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B Factory B Factory Measurements of the Measurements of the b s(d) s(d) “Radiative Penguin” “Radiative Penguin” Transition Rates Transition Rates for the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16- 21, 2008 Bruce A. Schumm Santa Cruz Institute for Particle Physics University of California, Santa Cruz BaBar
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For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Dec 19, 2015

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Page 1: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

B Factory Measurements B Factory Measurements of the bof the b s(d) s(d) “Radiative “Radiative Penguin” Transition RatesPenguin” Transition Rates

for the BaBar and Belle Collaborations

Miami 2008 Topical Conference on Elementary Physics, Astrophysics,

and Cosmology

Fort Lauderdale, FL, Dec 16-21, 2008

Bruce A. SchummSanta Cruz Institute for Particle Physics

University of California, Santa Cruz

BaBar

Page 2: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 2Bruce SchummBaBar

OutlineOutline

Effective Neutral Currents: General Motivation

b s PenguinsSUSY parameter space implications

b s “Inclusive” approach

B XS “Semi-Inclusive” approach

b d Penguins and |Vtd/Vts|

Motivation

B →(ρ,ω)“Exclusive” approach

B→Xd “Semi-Inclusive” approach

Status of |Vtd/Vts|

Conclusions

Page 3: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 3Bruce SchummBaBar

Effective Neutral Currents and Radiative PenguinsEffective Neutral Currents and Radiative Penguins

so new physics can enter at leading order:

The SM b s(d) transition is high order (two weak plus one EM vertex) …

+ photon off any charged

leg

Although rare (~ 5x10-4 for s and ~10-5 for d), the isolated high-energy photon is a powerful signature.

Vtb Vt(s,d)

Page 4: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 4Bruce SchummBaBar

OutlineOutline

Effective Neutral Currents: General Motivation

b sSUSY parameter space implications

Inclusive approach

Other approaches

b d and |Vtd/Vts|

Motivation

B →(ρ,ω)(“Standard” Approach)

B→Xd (“Semi-Inclusive” Approach)

Status of |Vtd/Vts|

Conclusions

Page 5: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 5Bruce SchummBaBar

B B s s and SUSY Parameter Space and SUSY Parameter Space

Direct searches (LEP)

B s constraints

MSSMConstraints

bs has a significant impact on the tan-mA plane…

Page 6: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 6Bruce SchummBaBar

B B s s and SUSY Parameter Space (cont’d) and SUSY Parameter Space (cont’d)

Fate of “Snowmass” MSSM study points

… on some of our favorite scenarios …

Page 7: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 7Bruce SchummBaBar

B B s s and SUSY Parameter Space (cont’d) and SUSY Parameter Space (cont’d)

C.F. Berger, J.S. Gainer, J.L. Hewett, T.G. Rizzo,“Supersymmetry Without Prejudice”, arXiv:0812.0980v1 [hep-ph]

Explore 107 points over 19-dimensional parameter space of CP-conserving MSSM

b s most effective constraint (72% of models surviving prior constraints are eliminated; better than direct searches for SUSY partners)

… and just in general.

Page 8: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 8Bruce SchummBaBar

The eThe e++ee-- Cross Section in the Upsilon Region Cross Section in the Upsilon Region

bbOn-Peak Data

Off-Peak Data(~10% of Sample)

(4S) resonance is ~1 nb at peak, competing with a “continuum” background of ~3 nb

The (4S) resonance is the lightest resonance that decays into “open Beauty” ( or ) 00BBBB

bb

Page 9: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 9Bruce SchummBaBar

B Factory Data SetsB Factory Data Sets

700 fb-1

440 fb-1

Page 10: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 10Bruce SchummBaBar

Inclusive Measurement of b Inclusive Measurement of b s s: Introduction: Introduction

qq + ττ

BB

XSγ

Most exacting approach (“Inclusive”) is aggressive:

Use only high-energy as signature

Suppress continuum with event shapes, requirement of a high-energy lepton.

Estimate remaining contribution by scaling off-peak data.

Challenge: background from 0() decays (plus some fakes) in B decays

Page 11: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 11Bruce SchummBaBar

Inclusive Measurement of b Inclusive Measurement of b s s: Practicalities: Practicalities

To remove 0() background:

• Veto event if you find the 2nd photon (~45% efficient for 0() fakes)

• Estimate and subtract out cases for which 2nd photon is missed (S/B ~ 1/1)

• Requires knowledge of second photon efficiency to < 1%; measure using, e.g., 0s from e+e- ; +-0

• Becoming limiting experimental uncertainty

No s signal here; provides test of 0 subtraction

BELLE: (3.370.43)x10-4 arXiv:0804.1580 605 fb-1

BaBar: (3.920.56)x10-4 PRL97,171803 82 fb-1

NOTE: Measurements scaled to Ecms = 1.6 GeV

Page 12: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 12Bruce SchummBaBar

b b s s Via a Sum of Exclusive Final States (BaBar) Via a Sum of Exclusive Final States (BaBar)

This “Semi-Inclusive” approaches employs a fit to the mass distribution, for which backgrounds tend to be self-calibrating…

Reconstruct a total of 38 exclusive b s final states that comprise about 55% of the total width

Fit to reconstructed mass of exclusive final state to determine signal yield

Page 13: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 13Bruce SchummBaBar

BaBar Semi-Inclusive Analysis (continued)BaBar Semi-Inclusive Analysis (continued)

But need to rely on models to correct for the 45% of states that are not measured (depends on mass M(Xs) that photon recoils against).

