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Photon antibunching

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If the field had a classical stochastic process underlying it, say a positive definite probability distribution for photon number, the variance would have to be greater than or equal to the mean. This can be shown by an application of the Cauchy–Schwarz inequality to the definition of
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This quantity is basically the probability of detecting two simultaneous photons, normalized by the probability of detecting two photons at once for a random photon source. Here and after we assume stationary counting statistics.
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generally refers to a light field with photons more equally spaced than a coherent laser field, a signature being a measured two-time correlation suppressed below that of a coherent laser field. More specifically, it can refer to
1497: 1091: 964: 334: 1309: 1012:. Sub-Poissonian fields violate this, and hence are nonclassical in the sense that there can be no underlying positive definite probability distribution for photon number (or intensity). 318:{\displaystyle V_{n}=\langle \Delta n^{2}\rangle =\langle n^{2}\rangle -\langle n\rangle ^{2}=\left\langle \left(a^{\dagger }a\right)^{2}\right\rangle -\langle a^{\dagger }a\rangle ^{2}.} 465: 588: 122:
Photon detections as a function of time for a) antibunching (e.g. light emitted from a single atom), b) random (e.g. a coherent state, laser beam), and c) bunching (chaotic light). Ď„
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A more general definition for photon antibunching concerns the slope of the correlation function away from zero time delay. It can also be shown by an application of the
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photon statistics, that is a photon number distribution for which the variance is less than the mean. A coherent state, as output by a laser far above threshold, has
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H. J. Carmichael and D. F. Walls, A Quantum-Mechanical Master Equation Treatment of the Dynamical Stark Effect, J. Phys. B: Atom. Mol. Phys. 9, 1199 (1976).
1075:. An experiment with more precision that did not require subtraction of a background count rate was done for a single atom in an ion trap by Walther et al. 1651: 1424: 1311:. Hence a rise in the second order intensity correlation function at early times is also nonclassical. This initial rise is photon antibunching. 1750:
Nogueira, W. A. T.; Walborn, S. P.; P\'adua, S.; Monken, C. H. (30 April 2001). "Experimental Observation of Spatial Antibunching of Photons".
1231:{\displaystyle g^{(2)}(\tau )={{\langle a^{\dagger }(0)a^{\dagger }(\tau )a(\tau )a(0)\rangle } \over {\langle a^{\dagger }a\rangle ^{2}}}.} 915: 86: 449:{\displaystyle V_{n}=\langle {(a^{\dagger }})^{2}a^{2}\rangle +\langle a^{\dagger }a\rangle -\langle a^{\dagger }a\rangle ^{2}.} 58: 1572: 1241:
It can be shown that for a classical positive definite probability distribution to exist (i.e. for the field to be classical)
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Nogueira, W. A. T.; Walborn, S. P.; P\'adua, S.; Monken, C. H. (30 January 2004). "Generation of a Two-Photon Singlet Beam".
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https://web.archive.org/web/20110615173635/http://www.ucd.ie/speclab/UCDSOPAMS/peoplehtml/quantumoptics2006/lecture5.pdf
105: 72: 1244: 568:{\displaystyle V_{n}-\langle n\rangle =\langle (a^{\dagger })^{2}a^{2}\rangle -\langle a^{\dagger }a\rangle ^{2}.} 1623: 699:{\displaystyle g^{(2)}(0)={{\langle (a^{\dagger })^{2}a^{2}\rangle } \over {\langle a^{\dagger }a\rangle ^{2}}}.} 54: 1627: 1604: 151: 43: 1599: 1314:
Another way of looking at this time dependent correlation function, inspired by quantum trajectory theory is
1079: 154:, the number of fluctuations is larger than a coherent state; for an antibunched source they are smaller. 1408:{\displaystyle g^{(2)}(\tau )={{\langle a^{\dagger }a\rangle _{C}} \over {\langle a^{\dagger }a\rangle }}} 1505: 1015:
Photon antibunching by this definition was first proposed by Carmichael and Walls and first observed by
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Then we see that sub-Poisson photon statistics, one definition of photon antibunching, is given by
1030: 1890: 1609: 79: 32: 973: 1024: 1540: 882: 821:{\displaystyle {{1} \over {(\langle n\rangle )^{2}}}(V_{n}-\langle n\rangle )=g^{(2)}(0)-1.} 1830: 1769: 1716: 1672: 143: 139: 8: 1589: 1083: 579: 1834: 1773: 1720: 1707:
Zou, X T; Mandel, L (1990). "Photon-antibunching and sub-Poissonian photon statistics".
