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Branching ratio and helicity amplitudes for  b   (pK)  decays (  spin = 3/2) Combined work of: Gudrun Hiller (Dortmund UNI), the Bearer of the Light.

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Presentation on theme: "Branching ratio and helicity amplitudes for  b   (pK)  decays (  spin = 3/2) Combined work of: Gudrun Hiller (Dortmund UNI), the Bearer of the Light."— Presentation transcript:

1 Branching ratio and helicity amplitudes for  b   (pK)  decays (  spin = 3/2) Combined work of: Gudrun Hiller (Dortmund UNI), the Bearer of the Light Thomas Schietinger (PSI), the Scholar Mathias Knecht and Federica Legger (EPFL), the water Carriers Theoretical physics for experimentalists:

2 2 Outline  Once upon a time:  the electromagnetic penguin b  s   the photon polarization (theory and experiment)  my thesis results & open questions  The mighty quest for  spin = 3/2:  Branching ratio for  b   (pK)   the tools: Mathematica  Helicity amplitudes  Sensitivity to photon polarization  Summary and outlook

3 3 Motivations  Standard Model (SM): best description of known elementary particles and their interactions:  passed all experimental tests up to now;  still one missing particle, the Higgs boson. However...  19 (!!!) free parameters;  gravity is not included.  Quest for new physics in the quark sector:  CKM picture is very successful  but we still know little about b  s, d transitions ! quarks leptons udud cscs tbtb e  

4 4 The electromagnetic penguin b  s   New physics in the decay rate :  are there any contribution from supersymmetric particles?  the measured b  s  branching fraction is compatible with SM prediction  Theory: BF(b  s  ) [10 -6 ]= 357 ± 30  Experiment: BF(b  s  ) [10 -6 ]= 355 ± 24 +9 -10 ± 3  from HFAG (combined measurements by Belle, BaBar, CLEO)  Need other observables to test the SM... Gambino, Misiak, NPB 611 (2001) 338 http://www.slac.stanford.edu/xorg/hfag/rare b s u,c,t W 

5 5 b s W   The W boson only couples to a left-handed s quark  Left-handed photon (to conserve ang. momentum) “Naïve” SM Atwood, Gronau, Soni, PRL 79, 185 (1997) Photon polarization:  pure 2-body decay: right-handed components of the order of r = m s /m b Grinstein, Grossman, Ligeti, Pirjol, PRD 71, 011504 (2005) SM + QCD  when considering b  s  + gluons  right-handed components may be up to 10-15%  explicit calculations only for B  K*  B  The electromagnetic penguin b  s 

6 6 Photon polarization measurements Melikov, Nikitin, Simula, PLB 442, 381 (1998) Grossman, Pirjol, JHEP06, 029 (2000) Atwood, Gronau, Soni, PRL 79, 185 (1997) Mannel, Recksiegel, JPG: NPP 24, 979 (1998) LHCb B factories Knecht, Schietinger, PLB 634, 403 (2006) Gronau, Pirjol, PRD 66, 054008 (2002) B-B interference First measurements of K* polarization in B->K*l+l- by Belle/Babar e + e - conversion Exp. statusTheor. Refs. Latest world average sin2  = 0.0 ± 0.3 Higher K* resonances Difficult to disentangle resonance structure (Babar, hep/0507031) Gronau, Grossman, Pirjol, PRL 88, 051802 (2002) Charmonium res. interference No results so far... b-baryons Hiller, Kagan, PRD 65, 074038 (2002) Exploit ang. correlations between polarized initial state and final state. Under study at LHCb (F.Legger, M. Knecht) Legger, Schietinger, PLB 644 (2007) xxx

7 7 Polarized b baryons decays s d  u b d u bb  Hiller, Kagan, PRD 65, 074038 (2002)  If initial state is polarized:  exploit angular correlations between initial and final states  only possible with b baryons  feasible at hadron colliders Mannel, Recksiegel, JPG: NPP 24, 979 (1998) Case study:  b  (  (1115)  p  )  Long distance contributions from internal W exchange, or vector meson cc contributions are expected to be small

8 8 Polarized  b   (1115)  decays  Angular distributions  depend on photon polarization    P B =  b polarization   p = weak decay parameter Evtgen   = 1 P B = 1 cos  ,  b rest framecos  p,  rest frame  b   (1115)    (fit) = 1.036   (theory) = 1  p (fit) = 0.679  p (theory) = 0.642  b   (1115) 

9 9 However...  From the experimental point of view the decay  b   (1115)  is quite hard to observe (c  = 7.89 cm)  Can we probe the photon polarization in heavier  resonance decays?   b  (  (X)  pK)   what do we need?  Branching ratios for  b   (X)   Angular distributions for  spin = 1/2, 3/2  spin > 3/2: helicity states > observables s d u b d u bb  u u p K

10 10  (X) resonance spectrum 1690 1670  spin = 1/2  spin = 3/2 1520  Invariant pK mass spectrum obtained with:  BR(  b   (X)  ), calculated rescaling BR(  b   (1115)  ) with a kinematical factor, assuming the same form factors and no spin dependence for all  (X) resonances. PDG 2004 Legger, Schietinger, PLB 644 (2007) xxx

11 11 Helicity formalism for  b   (pK)   Photon helicity = ±1,   helicity = ±1/2  2 helicity amplitudes  Photon angular distribution  Proton angular distribution flat because of P conservation J  = 1/2  Photon helicity = ±1,   helicity = ±1/2, ±3/2  4 helicity amplitudes  Photon angular distribution J  = 3/2 Legger, Schietinger, PLB 644 (2007) xxx

