Search for New Physics in B Rare Decays at LHCb

Search for New Physics in Rare Decays at LHCb

Abstract

The LHCb experiment, bolstered up by the -hadrons to be produced yearly in its interaction region, is an excellent place to study rare decays. Flavor-changing neutral currents are forbidden at tree level in the Standard Model. They proceed through loop diagrams and hence are indirectly sensitive to New Physics through the effect of new particles on observable quantities. In this paper, we present preparation studies of the three most promising rare decay analyzes. These aim at the observation of the photon polarization in , the measurement of the angular distribution of the decay, and the search for the yet unobserved decay. The current analysis strategies and the expected sensitivities are presented.

I Introduction

The Standard Model (SM) is successful in explaining almost all observations in particle physics experiments so far. Nevertheless, there are reasons to consider it as a low energy effective limit of a more general theory. In that prospect, observables for processes where the SM contribution is highly suppressed are particularly interesting. Within the SM, flavor-changing neutral current processes are highly suppressed since they are forbidden at tree level and can only proceed via loops diagrams. If New Physics (NP) exists, new particles can also contribute to those processes in the loop diagrams, modifying observable quantities with respect to the SM prediction.

The LHCb detector LHCb () will take advantage of the copious production cross-section expected at LHC LHC (). It is a single-arm forward spectrometer primarily optimized for the study of -violation and rare -hadron decays. The detector is characterized by its precise vertex detector, powerful particle identification capabilities and versatile trigger. Nominally, LHCb will operate at a luminosity , giving of data per year ( seconds). The analyzes presented in this document are applied to Monte Carlo simulated data with a full detector response, including pile-up (multiple collisions in a single bunch crossing) and spill-over (signal coming from particles produced in a previous bunch crossing).

physics requires excellent vertexing capabilities, momentum resolution and particle identification. The study of rare decays demands high background rejection and trigger performance. LHCb was designed to fulfill these requirements. Its Vertex Locator provides an impact parameter resolution of that results in a proper-time resolution of depending on the decay mode. The tracking system yields a momentum resolution of , leading to an invariant mass resolution of and for and , respectively.

Ii Photon Polarization

The branching fraction of this decay,  Wicht08 (), was recently measured by the Belle collaboration and is in agreement with the SM prediction. In the SM the polarization of the photon is precisely predicted. and are allowed transitions under helicity conservation, whereas the crossed transitions are suppressed by a factor . An observable is defined from the transition amplitude ratio as

which is proportional to and very small in the SM. In extensions of the SM, such as the Left-Right Symmetric Model phi_gamma_LR () and the unconstrained MSSM phi_gamma_uMSSM () predict large values for . The measurement of the photon polarization thus provides a null test for the SM.

The photon polarization is measured indirectly, through the time-dependent decay rate Atwood97 (). For the decay of () mesons, the decay rate is:

(1)

Unlike Belle and BaBar analyzes studying asymmetry in  Ushiroda06 (); Aubert08 () decay, we consider an analysis without flavor tagging. Thus, adding the and contributions, the two last terms of Eq. (1) cancel out. Furthermore, since in the SM is expected to be non-zero in the system, the decay rate is sensitive to , through  Muheim08 (). Here represents the decay weak phase, that is approximately zero in the SM. Note that, in the SM, a flavor tagged analysis is not expected to provide a better sensitivity on the measure of , because and .

The main experimental issue is to understand the bias on the lifetime coming from the trigger and offline cuts for the selection. For 2, the expected signal yield is 11000 events with a and a mass resolution of 92 phi_gamma_note1 (). This yield, leads to an expected resolution of 0.1 for the photon polarization observable  phi_gamma_note2 ().

There are others channels considered to probe photon polarization, such as , , and .

Iii Angular Analysis

This decay branching fraction  PDGlive () is in agreement with the SM. Asymmetries related to angular distributions are theoretically well predicted because hadronic uncertainties cancel out in the ratios. The forward-backward asymmetry of , the angle between the and the flight direction in the di-muon rest frame is such an observable. Thus, the shape of as a function of the di-muon invariant mass squared, , is calculated for the SM and for extension models. The zero-crossing point of ( such that ) is a particularly interesting observable. Its SM prediction is  qzero ().

The for this channel was already measured at BaBar, Belle and CDF Babar_Kmumu (); Belle_Kmumu (); CDF_Kmumu () and exhibits some tension with respect to the SM prediction. However, the statistics is very low: the Belle analysis, the most sensitive so far, is based on 230 events only. LHCb expects 7000 events per 2, with .

The challenge for this analysis is the understanding of the biases on angular observables induced by detector and reconstruction effects. It is worth to note that the zero-crossing point value is little sensitive to those biases, making its measurement particularly interesting with early data.

Figure 1: LHCb sensitivity to with the unbinned analysis for 2, with and LHCb experimental error bands, allowing the extraction of the zero-crossing point value . This simulation assumes the SM with .

The LHCb strategy for this decay consists of different methods of increasing sensitivity but also increasing requirements in statistics and acceptance understanding.

