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

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CLs<br />

0.7<br />

0.6<br />

0.5<br />

0.4<br />

0.3<br />

0.2<br />

0.1<br />

0<br />

1 2 3<br />

LHCb<br />

4 5 6<br />

0<br />

-8 -<br />

B(B →→<br />

) [10 ]<br />

0<br />

-8 -<br />

(a) (b)<br />

B(B →→<br />

) [10 ]<br />

s<br />

CLs<br />

0.7<br />

0.6<br />

0.5<br />

0.4<br />

0.3<br />

0.2<br />

0.1<br />

LHCb<br />

0<br />

0.2 0.4 0.6 0.8 1.0 1.2 1.4 1.6 1.8<br />

Figure 1: (a) Observed (solid curve) <strong>and</strong> expected (dashed curve) CLs values as a function of B(B 0 s → µ + µ − ).<br />

The green sha<strong>de</strong>d area contains the ±1σ interval of possible results compatible with the expected value when<br />

only background is observed. The 90 % (95 %) C.L. observed value is i<strong>de</strong>ntified by the solid (dashed) line. (b) the<br />

same for B(B 0 → µ + µ − ).<br />

also shown in the same figure as a green area covering the region of ±1σ of background-only<br />

compatible observations. The uncertainties in the signal <strong>and</strong> background likelihoods <strong>and</strong> normalization<br />

factors are used to compute the uncertainties in the background <strong>and</strong> signal predictions.<br />

The upper limits read:<br />

B(B 0 s → µ + µ − ) < 4.3 (5.6) × 10 −8 at 90 % (95 %) C.L.,<br />

B(B 0 → µ + µ − ) < 1.2 (1.5) × 10 −8 at 90 % (95 %) C.L.,<br />

while the expected values of the limits are B(B 0 s → µ + µ − ) < 5.1 (6.5) × 10 −8 <strong>and</strong> B(B 0 →<br />

µ + µ − ) < 1.4 (1.8) × 10 −8 at 90 % (95 %) C.L. The limits observed are similar to the best<br />

published limits for the B 0 s → µ + µ − <strong>de</strong>cay <strong>and</strong> more restrictive for the B 0 → µ + µ − <strong>de</strong>cay.<br />

References<br />

1. A.J. Buras, arXiv:1012.1447;<br />

E. Gamiz et al, Phys. Rev. D80 (2009) 014503;<br />

A.J. Buras, Phys. Lett. B566 (2003) 115.<br />

2. C. Hamzaoui, M. Pospelov <strong>and</strong> M. Toharia, “Higgs-mediated FCNC in supersymmetric<br />

mo<strong>de</strong>ls with large tan β”, Phys. Rev. D59 (1999) 095005; S.Rai Choudhury <strong>and</strong> N. Gaur,<br />

Phys. Lett. B451 (1999) 86; K.S. Babu <strong>and</strong> C.F. Kolda, Phys. Rev. Lett.84 (2000) 228.<br />

3. V. Abazov et al. [D0 Collaboration], Phys. Lett. B693 (2010) 539.<br />

4. T. Aaltonen et al. [CDF Collaboration], Phys. Rev. Lett.100 (2008) 101802.<br />

5. T. Aaltonen et al. [CDF Collaboration], CDF Public Note 9892.<br />

6. A.A. Alves et al. [LHCb Collaboration], JINST 3 (2008) S08005.<br />

7. R. Aaij et al. [LHCb Collaboration], Phys. Lett. B699 (<strong>2011</strong>), 330.<br />

8. A.L. Read, J. Phys. G28 (2002) 2693;<br />

T. Junk, Nucl. Instrum. Methods A434 (1999) 435.<br />

9. B. A<strong>de</strong>va et al. [LHCb Collaboration], arXiv:0912.4179.<br />

10. D. Karlen, Comp. Phys. 12 (1998) 380.<br />

11. D. Martinez Santos, CERN-THESIS-2010-068.<br />

12. K. Nakamura et al. [Particle Data Group], J. Phys. G37 (2010) 075021.<br />

13. D. Asner et al. [Heavy Flavour Averaging Group], arXiv:1010.1589. Updated values for<br />

fd/fs available at http://www.slac.stanford.edu/xorg/hfag/osc/end 2009/ have been used.<br />

14. R. Louvot, arXiv:0905.4345.<br />

15. E. Lopez Asamar et al., LHCb-PUB-2007-073.

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