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Mandel Q parameter

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459: 63: 22: 111: 200: 454:{\displaystyle Q={\frac {\left\langle (\Delta {\hat {n}})^{2}\right\rangle -\langle {\hat {n}}\rangle }{\langle {\hat {n}}\rangle }}={\frac {\langle {\hat {n}}^{(2)}\rangle -\langle {\hat {n}}\rangle ^{2}}{\langle {\hat {n}}\rangle }}-1=\langle {\hat {n}}\rangle \left(g^{(2)}(0)-1\right)} 646: 194:. It is a convenient way to characterize non-classical states with negative values indicating a sub-Poissonian statistics, which have no classical analog. It is defined as the normalized variance of the boson distribution: 552: 763: 711: 491: 528: 678: 795: 542:
Negative values of Q corresponds to state which variance of photon number is less than the mean (equivalent to sub-Poissonian statistics). In this case, the
129: 641:{\displaystyle -1\leq Q<0\Leftrightarrow 0\leq \langle (\Delta {\hat {n}})^{2}\rangle \leq \langle {\hat {n}}\rangle } 35: 165: 147: 49: 730: 736: 81: 960: 85: 41: 687: 467: 500: 125: 878: 823: 722: 183: 654: 8: 774: 726: 77: 882: 827: 684:(Fock states), which by definition have a well-defined number of photons and for which 896: 847: 839: 886: 831: 729:. The resulting occupation distribution of the number state is characterized by a 814:
Mandel, L. (1979). "Sub-Poissonian photon statistics in resonance fluorescence".
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distribution cannot be interpreted as a classical probability distribution.
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is the normalized second-order correlation function as defined by
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measures the departure of the occupation number distribution from
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have a Poissonian photon-number statistics for which
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may be too technical for most readers to understand
789: 757: 705: 672: 640: 522: 485: 453: 72:may lack focus or may be about more than one topic 952: 76:Please help improve this article, possibly by 752: 746: 635: 620: 614: 583: 407: 392: 377: 362: 351: 335: 329: 301: 289: 274: 269: 254: 50:Learn how and when to remove these messages 858: 890: 867:"The Quantum Theory of Optical Coherence" 807: 166:Learn how and when to remove this message 148:Learn how and when to remove this message 132:, without removing the technical details. 864: 953: 813: 537: 130:make it understandable to non-experts 938:Optical Coherence and Quantum Optics 915:Optical Coherence and Quantum Optics 104: 80:the article and/or by introducing a 56: 15: 758:{\displaystyle Q=\langle n\rangle } 13: 924: 691: 589: 221: 14: 972: 31:This article has multiple issues. 725:, the phase-space functional is 109: 61: 20: 84:, or discuss this issue on the 39:or discuss these issues on the 907: 629: 605: 598: 586: 574: 515: 509: 477: 437: 431: 426: 420: 401: 371: 344: 324: 318: 311: 283: 263: 237: 230: 218: 1: 800: 7: 945:The Quantum Theory of Light 716: 10: 977: 913:Mandel, L., and Wolf, E., 706:{\displaystyle \Delta n=0} 486:{\displaystyle {\hat {n}}} 892:10.1103/PhysRev.130.2529 865:Glauber, Roy J. (1963). 731:Bose–Einstein statistics 523:{\displaystyle g^{(2)}} 186:. It was introduced in 791: 759: 707: 674: 642: 524: 495:photon number operator 487: 455: 792: 760: 708: 675: 643: 525: 488: 456: 184:Poissonian statistics 775: 737: 723:black-body radiation 688: 682:photon number states 673:{\displaystyle Q=-1} 655: 651:The minimal value 553: 501: 468: 201: 883:1963PhRv..130.2529G 836:10.1364/OL.4.000205 828:1979OptL....4..205M 790:{\displaystyle Q=0} 538:Non-classical value 82:disambiguation page 787: 755: 703: 670: 638: 520: 483: 451: 180:Mandel Q parameter 632: 601: 480: 404: 381: 374: 347: 314: 293: 286: 266: 233: 176: 175: 168: 158: 157: 150: 103: 102: 54: 968: 940:(Cambridge 1995) 918: 917:(Cambridge 1995) 911: 905: 904: 894: 877:(6): 2529–2539. 