The first method is a binned analysis for , combined with a linear fit to extract the zero-crossing point value Kstar_note1 (). With a few hundreds of , this method will already compete with current measurements. With 2, the expected resolution on is and LHCb expects to reach the theoretical precision with 10 of data.

The second method consists of an unbinned analysis for , with no linear assumption around the zero-crossing point Kstar_note2 (). This analysis yields a sensitivity similar to the binned analysis. Figure 1 depicts the expected shape obtained by the unbinned analysis for the SM and with 2.

The next step is a full angular analysis, based on the three angles, which, with the di-muon invariant mass, completely define the decay kinematics Kstar_note3 (). Using the three angle distributions, a number of asymmetries and transversity amplitudes can be computed. The full angular analysis requires a good knowledge of detector acceptance effects and an integrated luminosity of at least 2.

A thorough study has assessed the sensitivity to various observables Egede_theo (), of which some were shown to differ significantly between SM and NP scenarios. An example of the sensitivity achievable with 10 for an observable particularly sensitive to NP is shown in Fig. 2.

Figure 2: observable, defined in Egede_theo (). The SM prediction is shown by the dashed line, with and theoretical uncertainty bands. The dotted line depicts a particular SUSY scenario with positive mass insertion and large gluino mass, with and LHCb experimental error bands (the solid line showing the central value of the toy experiments).

Iv Branching Fraction

Within the SM, the branching ratio is expected to be  Blanke06 (). In the MSSM, this decay receives additional contributions from new particles, e.g. for large values, the ratio of the Higgs vacuum expectation values, the branching ratio is then proportional to to the sixth power, and can be considerably enhanced Ellis07_WMAPMSSM (). The latest upper limit given by the CDF experiment is at CL mumu_CDF ().

Figure 3: Expected CL upper limit on in absence of signal for 8 collisions (left) and at which a discovery (stars) or a evidence (solid blue curve) is expected for 14 collisions (right), as a function of the integrated luminosity. On the exclusion plot, the black curve is the result of the standard analysis, and the red dashed curve is the result of the robust analysis. The background estimate has conservatively been set to its CL upper limit in the exclusion plot, and similarly the dashed curves indicates the 90% CL upper and lower limit in the observation case. The Tevatron limit is calculated by extrapolating the current result to 8 per experiment.

The current LHCb strategy for the decay search mumu-1 () can be summarized as follows. An efficient selection is applied with the goal to remove obvious background with minimal loss of signal events. The analysis relies on three independent variables related to, the di-muon invariant mass, the particle identification of the daughters, and geometrical information from the decay topology. Since the three variables are uncorrelated, they can be calibrated independently. For each event, likelihood values are calculated for each of the three variables, under the signal and background hypotheses. Calibration methods for these values, both for signal and for background, are designed to rely solely on real data. The compatibility of the obtained likelihood distributions is tested against various branching ratio hypotheses, using the CL modified frequentist analysis Cls (). The final result is either a measurement or an upper limit of the branching fraction.

The branching fraction is expressed as:

where is the number of signal events, is the production cross-section, the integrated luminosity, the probability of a quark to hadronize in a meson, and the product of the reconstruction, trigger, and selection efficiencies. Since the number of produced, , will not be precisely known, the use of a normalization channel of well-known branching fraction is required to obtain an absolute measurement of the branching fraction or upper limit.

The branching fraction is then:

where , and are the quantities for the normalization channel, with definitions analogous to those of the signal channel.

Possible normalization channels are and . Particular care has been taken to analyze the signal and normalization channels in a common way such as to cancel any large systematic effects in the efficiency ratio.

The main systematics arise from the uncertainty on the ratio or . With sufficient statistics, all other systematic uncertainties are expected to get much smaller than that, as the analysis relies solely on data. To eliminate the factor , the decay mode could be used in the future a normalization channel, if its absolute branching fraction can be measured more precisely at Belle.

The expected sensitivity of LHCb to the decay as a function of the integrated luminosity is shown in Fig. 3. The solid line in the left plot shows the expected upper limit, at 90% confidence level, on the branching fraction when no signal is observed, for collisions at . The branching fraction for which a discovery (or for which a evidence) is expected, is shown on the right plot for 14 collisions.

The left plot also indicates the expected limit from the Tevatron experiments, extrapolating the current results to 8 of data per experiment. It shows that LHCb can compete with the Tevatron with approximately 0.1 of data and overtake its expected limit with about 0.2. In that time frame, the detector may not be fully understood yet. Therefore, an alternative robust analysis is designed using variables with a physical content similar to the ones of the standard analysis, but avoiding the use of error estimates. This implies a modified selection and definition of the geometrical likelihood. The robust analysis sensitivity is also depicted in Fig. 3 (left), as a red dashed curve. The robust analysis presents a sensitivity comparable with the one of the standard analysis. Therefore, it constitutes a valuable option for the early data.