1676: 1854: 1820: 1793: 1759: 906: 1846: 1785: 1732: 1858: 1797: 1838: 1777: 1724: 1680: 147: 1842: 1492:{\displaystyle \langle O\rangle _{C}\equiv \langle \Psi _{C}|O|\Psi _{C}\rangle .} 1781: 1684: 1020: 1016: 135: 1884: 1728: 1850: 1789: 126:
is the coherence time (the time scale of photon or intensity fluctuations).
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Spatial antibunching has been observed in photon pairs produced by
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is the state conditioned on previous detection of a photon at time
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statistics and yields bunched photon spacing. In the thermal
959:{\displaystyle Q\equiv {\frac {V_{n}}{\langle n\rangle }}-1.} 1543: 1508: 1427: 1323: 1247: 1094: 1033: 976: 918: 885: 837: 722: 591: 468: 337: 171: 328:
Using commutation relations, this can be written as
142:statistics yielding random photon spacing; while a 46:. Unsourced material may be challenged and removed. 1555: 1529: 1491: 1407: 1303: 1230: 1067: 1004: 958: 897: 871: 820: 698: 567: 448: 317: 162:The variance of the photon number distribution is 1882: 879:. We can equivalently express antibunching by 1304:{\displaystyle g^{(2)}(\tau )\leq g^{(2)}(0)} 1524: 1483: 1447: 1435: 1428: 1399: 1383: 1372: 1355: 1213: 1196: 1191: 1126: 944: 938: 778: 772: 740: 734: 681: 664: 659: 623: 553: 536: 530: 494: 488: 482: 434: 417: 411: 395: 389: 351: 303: 286: 233: 226: 220: 207: 201: 185: 1824: 1763: 1706: 106:Learn how and when to remove this message 117: 1663:Paul, H (1982). "Photon antibunching". 1883: 1573:spontaneous parametric down-conversion 1662: 1585:Correlation does not imply causation 582:(for zero delay time) is defined as 44:adding citations to reliable sources 15: 1877:(Becker & Hickl GmbH, web page) 13: 1530:{\displaystyle |\Psi _{C}\rangle } 1515: 1474: 1451: 188: 14: 1902: 1868: 1650:Anti-bunching and Entanglement - 1082:to the time dependent intensity 20: 872:{\displaystyle g^{(2)}(0)<1} 31:needs additional citations for 1804: 1743: 1700: 1691: 1656: 1644: 1628:GNU Free Documentation License 1605:Hanbury Brown and Twiss effect 1566: 1510: 1469: 1461: 1346: 1340: 1335: 1329: 1298: 1292: 1287: 1281: 1270: 1264: 1259: 1253: 1188: 1182: 1176: 1170: 1164: 1158: 1145: 1139: 1117: 1111: 1106: 1100: 1056: 1050: 1045: 1039: 999: 993: 988: 982: 860: 854: 849: 843: 809: 803: 798: 792: 781: 756: 744: 731: 640: 626: 614: 608: 603: 597: 511: 497: 370: 355: 157: 1: 1843:10.1103/PhysRevLett.92.043602 1638: 1068:{\displaystyle g^{(2)}(0)=0} 7: 1782:10.1103/PhysRevLett.86.4009 1622:Article based on text from 1578: 578:The second-order intensity 10: 1907: 1685:10.1103/RevModPhys.54.1061 1615: 1005:{\displaystyle g^{(2)}(0)} 1665:Reviews of Modern Physics 1080:Cauchy–Schwarz inequality 1729:10.1103/PhysRevA.41.475 1626:, reproduced under