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Physical Review D
Volumn 37, Issue 9, 1988, Pages 2564-2569
Radiative and pionic decays of the D/emph> mesons and the magnetic moment of the charmed quark
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[No Author keywords available]
Indexed keywords

EID: 4243961076     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.37.2564     Document Type: Article
Times cited : (51)
References (44)
  • 10
    • 84931555031 scopus 로고    scopus 로고
    • This work contains a detailed treatment of configuration mixing and relativistic effects.
  • 22
    • 84931555030 scopus 로고    scopus 로고
    • talk at 1987 International Symposium on Lepton and Photon Interactions at High Energies, Hamburg, 1987 (unpublished).
    • Hitlin, D.1
  • 26
    • 84931555028 scopus 로고    scopus 로고
    • There is an error in that paper, the term α0 KstarK correctly equals sqrt 3 / 2 giving f barKstarK = 4.4.
  • 27
    • 84931555027 scopus 로고    scopus 로고
    • The only other observed decay of possible relevance is ψ (3685) -> ηcgamma. However, this is a hindered M1 transition and computing the rate involves more assumptions.
  • 30
    • 0001195170 scopus 로고
    • have suggested using an anomalous moment for the transition ψ (3097) -> ηcgamma. Note that in Ref. 6 the computed rate for this transition is too large (and Rγ= case 1 over 25 ), in contrast with their excellent results for (u,d,s) transitions. Multiplying the amplitude of Ref. 6 by λ = 0.50 leads to excellent agreement for the psi decay and improves the ratio Rgamma. The anomalous moment also enters in the rate for ψ -> e+e-. For relative s states one multiplies the expression by ( 2 λ2+ 1 ) / 3. Including this in Ref. 6 leads to excellent agreement with experiment for such states. However, this rate seems difficult to evaluate, so the good agreement obtained here could be model dependent.
    • (1983) Phys. Rev. D , vol.28 , pp. 1692
    • McClary, R.1    Byers, N.2
  • 33
    • 0001281057 scopus 로고
    • parametrize the annihilation cross section in terms of constants F1 and F2 and find that lambda is close to unity. However, F1, F2 could have momentum dependence making their formulas equivalent to those of Ref. 22 and therefore allowing the effects we compute.
    • (1983) Phys. Rev. D , vol.27 , pp. 1196
    • Silverman, D.J.1    Shaw, G.L.2
  • 35
    • 84931555038 scopus 로고    scopus 로고
    • Note that Eq. (12) is somewhat arbitrary. One could replace the exponent -2 by -n, change M to sqrt n / 2 M, and not influence δ R for W < 40 GeV. The use of a larger mass decreases δ R at higher energies: δ R (100 GeV)= 1.7, if n=5.
  • 40
    • 84931555036 scopus 로고    scopus 로고
    • See, e.g., R. Rueckl, CERN report, 1983 (unpublished).

* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.