About 3 (10) are enough for a evidence ( observation) if the branching fraction is equal to the SM prediction. Any enhancement driven by NP will be observed sooner. Particularly, if the branching fraction is as high as , as predicted in Ref. Ellis07_WMAPMSSM (), a discovery is possible with very little luminosity ().

V Conclusion

The large production cross-section expected at LHC, together with the characteristics of LHCb, leads to a good performance in the search for NP in FCNC decays. Rare decays are particularly interesting because of the precise theoretical predictions for some of their observables, and they provide stringent test of the SM and its extensions. Expected sensitivities for LHCb’s analyzes of the most promising rare decays were presented.

One year of data taken in nominal conditions yields to the observation of the photon polarization in the decay to a 10% level and to the measurement of the zero-crossing point to a resolution in the decay mode. The same amount of data allows to set a limit on the branching fraction down to the SM prediction if no signal is observed, strongly constraining NP models with high values. In case the branching fraction is enhanced, an observation of NP is possible.

In the long term, a full angular analysis of the can be performed and bringing enhanced sensitivity in probing for NP. A discovery of the decay is possible if the branching fraction is at the SM level with about 10. Any NP enhancement will be discovered before.


References

  1. A. Alves et al. [LHCb collaboration], JINST 3, S08005 (2008).
  2. L. Evans and P. Bryant (Eds), JINST 3, S08001 (2008).
  3. J. Wicht et al. [Belle collaboration], Phys. Rev. Lett. 100, 121801 (2008), [hep-ex/0712.2659].
  4. R. N. Mohapatra and J. C. Pati, Phys. Rev. D11, 566 (1975).
  5. H. E. Haber and G. L. Kane, Phys. Rept. 117, 75 (1985).
  6. D. Atwood, M. Gronau and A. Soni, Phys. Rev. Lett. 79, 185 (1997).
  7. Y. Ushiroda et al. [Belle collaboration], Phys. Rev. D74, 111104 (2006), [hep-ex/0608017].
  8. B. Aubert et al. [BaBar collaboration], Phys. Rev. D78, 071102 (2008), [hep-ex/0807.3103].
  9. F. Muheim, Y. Xie and R. Zwicky, Phys. Lett. B664, 174 (2008), [hep-ph/0802.0876].
  10. L. Shchutska, A. Golutvin, and I. Belyaev, CERN-LHCb-2007-030, 2007.
  11. L. Shchutska et al., CERN-LHCb-2007-147, 2007.
  12. C. Amsler et al. [Particle Data Group], Phys. Lett. B667, 1 (2008), and 2009 partial update for the 2010 edition.
  13. M. Beneke, T. Feldmann, and D. Seidel, Eur. Phys. J. C41, 173 (2005), [hep-ph/0412400].
  14. B. Aubert et al. [BaBar collaboration], Phys. Rev. D73, 092001 (2006), [hep-ex/0604007].
  15. I. Adachi et al. [Belle collaboration], BELLE-CONF-822, [hep-ex/0810.0335].
  16. T. Aaltonen et al. [CDF collaboration], Phys. Rev. D79, 011104 (2009), [hep-ex/0804.3908].
  17. J. Dickens, V. Gibson, C. Lazzeroni, and M. Patel, CERN-LHCb-2007-039, 2007.
  18. F. Jansen, N. Serra, G. Y. Smit, and N. Tuning, CERN-LHCb-2009-003, 2009.
  19. W. Reece and U. Egede, CERN-LHCb-2008-041, 2008.
  20. U. Egede, T. Hurth, J. Matias, M. Ramon, and W. Reece, JHEP 11, 032 (2008), [hep-ph/0807.2589].
  21. M. Blanke, A. Buras, D. Guadagnoli, and C. Tarantino, JHEP 10, 003 (2006), [hep-ph/0604057].
  22. J. Ellis, T. Hahn, S. Heinemeyer, K. A. Olive, and G. Weiglein, JHEP 10, 092 (2007), [hep-ph/0709.0098].
  23. CDF collaboration, CDF Public note 9892, 2009.
  24. D. Martinez et al., CERN-LHCb-2007-033, 2007.
  25. A. Read, CERN Yellow Report 2000-005, 2000.
Comments 0
Request Comment
You are adding the first comment!
How to quickly get a good reply:
  • Give credit where it’s due by listing out the positive aspects of a paper before getting into which changes should be made.
  • Be specific in your critique, and provide supporting evidence with appropriate references to substantiate general statements.
  • Your comment should inspire ideas to flow and help the author improves the paper.

The better we are at sharing our knowledge with each other, the faster we move forward.
""
The feedback must be of minimum 40 characters and the title a minimum of 5 characters
   
Add comment
Cancel
Loading ...
224035
This is a comment super asjknd jkasnjk adsnkj
Upvote
Downvote
""
The feedback must be of minumum 40 characters
The feedback must be of minumum 40 characters
Submit
Cancel

You are asking your first question!
How to quickly get a good answer:
  • Keep your question short and to the point
  • Check for grammar or spelling errors.
  • Phrase it like a question
Test
Test description