the 1610:Squeezed coherent state 1556:{\displaystyle \tau =0} 459:This can be written as 1557: 1531: 1493: 1409: 1305: 1232: 1069: 1025:resonance fluorescence 1006: 960: 899: 898:{\displaystyle Q<0} 873: 822: 700: 569: 450: 319: 127: 1600:Hong–Ou–Mandel effect 1558: 1532: 1494: 1410: 1306: 1233: 1070: 1007: 961: 900: 874: 823: 701: 570: 451: 320: 121: 55:"Photon antibunching" 1541: 1506: 1425: 1321: 1245: 1092: 1084:correlation function 1031: 974: 916: 883: 835: 720: 589: 580:correlation function 466: 335: 169: 40:improve this article 1875:Photon antibunching 1835:2004PhRvL..92d3602N 1774:2001PhRvL..86.4009N 1721:1990PhRvA..41..475Z 1677:1982RvMP...54.1061P 1632:Photon Antibunching 1590:Degree of coherence 131:Photon antibunching 1553: 1527: 1489: 1405: 1301: 1228: 1065: 1023:, and Dagenais in 1002: 956: 907:Mandel Q parameter 895: 869: 818: 696: 565: 446: 315: 128: 1758:(18): 4009–4012. 1634: 1403: 1223: 948: 754: 691: 116: 115: 108: 90: 1898: 1863: 1862: 1828: 1826:quant-ph/0503117 1808: 1802: 1801: 1767: 1765:quant-ph/0206039 1747: 1741: 1740: 1704: 1698: 1695: 1689: 1688: 1671:(4): 1061–1102. 1660: 1654: 1648: 1621: 1562: 1560: 1559: 1554: 1536: 1534: 1533: 1528: 1523: 1522: 1513: 1498: 1496: 1495: 1490: 1482: 1481: 1472: 1464: 1459: 1458: 1443: 1442: 1414: 1412: 1411: 1406: 1404: 1402: 1395: 1394: 1381: 1380: 1379: 1367: 1366: 1353: 1339: 1338: 1310: 1308: 1307: 1302: 1291: 1290: 1263: 1262: 1237: 1235: 1234: 1229: 1224: 1222: 1221: 1220: 1208: 1207: 1194: 1157: 1156: 1138: 1137: 1124: 1110: 1109: 1074: 1072: 1071: 1066: 1049: 1048: 1011: 1009: 1008: 1003: 992: 991: 965: 963: 962: 957: 949: 947: 936: 935: 926: 904: 902: 901: 896: 878: 876: 875: 870: 853: 852: 827: 825: 824: 819: 802: 801: 768: 767: 755: 753: 752: 751: 729: 724: 705: 703: 702: 697: 692: 690: 689: 688: 676: 675: 662: 658: 657: 648: 647: 638: 637: 621: 607: 606: 574: 572: 571: 566: 561: 560: 548: 547: 529: 528: 519: 518: 509: 508: 478: 477: 455: 453: 452: 447: 442: 441: 429: 428: 407: 406: 388: 387: 378: 377: 368: 367: 366: 347: 346: 324: 322: 321: 316: 311: 310: 298: 297: 282: 278: 277: 272: 268: 264: 263: 241: 240: 219: 218: 200: 199: 181: 180: 148:super-Poissonian 111: 104: 100: 97: 91: 89: 48: 24: 16: 1906: 1905: 1901: 1900: 1899: 1897: 1896: 1895: 1881: 1880: 1871: 1866: 1813:Phys. Rev. Lett 1809: 1805: 1752:Phys. Rev. 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Rev. A 1708: 1702: 1693: 1668: 1664: 1658: 1646: 1570: 1501: 1417: 1313: 1240: 1077: 1014: 968: 830: 712: 708: 577: 458: 327: 161: 130: 129: 102: 93: 83: 76: 69: 62: 50: 38:Please help 33:verification 30: 1567:Experiments 158:Explanation 1639:References 1595:Fock state 905:where the 146:field has 140:Poissonian 66:newspapers 1545:τ 1525:⟩ 1516:Ψ 1484:⟩ 1475:Ψ 1452:Ψ 1448:⟨ 1445:≡ 1436:⟩ 1429:⟨ 1400:⟩ 1392:† 1384:⟨ 1373:⟩ 1364:† 1356:⟨ 1344:τ 1274:≤ 1268:τ 