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Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On...

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Radiative Decays @ LHCb Vanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) On behalf of LHCb Collaboration
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Page 1: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Radiative Decays @ LHCb

Vanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow)On behalf of LHCb Collaboration

Page 2: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 2

Outline

• Radiative penguins & photon polarization in b→ s g transitions

• Event Selection

• Probing for the photon polarization in Bs →fg

• Early data

• Summary

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Page 3: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 3

Loops and Penguins

•Rare (≡“loop-induced” ) and especially penguin-mediated decays are essential part of LHC(b) physics program:• Electroweak penguin B0 →K*0 m+m-

• talk by Will Reece

• Gluonic penguin Bs→ ff • Talk by Olivier Leroy , also charmless B-decays, talk by Lorence Carson

• Hunting for “SUSY/Higgs penguin”: Bs →m+m- • talk by Diego Martinez Santos

And the radiative penguins are here …

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LHC(b) penguinarium

Page 4: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 4

Radiative penguins

• Radiative penguin decays of B+&B0 mesons have been discovered by CLEO and both inclusive b→sg and exclusive decays have been intensively studied by CLEO, BaBaR and Belle• Br(b →sg) is one of the most efficient killer for

New Physics Models

• Belle has observed Bs →fg

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Belle: O(1 Bs→fg)/day at Y(5S)

Page 5: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 5

Why penguins are attractive?

• The clear picture in SM:• One diagram dominance• One Wilson coefficient C7

eff(m)

• Reliable theoretical description at (N)NLO allows the numerically precise predictions

• Loops• New Physics contribution can be comparable and

even dominating to (small) SM amplitudes • NP appears not only in modifications of Br, but also

in asymmetries and the angular effects • “Sensitive also to spin structure of NP”

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Page 6: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 6

• Not so rare decaysBr(B→K*0g ) = (4.3±0.4)x10-5

Br(Bs→fg ) = (3.8±0.5)x10-5

• 1-amplitude dominance

• strong phase appears at order of as or 1/mb

→“Direct” asymmetries are small (<1%) for b→sg & a bit larger O(10%) for b→dg

• Photons are polarized• Mixing asymmetries

vanishes, *BUT*

Exclusive radiative penguins

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Suppressed by : as , 1/mb or |VCKM|

Page 7: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 7

Mixing asymmetries are vanished, but …

• B→ fCP g is not CP eigenstate! gR/gL ≈ms/mb

• Take it into account:

• SM: • C = 0 direct CP-violation• S = sin2 y sinf• AD = sin2 y cosf

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not suppressed!

Page 8: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

8

B0→ KS p0 g

BaBar Belles(sin2y ) ~ 0.4

Page 9: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 9

DGs/Gs≠ 0

• C is practically zero• 1 diagram dominance

• S is a product of CP-eigenstate fraction and (small) phase difference of Bs oscillation and b→sg penguin

• double smallness is SM

• AD is just a fraction of CP-eigenstate • ≡ Fraction of wrongly polarized photons• No “other” suppression factors, only DGs/Gs

Essentially we study CP-violation in Bs→fg as an instrument to probe Lorentz structure of b→sg transitionsF.Muheim, Y.Xie & R.Zwicky, Phys.Lett.B664:174-179,2008

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Page 10: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 10

Expected performance for Bs→fg at LHCb

• What we “know” now:

• The yield is 11k per 2 fb-1 (and 70k of B0→ K*0g)

• Background is • <6k @ 90%CL

• The mass resolution ~96 MeV/c2

• Ecal resolution

• The proper time resolution: s~78fs• 50/50 s1=52fs, s2=114fs

L.Shchutska et al, CERN-LHCb-2007-03010.9.2k+9

LHCb: O(3 Bs→fg)/hour at 2x1032

Full Monte Carlo simulation

Page 11: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 11

Trigger

• Hardware L0 trigger for photons with high ET

• Next trigger levels (software) :• Photon confirmation (& suppression of merged

p0) and single (or pair) detached track reconstruction• e ~ 70%

• Full reconstruction of Bs →fg candidate

• Reconstruction of f-candidate • “inclusive f” trigger

More details in dedicated talk by Leandro de Paula10.9.2k+9

Large overlap,

high redundancy & robustness: e ~

95%

Page 12: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 12

Event selection

• B-decay products do not point to reconstructed primary vertices• Exclusively reconstructed B-candidate does point to primary vertex• B-candidate is

associated with the primary vertex with minimal impact parameter (significance)

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Page 13: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 13

Signal proper time resolution

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Page 14: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 14

Sensitivity to sin2y

• To evaluate our sensitivity to sin2y• toy Monte Carlo (104 experiments)

• Unbinned maximum likelihood fit• Proper lifetime & error • Reconstructed mass

• Per-event proper time errors

• Resolutions & Efficiencies from full MC

• Parameterize the background from mass-sidebands

• Important ingredient – proper time acceptance function

L.Shchutska et al, CERN-LHCb-2007-147

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m(Bs) = 5.367 GeV/c2

t(Bs) = 1.43 ps

DGs = 0.084 ps-1

Dms = 17.77 ps-1

Page 15: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 15

Proper time acceptance

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a = 0.74 ps-1

c = 1.86

dN/dt es(t)

Page 16: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 16

Proper time acceptance

• It is a vital to know it with very high precision• 5% bias in “a” -> bias in sin2y ~ 0.2

• We are planning to calibrate it using three techniques:• B0→ K*0 g• Bs→ f J/ y

• “per-event-acceptance” (“swimming” method)

• The acceptance could be extracted from data for all cases• E.g. with ~O(1%) precision for B0→ K*0 g

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Page 17: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 17

Background parameterization

• Fit separately left and right sidebands

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Left Right

Page 18: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 18

Results: s(AD,C,S)

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s(AD

)=0.22 s(S)=s(C)=0.11

2fb-1

Page 19: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 19

• Already with “early” data the measurements of direct CP-asymmetry in B→ K*0 g

• Double ratio:

•Measurement of B→fKg

“early measurements”

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The first 13 minutes @

nominal luminosity

B→ K*0

g

Page 20: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 20

Conclusions

• LHCb has good potential for measurement of photon polarization in Bs→fg decay

• For 2 fb-1: s(AD)=0.22, s(S)=s(C)=0.11

• The determination of proper time acceptance function from data in under the study:

• Three methods

• The result has moderate dependency on B/S

Stay tuned and wait for more news

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Page 21: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 21

Backup slides

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Page 22: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 22

Example of models

• Anomalous right-handend top couplings J.P.Lee’03

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lg = -cos 2y

Page 23: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 23

B: proper-time in sidebands

• Fit separately left and right sidebands

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Page 24: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 24

Signal proper time resolution as function of cosQ

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Page 25: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 25

Signal proper time resolution as function of cosQ

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-1.0 : -0.5 -0.5 : -0.15

-0.15 : 0.3 0.3: 1.0

Page 26: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 26

The shape of background

• Vary the “short/long”-lived components

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Relative change Absolute change

Page 27: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 27

Stability tests: B/S

• There is some dependency on B/S level:

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Conservative UL @ 90% CL

Page 28: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 28

Results: pulls

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AD

CS

Page 29: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 29

Resolution and DGs/Gs

• Vary the proper time resolution• Use simple model with two Gaussians and vary

the proportion

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Page 31: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

Vanya Belyaev: Radiative decays @ LHCb 31

Background parameterization

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Page 32: Radiative Decays @ LHCb Vanya BELYAEVVanya BELYAEV (NIKHEF/Amsterdam & ITEP/Moscow) Vanya BELYAEV On behalf of LHCb Collaboration.

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Likelihood

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