 1594: 1588: 1436: 1213: 1209: 1205: 1145: 1143: 1073: 1060:bound states 1027: 671: 288: 250: 243: 239: 222: 185:Paul Epstein 178: 162: 153: 143: 121:bifurcations 116: 112: 97: 95: 67:Stark effect 66: 64: 42: 41:consists of 36: 31: 24: 2857:The energy 1925:rigid rotor 1140:First order 485:classically 131:leading to 34:= 0. Each 3445:Categories 3232:W. Pauli, 3167:J. Stark, 3150:W. Voigt, 3095:References 3030:resonances 1021:) and the 257:Bohr model 3316:0947-6539 2994:α 2951:α 2937:− 2915:⟹ 2903:δ 2893:α 2889:≡ 2877:α 2813:− 2787:⟩ 2773:ψ 2758:μ 2733:ψ 2729:⟨ 2726:⟩ 2707:ψ 2692:μ 2672:ψ 2668:⟨ 2657:≠ 2645:∑ 2638:− 2623:α 2569:α 2542:∑ 2528:− 2525:≡ 2493:− 2467:⟩ 2453:ψ 2405:ψ 2401:⟨ 2398:⟩ 2386:′ 2377:ψ 2334:ψ 2330:⟨ 2319:≠ 2307:∑ 2262:… 2235:≤ 2183:… 2147:ψ 2108:ψ 2029:… 2014:− 2005:− 1981:∗ 1949:⟩ 1900:ℓ 1880:ℓ 1854:⊕ 1848:⊕ 1842:⊕ 1818:⟹ 1769:ℓ 1745:ℓ 1713:ℓ 1699:− 1685:ℓ 1681:∑ 1623:ψ 1572:⟩ 1568:μ 1564:⟨ 1561:⋅ 1553:− 1547:⟩ 1533:ψ 1523:μ 1503:ψ 1499:⟨ 1496:⋅ 1488:− 1448:μ 1414:… 1389:⟩ 1375:ψ 1365:μ 1345:ψ 1341:⟨ 1338:⋅ 1330:− 1324:⟩ 1310:ψ 1267:ψ 1263:⟨ 1181:ψ 1174:… 1157:ψ 1116:μ 1112:⋅ 1104:− 1004:μ 955:⋅ 951:μ 947:− 933:ϕ 908:μ 887:∑ 883:− 869:ϕ 863:≡ 826:ρ 815:∫ 784:∑ 780:− 753:ρ 742:∫ 727:ϕ 724:≈ 629:∂ 624:ϕ 621:∂ 607:− 604:≡ 534:∑ 530:− 516:ϕ 513:≈ 499:ϕ 441:ϕ 427:ρ 416:∫ 363:ϕ 305:ρ 231:Mechanism 211:) was by 115:= 15 for 27:= 15 for 3344:(1987). 3324:28833695 3213:Spectrum 3053:See also 3020:Problems 2825:′ 2741:′ 2715:′ 2653:′ 2505:′ 2413:′ 2315:′ 2047:with 2(2 1834:contains 1781:states, 236:Overview 193:hydrogen 107:Lithium 3138:9912027 3118:Bibcode 140:History 109:Rydberg 91:plasmas 3427:  3405:  3379:  3355:  3322:  3314:  3136:  3014:always 1737:where 1602:parity 1591:tensor 1019:moment 975:where 291:charge 3292:(PDF) 133:chaos 39:level 3425:ISBN 3403:ISBN 3377:ISBN 3353:ISBN 3320:PMID 3312:ISSN 3134:PMID 2211:< 1988:with 995:and 386:is 187:and 65:The 45:− 1 3304:doi 3255:385 3156:309 3126:doi 3037:). 3012:is 1655:is 1612:int 1598:int 1435:If 1056:ion 207:'s 123:of 3447:: 3318:. 3310:. 3300:23 3298:. 3294:. 3275:28 3262:^ 3238:36 3190:50 3173:43 3132:. 3124:. 3114:51 3112:. 2061:MK 1789:16 1461:, 1212:× 265:2p 261:2s 215:. 183:, 135:. 3433:. 3411:. 3385:. 3361:. 3326:. 3306:: 3221:3 3140:. 3128:: 3120:: 2998:0 2970:. 2965:2 2961:F 2955:0 2945:2 2942:1 2934:= 2929:) 2926:2 2923:( 2919:E 2910:j 2907:i 2897:0 2884:j 2881:i 2859:E 2845:. 