862: 856: 855: 811: 796: 794: 793: 788: 764: 762: 761: 756: 712: 710: 709: 704: 680:is obtained for 679: 677: 676: 671: 647: 645: 644: 639: 634: 633: 625: 613: 612: 603: 602: 594: 529: 527: 526: 521: 519: 518: 492: 490: 489: 484: 482: 481: 473: 460: 458: 457: 452: 450: 446: 430: 429: 406: 405: 397: 382: 380: 376: 375: 367: 360: 359: 358: 349: 348: 340: 328: 327: 316: 315: 307: 299: 294: 292: 288: 287: 279: 272: 268: 267: 259: 250: 246: 245: 244: 235: 234: 226: 211: 171: 164: 153: 146: 142: 139: 133: 113: 112: 105: 98: 95: 89: 65: 64: 57: 46: 24: 23: 16: 976: 975: 971: 970: 969: 967: 966: 965: 951: 950: 927: 925:Further reading 922: 921: 912: 908: 871:Physical Review 863: 859: 812: 808: 803: 776: 773: 772: 769:Coherent states 738: 735: 734: 719: 689: 686: 685: 656: 653: 652: 624: 623: 608: 604: 593: 592: 554: 551: 550: 540: 508: 504: 502: 499: 498: 472: 471: 469: 466: 465: 419: 415: 414: 410: 396: 395: 366: 365: 361: 354: 350: 339: 338: 317: 306: 305: 304: 300: 298: 278: 277: 273: 258: 257: 240: 236: 225: 224: 217: 213: 212: 210: 202: 199: 198: 172: 161: 160: 159: 154: 143: 137: 134: 126:help improve it 123: 114: 110: 99: 93: 90: 75: 66: 62: 25: 21: 12: 11: 5: 974: 964: 963: 961:Quantum optics 949: 948: 941: 926: 923: 920: 919: 906: 857: 816:Optics Letters 805: 804: 802: 799: 786: 783: 780: 754: 751: 748: 745: 742: 718: 715: 702: 699: 696: 693: 669: 666: 663: 660: 649: 648: 637: 631: 628: 622: 619: 616: 611: 607: 600: 597: 591: 588: 585: 582: 579: 576: 573: 570: 567: 564: 561: 558: 539: 536: 517: 514: 511: 507: 479: 476: 462: 461: 449: 445: 442: 439: 436: 433: 428: 425: 422: 418: 413: 409: 403: 400: 394: 391: 388: 385: 379: 373: 370: 364: 357: 353: 346: 343: 337: 334: 331: 326: 323: 320: 313: 310: 303: 297: 291: 285: 282: 276: 271: 265: 262: 256: 253: 249: 243: 239: 232: 229: 223: 220: 216: 209: 206: 192:Leonard Mandel 188:quantum optics 174: 173: 156: 155: 117: 115: 108: 101: 100: 69: 67: 60: 55: 29: 28: 26: 19: 9: 6: 4: 3: 2: 973: 962: 959: 958: 956: 947:(Oxford 2010) 946: 942: 939: 936: 932: 929: 928: 916: 910: 902: 898: 893: 888: 884: 880: 876: 872: 868: 861: 853: 849: 845: 841: 837: 833: 829: 825: 821: 817: 810: 806: 798: 784: 781: 778: 770: 766: 749: 743: 740: 732: 728: 724: 714: 700: 697: 694: 683: 667: 664: 661: 658: 626: 617: 609: 595: 580: 577: 571: 568: 565: 562: 559: 556: 549: 548: 547: 545: 535: 533: 512: 505: 496: 474: 447: 443: 440: 434: 423: 416: 411: 398: 389: 386: 383: 368: 355: 341: 332: 321: 308: 295: 280: 260: 251: 247: 241: 227: 214: 207: 204: 197: 196: 195: 193: 189: 185: 181: 170: 167: 152: 149: 141: 131: 127: 121: 118:This article 116: 107: 106: 97: 87: 83: 79: 73: 70:This article 68: 59: 58: 53: 51: 44: 43: 38: 37: 32: 27: 18: 17: 944: 937: 914: 909: 874: 870: 860: 822:(7): 205–7. 819: 815: 809: 767: 720: 650: 541: 463: 179: 177: 162: 144: 135: 119: 91: 71: 47: 40: 34: 33:Please help 30: 544:phase space 943:R. Loudon 801:References 733:for which 138:April 2014 94:April 2014 36:improve it 931:L. Mandel 901:0031-899X 844:0146-9592 753:⟩ 747:⟨ 692:Δ 665:− 636:⟩ 630:^ 621:⟨ 618:≤ 615:⟩ 599:^ 590:Δ 584:⟨ 581:≤ 575:⇔ 563:≤ 557:− 478:^ 441:− 408:⟩ 402:^ 393:⟨ 384:− 378:⟩ 372:^ 363:⟨ 352:⟩ 345:^ 336:⟨ 333:− 330:⟩ 312:^ 302:⟨ 290:⟩ 284:^ 275:⟨ 270:⟩ 264:^ 255:⟨ 252:− 231:^ 222:Δ 86:talk page 78:splitting 42:talk page 955:Category 852:19687850 727:Gaussian 717:Examples 248:⟩ 215:⟨ 935:E. Wolf 879:Bibcode 824:Bibcode 532:Glauber 493:is the 464:where 124:Please 899:  850:  842:  497:and 897:ISSN 848:PMID 840:ISSN 721:For 569:< 178:The 887:doi 875:130 832:doi 190:by 128:to 957:: 933:, 895:. 885:. 873:. 869:. 846:. 838:. 830:. 818:. 797:. 765:. 713:. 534:. 45:. 903:. 889:: 881:: 854:. 834:: 826:: 820:4 785:0 782:= 779:Q 750:n 744:= 741:Q 701:0 698:= 695:n 668:1 662:= 659:Q 627:n 610:2 606:) 596:n 587:( 578:0 572:0 566:Q 560:1 516:) 513:2 510:( 506:g 475:n 448:) 444:1 438:) 435:0 432:( 427:) 424:2 421:( 417:g 412:( 399:n 390:= 387:1 369:n 356:2 342:n 325:) 322:2 319:( 309:n 296:= 281:n 261:n 242:2 238:) 228:n 219:( 208:= 205:Q 169:) 163:( 151:) 145:( 140:) 136:( 122:. 96:) 92:( 88:. 74:. 52:) 48:(

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Poissonian statistics
quantum optics
Leonard Mandel
photon number operator
Glauber
phase space
photon number states
black-body radiation
Gaussian
Bose–Einstein statistics
Coherent states
Bibcode
1979OptL....4..205M
doi
10.1364/OL.4.000205
ISSN
0146-9592
PMID
19687850
"The Quantum Theory of Optical Coherence"

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