12 12    depends on the asymmetry of  b spin with respect to photon momentum  and can be factorized into the photon helicity parameter   and the strong parameter    can be extracted from the proton angular distribution  b   (pK)  decays  (J  = 3/2) Legger, Schietinger, PLB 644 (2007) xxx

13 13  The photon helicity can be probed in decays involving  resonances of spin 3/2 by measuring   3/2 and   Can we get a better estimate of the BR ?  Include at least the spin dependence  Form factors will have to be measured  Can we get an estimation of  ? Open questions

14 14  Electromagnetic dipole operators:  long distance effects  non perturbative approach (HQET)  Wilson coefficients: C 7, C 7 ’  short distance  Fermi theory (point-like interactions) The effective hamiltonian: Decay amplitude for  b   (1520) 

15 15 The effective hamiltonian: Decay amplitude for  b   (1520)  The matrix element:  bb  (p, s) (q,  ) (p´,s´)

16 16 The effective hamiltonian: Decay amplitude for  b   (1520)  The matrix element: Find   and   !! u(p,s) = Dirac spinor to describe the  b (spin 1/2) Rarita-Schwinger (RS) spinor to describe the  (spin 3/2) Dirac spinor Polarization vector 1/2  1 = 3/2 Rarita, Schwinger, Phys Rev 60(1941) 61

17 17 Conditions Gauge invariance On-shell photon Equations of motion (EOM) RS spinors Main actors:

18 18   and   Ansatz: We define the tensor   (antisymmetric in  and ):

19 19   and   Ansatz: On-shell photon! Reabsorbed in B and C using EOM We define the tensor   (antisymmetric in  and ):

20 20   and   We define the tensor   (antisymmetric in  and ): Ansatz: On-shell photon! Reabsorbed in B and C using EOM Contracting with q 

21 21   and   Form factors  (5)  is related to  (5)  through the identity: it is straightforward to obtain (ask Mathias) :

22 22 Spin averaged matrix element To evaluate the BR we need: where Writing explicitely the spinor indices!

23 23 Spin averaged matrix element Sum over spins: Aliev, Ozpineci, hep-ph/0406331 We finally obtain: To calculate the trace we use: with the TRACER package

24 24 Trace evaluation

25 25 Trace evaluation

26 26 Branching Ratio In the limit f2f2 BR (  b   0  ~ 7·10 -5

27 27 HFAG ICHEP 2006 From B + and B 0 radiative decays, and dedicated form factors studies, BR should have the same order of magnitude K*(892) = vector K 1 (1270) = axial vector K 1 (1400) = axial vector K 2 *(1430) = tensor S. Veseli, M.G. Olsson, Z. Phys. C 71 (1996) 287

28 28 Helicity amplitudes We use the  b rest frame:  bb  p´=(E´,0,0,E) q=(E,0,0,-E) z

29 29 Helicity amplitudes The amplitudes A  3/2 (A  1/2 ) result from a  b -baryon with h =  1/2 (h = +1/2) and a photon with J z = +1 Photon polarization vectors: JzJz in  b rest frame:  polarization vectors:  helicity RS spinor Dirac spinor

30 30 Helicity amplitudes: results In the limit and f 1 ~f 2 Right-handed photon

31 31 Helicity amplitudes: naïve picture  bb  Opposed b and  b spin -> suppressed ~ O(1/m b ) Left-handed photon = SM b s M. Suzuki, J. Phys. G: Nucl. Part. Phys. 31 (2005) 755  bb  b s Spin flip b vs s Quark level:  b s Spin flip  b vs 

32 32 Sensitivity to the photon polarization Photon polarization:  b Polarization = 20% 10k  (1520) events (~3 yrs LHCb running ) 3  significance

33 33 Conclusions and outlook  The BR(  b   ) has been calculated in the framework of HQET  form factors will need to be measured  Helicity amplitudes for the decay  b   have been evaluated  straightforward extension to decay involving J P = 3/2 + resonances, by replacing C ’ 7 -> -C ’ 7  Still to do: work out a better estimate of the Lb polarization  (Some) theoretical models and calculations are (also) accessible to experimentalists!

34 Backup slides

35 35  b production at LHC:  bb cross section in pp collision = 500  b   10% of produced bb hadronize in baryons   b dominates (  90%)   b produced with transversal polarization  Expectations are P B ~ 20%  ATLAS plans to measure it with a statistical precision better than 1% p1p1 p2p2 bb n Ajaltouni, Conte, Leitner, PLB, 614 (2005) 165 Feasibility of Beauty Baryon Polarization Measurement in  b  J  decay channel by ATLAS – Atlas note 94-036 PHYS

36 36 Photon polarization   b   (1670)  selected evts.  transversally polarized  b )  efficiency corrected (from unpolarized decays)  from data, the correction can be obtained from B  K*  decays 

37 37 Sensitivity on |r| measurement  Values of |r| that can be probed from single measurements  Getting close to the SM expected range, becomes interesting if NP! 1 year, 3  5 years, 3  SM naive SM + QCD SM naive SM + QCD  b Polarization = 20%

38 38 Combined measurements 1 year, 3  5 years, 3  SM naive SM + QCD  Combining measurement increases range by a few percent at most   (X) measurements have good sensitivity (in case  (1115) turns out to be difficult)  b Polarization = 20% SM naive SM + QCD

39 39 Dependence on  b polarization  If only the photon asymmetry is measured, a polarization of at least 20% is needed to have good sensitivity  b   (X)  b   (1115)  1 year


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