Flavor Mixing in Weak Interactions pp 361-382 | Cite as
The Experimental Situation in D Meson Decay
Abstract
- 1)
The change of the two QCD couplings f + and f - from their calculated values.2 These coefficients have now been calculated by renormalization group techniques not only in leading log approximations but, recently, in the next-to-leading log order. The next order changes are, in fact, small, reinforcing the correctness of the leading log values (f + ≅ .7, f - ≅ 1.9, for six fermions and a mass scale of ∼2 GeV) which have been in use for several years. Nonetheless, in order to account for the experimental facts within this context, it is necessary to postulate that f - is, in fact, very much larger than f +. Since the two spectator diagrams in D + decay lead to the same final quark state, they can interfere. If f - >> f +, this interference can be destructive, reducing the D + decay rate and lengthening the D + lifetime. Thus, in this picture the D +/D° lifetime difference is ascribed to an increase in the D + lifetime, with the D° and F + lifetimes occurring at values one would estimate by scaling from muon decay by (m μ/m c )5.
- 2)
The second approach attributes the shorter D° lifetime to the importance of additional (W exchange) amplitudes, occurring only in D° decay.3 These are, naively, suppressed by helicity conservation at the light quark vertex. Either through explicit radiation of soft gluons, or through the gluon component of the quark wavefunction, the W exchange diagram is then enhanced. In this picture, the D + lifetime would occur at the “normal” value while the D° lifetime (and perhaps the F + lifetime through similarly enhanced W annihilation graphs) would be shortened. Since the W exchange process leads to I = 1/2 final states in hadronic D° decay, whereas the spectator process produces both I = 1/2 and I = 3/2 final states, reinforcement of I = 1/2 configurations would be indicative of the importance of exchange diagrams.
Keywords
Decay Mode Branching Ratio Dalitz Plot Final State Interaction Semileptonic DecayPreview
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References
- 1.J. Ellis, M. K. Gaillard, and D. V. Nanopoulos, Nucl. Phys. B100: 313 (1975).ADSCrossRefGoogle Scholar
- 2.B. Guberina, S. Nussinov, R. D. Peccei, and R. Rückl, Phys. Lett. 89B: 111 (1979);ADSGoogle Scholar
- Y. Koide, Phys. Rev. D20: 1739 (1979)ADSGoogle Scholar
- K. Jagannathan and V. S. Mathur, Phys. Rev. D21: 3165 (1980)ADSGoogle Scholar
- N. Deshpande, M. Gronau and D. Sutherland, Phys. Lett. 90B: 431 (1980).Google Scholar
- G. Altarelli, G. Curci, G. Martinelli and R. Petrarca, Phys. Lett. 99B: 141 (1981)Google Scholar
- G. Altarelli, G. Curci, G. Martinelli and R. Petrarca, Nucl. Phys. B 187: 461 (1981).ADSCrossRefGoogle Scholar
- 3.M. Bander, D. Silverman and A. Soni, Phys. Rev. Lett. 44: 7 (1980)Google Scholar
- W. Bernreuther, O. Nachtmann and B. Stech, Z. Phys. C4: 257 (1980);Google Scholar
- S. P. Rosen, Phys. Rev. Lett. 44: 4 (1980);ADSCrossRefGoogle Scholar
- H. Fritzsch and P. Minkowski, Phys. Lett. 90B: 455 (1980).Google Scholar
- 4.V. Barger and S. Pakvasa, Phys. Rev. Lett. 43: 812 (1979);ADSCrossRefGoogle Scholar
- H.Fritzsch and P.Minkowski, Nucl.Phys. B171:413(1980)Google Scholar
- I. Bigi, Phys. Lett. 90B: 177 (1980);Google Scholar
- D. Sutherland, Phys. Lett. 90B: 173 (1980);Google Scholar
- L. F. Abbott, P. Sikivie and M. B. Wise, Phys. Rev. D21: 768 (1980);ADSGoogle Scholar
- M. Suzuki, Phys. Rev. Lett. 43: 818 (1979).ADSCrossRefGoogle Scholar
- 5.D. Bernstein et al., SLAC-PUB-3222 (1983), to appear in Nucl. Instrum. and Methods;Google Scholar
- Members of the MARK III Collaboration are R. M. Baltrusaitis, D. Coffman, G. Dubois, J. Hauser, D. G. Hitlin, J. D. Richman, J. J. Russell, and R. H. Schindler, California Institute of Technology; K. O. Bunnell, R. E. Cassell, D. H. Coward, S. Dado, K. F. Einsweiler, L. Moss, R. F. Mozley, A. Odian, J. R. Roehrig, W. Toki, F. Villa, N. Wermes, and D. E. Wisinski, Stanford Linear Accelerator Center; D. E. Dorfan, R. Fabrizio, F. Grancagnolo, R. P. Hamilton, C. A. Heusch, L. Koepke, W. Lockman, R. Partridge, J. Perrier, H. F. Sadrozinski, T. L. Schalk, A. Seiden, and A. Weinstein, University of California at Santa Cruz; J. J. Becker, G. T. Blaylock, B.Eisenstein, G. Gladding, S. A. Plaetzer, A. L. Spadafora, J. J. Thaler, B. Tripsas, A. Wattenberg, and W. J. Wisniewski, University of Illinois, Champaign-Urbana; J. S. Brown, T. H. Burnett, V. Cook, C. Del Papa, A. L. Duncan, P. M. Mockett, A. Nappi, J. C. Sleeman, and H. J. Willutzki, University of Washington, Seattle.Google Scholar
- 6.K. Niu, these Proceedings.Google Scholar
- 7.R. Schindler et al., Phys. Rev. D24: 78 (1981).ADSGoogle Scholar
- 8.W. Bacino et al., Phys. Rev. Lett. 45: 329 (1980).ADSCrossRefGoogle Scholar
- 9.I. Bigi and M. Fukugita, Phys. Lett. 91B: 121 (1980).Google Scholar
- 10.H. J. Lipkin Phys. Rev. Lett. 44: 710 (1980).ADSCrossRefGoogle Scholar
- 11.D. J. Summers et al., Phys. Rev. Lett. 52: 410 (1984).ADSCrossRefGoogle Scholar
- 12.R. Bailey et al., Phys. Lett. 132B: 237 (1983).Google Scholar
- 13.G. Abrams et al., Phys. Rev. Lett. 43: 481 (1979).ADSCrossRefGoogle Scholar
- 14.R. Partridge, Ph.D. Thesis, California Institute of Technology, 1984 (unpublished).Google Scholar