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2011 QCD and High Energy Interactions - Rencontres de Moriond ...

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9<br />

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+<br />

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CDF exclusion at 95% C.L.<br />

SM<br />

5σ<br />

NP discovery (bound)<br />

5σ<br />

NP discovery (N ∈[1.2,1.4])<br />

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Luminosity [ fb ]<br />

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SM<br />

4<br />

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5σ<br />

NP discovery (bound)<br />

5σ<br />

NP discovery (N ∈[1.2,1.4])<br />

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LHCb-PUB-2009-029 ( ∞ statistics)<br />

New method ( ∞ statistics)<br />

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Figure 2: Illustration of the LHCb NP reach in B 0 s → µ + µ − resulting from the strategy proposed in Ref. [13].<br />

LHCb, the <strong>de</strong>cays must be robust with respect to the impact of NP, <strong>and</strong> the ratio of their BRs<br />

must be theoretically well un<strong>de</strong>rstood. These requirements are satisfied by the U-spin-related<br />

¯B 0 s → D + s π − <strong>and</strong> ¯ B 0 d → D+ K − <strong>de</strong>cays. In these channels, “factorization” of hadronic matrix<br />

elements is expected to work very well, <strong>and</strong> the theoretical precision is limited by non-factorizable<br />

U-spin-breaking effects, leading to an uncertainty at the few-percent level. These features can<br />

also be tested through experimental data, supporting this picture. 14 The NP discovery potential<br />

in B 0 s → µ + µ − at LHCb resulting from this method is illustrated in Fig. 2, which shows the<br />

smallest value of BR(B 0 s → µ + µ − ) allowing the <strong>de</strong>tection of a 5σ <strong>de</strong>viation from the SM as a<br />

function of the luminosity at LHCb (at the nominal beam energy of 14 TeV). 13<br />

LHCb has reported the first results for fs/fd from this strategy at this conference, 15 yielding<br />

fs/fd = 0.245 ± 0.017|stat ± 0.018|sys ± 0.018|theo. This is an average over the data for the<br />

¯B 0 s → D + s π − , ¯ B 0 d → D+ K − <strong>and</strong> ¯ B 0 s → D + s π − , ¯ B 0 d → D+ π − systems, where the latter offers a<br />

variant of the method for extracting fs/fd. 14<br />

3 Concluding Remarks<br />

We are moving towards new frontiers in B physics. There are good chances that these studies<br />

will reveal first footprints of NP at the LHC. Exciting years are ahead of us!<br />

References<br />

1. A. J. Buras, PoS E PS-HEP2009 (2009) 024 [arXiv:0910.1032 [hep-ph]].<br />

2. A. S. Dighe, I. Dunietz <strong>and</strong> R. Fleischer, Eur. Phys. J. C 6 (1999) 647.<br />

3. I. Dunietz, R. Fleischer <strong>and</strong> U. Nierste, Phys. Rev. D 63 (2001) 114015.<br />

4. LHCb Collaboration, LHCb-CONF-<strong>2011</strong>-002.<br />

5. S. Faller, R. Fleischer <strong>and</strong> T. Mannel, Phys. Rev. D 79 (2009) 014005.<br />

6. R. Fleischer, Eur. Phys. J. C 10 (1999) 299.<br />

7. K. De Bruyn, R. Fleischer <strong>and</strong> P. Koppenburg, Eur. Phys. J. C 70 (2010) 1025.<br />

8. R. Fleischer, Phys. Lett. B 459 (1999) 306; Eur. Phys. J. C 52 (2007) 267.<br />

9. B. A<strong>de</strong>va et al. [LHCb Collaboration], LHCb-PUB-2009-029 [arXiv:0912.4179 [hep-ex]].<br />

10. R. Fleischer <strong>and</strong> R. Knegjens, Eur. Phys. J. C 71 (<strong>2011</strong>) 1532.<br />

11. LHCb Collaboration, LHCb-CONF-<strong>2011</strong>-018.<br />

12. R. Aaij et al. [LHCb Collaboration], Phys. Lett. B 699 (<strong>2011</strong>) 330.<br />

13. R. Fleischer, N. Serra <strong>and</strong> N. Tuning, Phys. Rev. D 82 (2010) 034038.<br />

14. R. Fleischer, N. Serra <strong>and</strong> N. Tuning, Phys. Rev. D 83 (<strong>2011</strong>) 014017.<br />

15. LHCb Collaboration, LHCb-CONF-<strong>2011</strong>-013.

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