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Volumn 60, Issue 1, 1999, Pages 674-677

Direct measurement of the Wigner function by photon counting

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EID: 0001446129     PISSN: 10502947     EISSN: 10941622     Source Type: Journal    
DOI: 10.1103/PhysRevA.60.674     Document Type: Article
Times cited : (230)

References (16)
  • 1
    • 33745014742 scopus 로고
    • E. P. Wigner, Phys. Rev. 40, 749 (1932). For a review, see
    • (1932) Phys. Rev. , vol.40 , pp. 749
    • Wigner, E.P.1
  • 11
    • 85037225572 scopus 로고    scopus 로고
    • The operating mode of the SPCM results in a certain amount of extraneous pulses originating from dark counts and afterpulsing. The dark count rate of our module is less than 100 (Formula presented). This gives on average (Formula presented) during a single counting interval, which is 30 (Formula presented)s long. The typical afterpulsing probability is (Formula presented). Thus, both of these effects give a negligible contribution to the measured count statistics
    • The operating mode of the SPCM results in a certain amount of extraneous pulses originating from dark counts and afterpulsing. The dark count rate of our module is less than 100 (Formula presented). This gives on average (Formula presented) during a single counting interval, which is 30 (Formula presented)s long. The typical afterpulsing probability is (Formula presented). Thus, both of these effects give a negligible contribution to the measured count statistics.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.