1214:⟩ 1205:† 1197:⟨ 1192:⟩ 1174:τ 1162:τ 1154:† 1135:† 1127:⟨ 1115:τ 951:− 945:⟩ 939:⟨ 923:≡ 813:− 779:⟩ 773:⟨ 770:− 741:⟩ 735:⟨ 682:⟩ 673:† 665:⟨ 660:⟩ 635:† 624:⟨ 554:⟩ 545:† 537:⟨ 534:− 531:⟩ 506:† 495:⟨ 489:⟩ 483:⟨ 480:− 435:⟩ 426:† 418:⟨ 415:− 412:⟩ 404:† 396:⟨ 390:⟩ 364:† 352:⟨ 304:⟩ 295:† 287:⟨ 284:− 261:† 234:⟩ 227:⟨ 224:− 221:⟩ 208:⟨ 202:⟩ 189:Δ 186:⟨ 1885:Category 1859:25022990 1851:14995372 1798:25655506 1790:11328082 1579:See also 280:⟩ 247:⟨ 96:May 2008 1831:Bibcode 1770:Bibcode 1737:9902890 1717:Bibcode 1673:Bibcode 1616:Sources 80:scholar 1857:  1849:  1796:  1788:  1735:  1630:: see 1418:where 1021:Mandel 1017:Kimble 82:  75:  68:  61:  53:  1855:S2CID 1821:arXiv 1794:S2CID 1760:arXiv 1624:Qwiki 1502:with 87:JSTOR 73:books 1847:PMID 1786:PMID 1733:PMID 890:< 864:< 59:news 1839:doi 1778:doi 1725:doi 1681:doi 1575:. 42:by 1887:: 1853:. 1845:. 1837:. 1829:. 1817:92 1815:. 1792:. 1784:. 1776:. 1768:. 1756:86 1754:. 1731:. 1723:. 1713:41 1711:. 1679:. 1669:54 1667:. 1563:. 1019:, 954:1. 816:1. 1861:. 1841:: 1833:: 1823:: 1800:. 1780:: 1772:: 1762:: 1739:. 1727:: 1719:: 1687:. 1683:: 1675:: 1551:0 1548:= 1520:C 1511:| 1487:. 1479:C 1470:| 1466:O 1462:| 1456:C 1440:C 1432:O 1397:a 1388:a 1377:C 1369:a 1360:a 1350:= 1347:) 1341:( 1336:) 1333:2 1330:( 1326:g 1299:) 1296:0 1293:( 1288:) 1285:2 1282:( 1278:g 1271:) 1265:( 1260:) 1257:2 1254:( 1250:g 1226:. 1218:2 1210:a 1201:a 1189:) 1186:0 1183:( 1180:a 1177:) 1171:( 1168:a 1165:) 1159:( 1150:a 1146:) 1143:0 1140:( 1131:a 1121:= 1118:) 1112:( 1107:) 1104:2 1101:( 1097:g 1063:0 1060:= 1057:) 1054:0 1051:( 1046:) 1043:2 1040:( 1036:g 1000:) 997:0 994:( 989:) 986:2 983:( 979:g 942:n 933:n 929:V 920:Q 893:0 887:Q 867:1 861:) 858:0 855:( 850:) 847:2 844:( 840:g 810:) 807:0 804:( 799:) 796:2 793:( 789:g 785:= 782:) 776:n 765:n 761:V 757:( 749:2 745:) 738:n 732:( 727:1 694:. 686:2 678:a 669:a 655:2 651:a 645:2 641:) 631:a 627:( 618:= 615:) 612:0 609:( 604:) 601:2 598:( 594:g 563:. 558:2 550:a 541:a 526:2 522:a 516:2 512:) 502:a 498:( 492:= 486:n 475:n 471:V 444:. 439:2 431:a 422:a 409:a 400:a 393:+ 385:2 381:a 375:2 371:) 360:a 356:( 349:= 344:n 340:V 313:. 308:2 300:a 291:a 275:2 270:) 266:a 257:a 252:( 243:= 238:2 230:n 216:2 212:n 205:= 197:2 193:n 183:= 178:n 174:V 124:c 109:) 103:( 98:) 94:( 84:· 77:· 70:· 63:· 36:.

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"Photon antibunching"
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sub-Poissonian
Poissonian
thermal light
super-Poissonian
(bunched) case
correlation function
Mandel Q parameter
Kimble
Mandel
resonance fluorescence
Cauchy–Schwarz inequality
correlation function
spontaneous parametric down-conversion
Correlation does not imply causation
Degree of coherence
Fock state
Hong–Ou–Mandel effect
Hanbury Brown and Twiss effect

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