2837:) 2834:0 2831:( 2822:k 2817:E 2808:) 2805:0 2802:( 2797:k 2793:E 2782:0 2777:k 2768:| 2762:j 2753:| 2747:0 2738:k 2721:0 2712:k 2702:| 2696:i 2687:| 2681:0 2676:k 2660:k 2650:k 2641:2 2635:= 2630:j 2627:i 2596:j 2592:F 2586:i 2582:F 2576:j 2573:i 2563:3 2558:1 2555:= 2552:j 2549:, 2546:i 2536:2 2533:1 2517:) 2514:0 2511:( 2502:k 2497:E 2488:) 2485:0 2482:( 2477:k 2473:E 2462:0 2457:k 2448:| 2441:t 2438:n 2435:i 2430:V 2425:| 2419:0 2410:k 2393:0 2382:k 2372:| 2365:t 2362:n 2359:i 2354:V 2349:| 2343:0 2338:k 2322:k 2312:k 2303:= 2298:) 2295:2 2292:( 2287:k 2283:E 2259:, 2254:) 2251:0 2248:( 2243:2 2239:E 2230:) 2227:0 2224:( 2219:1 2215:E 2206:) 2203:0 2200:( 2195:0 2191:E 2186:, 2180:, 2177:1 2174:, 2171:0 2168:= 2165:k 2161:, 2156:0 2151:k 2141:) 2138:0 2135:( 2130:k 2126:E 2122:= 2117:0 2112:k 2102:) 2099:0 2096:( 2092:H 2057:D 2053:J 2049:J 2035:J 2032:, 2026:, 2023:1 2020:+ 2017:J 2011:, 2008:J 2002:= 1999:K 1996:, 1993:M 1977:) 1971:J 1966:K 1963:M 1959:D 1955:( 1952:= 1946:M 1943:K 1940:J 1936:| 1914:n 1860:. 1857:f 1851:d 1845:p 1839:s 1829:4 1826:= 1823:n 1813:7 1810:+ 1807:5 1804:+ 1801:3 1798:+ 1795:1 1792:= 1759:n 1725:, 1722:) 1719:1 1716:+ 1710:2 1707:( 1702:1 1696:n 1691:0 1688:= 1677:= 1672:2 1668:n 1657:n 1653:n 1632:0 1627:i 1609:V 1595:V 1575:. 1557:F 1550:= 1542:0 1537:1 1528:| 1518:| 1512:0 1507:1 1492:F 1485:= 1480:) 1477:1 1474:( 1470:E 1437:g 1423:. 1420:g 1417:, 1411:, 1408:1 1405:= 1402:l 1399:, 1396:k 1392:, 1384:0 1379:l 1370:| 1360:| 1354:0 1349:k 1334:F 1327:= 1319:0 1314:l 1305:| 1298:t 1295:n 1292:i 1287:V 1282:| 1276:0 1271:k 1260:= 1255:l 1252:k 1248:) 1241:t 1238:n 1235:i 1229:V 1224:( 1214:g 1210:g 1206:g 1190:0 1185:g 1177:, 1171:, 1166:0 1161:1 1146:g 1120:. 1108:F 1101:= 1095:t 1092:n 1089:i 1084:V 1042:0 1039:= 1036:q 983:q 963:, 959:F 944:) 940:0 936:( 930:q 927:= 922:i 918:F 912:i 902:3 897:1 894:= 891:i 880:) 876:0 872:( 866:q 860:r 855:3 851:d 845:i 841:r 837:) 833:r 829:( 820:V 809:i 805:F 799:3 794:1 791:= 788:i 777:r 772:3 768:d 764:) 760:r 756:( 747:V 738:) 734:0 730:( 718:t 715:n 712:i 707:V 684:V 672:0 655:0 649:| 645:) 637:i 633:r 615:( 599:i 595:F 574:, 569:i 565:F 559:i 555:r 549:3 544:1 541:= 538:i 527:) 523:0 519:( 510:) 506:r 502:( 471:. 467:r 461:3 457:d 452:) 448:r 444:( 438:) 434:r 430:( 421:V 412:= 406:t 403:n 400:i 395:V 374:) 370:r 366:( 338:V 316:) 312:r 308:( 117:m 113:n 61:. 43:n 37:n 32:m 25:n

Index


magnetic quantum number
n level
degenerate sublevels
electric field
underlying symmetries
Coulomb potential
spectral lines
electric field
Zeeman effect
magnetic field
pressure broadening
plasmas

Rydberg
bifurcations
closed orbits
dynamical systems
chaos
Johannes Stark
Antonino Lo Surdo
Nobel Prize in Physics
Zeeman effect
Hendrik Lorentz
Woldemar Voigt
("old") quantum theory
Paul Epstein
Karl Schwarzschild
hydrogen
Hendrik Kramers

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

↑