Mass Recoiling Against RESULT

BF(B s) = (3.49 0.57)x10-4

PRD72:052004

• 82 fb-1 analyzed is less than 10% of world sample

• Has systematics independent of those of inclusive approach

Page 14: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 14Bruce SchummBaBar

Summary of Measurements of the b Summary of Measurements of the b s s Rate Rate

Experimental accuracy commensurate with theoretical control, but work continue on both ends

Inclusive

Semi-Inclusive

Inclusive

Inclusive

Inclusive

A. Limosani, Melbourne

Most of BaBar data set still unanalyzed

Page 15: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 15Bruce SchummBaBar

OutlineOutline

Effective Neutral Currents: General Motivation

b sSUSY parameter space implications

Inclusive approach

Other approaches

b d and |Vtd/Vts|

Motivation

B →(ρ,ω)(“Standard” Approach)

B→Xd (“Semi-Inclusive” Approach)

Status of |Vtd/Vts|

Conclusions

Page 16: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 16Bruce SchummBaBar

Measuring |VMeasuring |Vtdtd/V/Vtsts||

(d) (d)(d)

(d)

(d)

(d)

Vt(s,d)Note: In both cases, hadronic

uncertainties minimized by comparing to corresponding Vts

process (Bs mixing, b s)

Observable is | Vtd / Vts |

B Mixing

Radiative Penguins

Two independent diagrams provide sensitivity to CKM

parameter Vtd

Page 17: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 17Bruce SchummBaBar

|V|Vtdtd/V/Vtsts| from Penguins: Motivation| from Penguins: Motivation

ICHEP ’08 B Mixing Results [Farrington(CDF), Moulik(D0), averaged by DeLodovico(BaBar)]:

How do penguins fit into the picture?

Mixing: xd = mB/B ~ 1 mB ~ B

Penguins: Br(bd) ~ 10-5 d ~ 10-5 B

“These [b d] vertices are CKM-suppressed in the standard model, but new physics contributions may not follow the CKM pattern in flavor-

changing-neutral-current transitions and hence new physics effects may become more easily discernible in B Xd + (and its charge conjugate)

than in the corresponding CKM-allowed vertices b s and b sg”

Furthermore (Ali, Asatrian, Greub, Phys. Lett B 429, 87):

With |Vtd/Vts| precisely constrained by mixing, b d is a compelling testbed for

new physics.

SM effects suppressed

by 10-5 relative to

mixing

Page 18: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 18Bruce SchummBaBar

Exclusive Approach: B Exclusive Approach: B (() )

“Traditional” Approach: measure exclusive rate Br(B () ); normalize with Br(B K* )

(and )

Values of 2 and R are state (+,0,) dependent and are available from

Ali, Parkhomenko, arXiv:hep-ph/0610149

Ball, Zwicky, J. High. Energy Phys. 0604, 046 (2006); Ball, Jones, Zwicky, Phys. Rev. D 75 054004 (2007)

at approximately 8% overall accuracy.

Annihilation Diagram

Page 19: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 19Bruce SchummBaBar

Measurement of B(B Measurement of B(B (() ) ) )

Belle: New result this Spring

351 fb-1 (2006) 598 fb-1 (April 2008)

BaBar: New result this Summer

316 fb-1 (April 2007) 423 fb-1 (July 2008)

Challenge: BRs are small (<10-6); backgrounds are high

continuum Neural Net with event shape, B tagging information, …

B → K*; K* K Require excellent particle ID

B → ( Veto if found such that M ~ M(,)

Page 20: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 20Bruce SchummBaBar

Measurement of Measurement of BB(B (B (() ) ) (continued)) (continued)

2*2*BbeamES pEM

Remaining separation achieved by two-dimensional fit to the largely independent kinematic variables

“Energy-substituted mass”; since Ebeam ~ MB, largely a measurement of momentum balance

*In e+e- CMS frame

EB = Ebeam for properly reconstructed candidate; total energy measurement

2*2*

BbeamESpEM

***

beamBEEE

Example: BaBar B0 0 “self-calibrating” continuum background subtraction

efficiencies (~5-15%) estimated with control samples

SignalContinuum

bs Feedthrough

Page 21: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 21Bruce SchummBaBar

Recent Updates of B Recent Updates of B (() )

Mode BaBar ’07 (x10-7) BaBar ’08 (x10-7)

+ 0

6.07.9 4.2

2.2

0.20.12 2.4

7.3

9.00.11 7.3

3.3

6.09.7 2.2

0.2

Mode Belle ’06 (x10-7) Belle ’08 (x10-7)

+ 0

9.09.2

1.17.27.8

9.07.1

0.16.18.7

3.10.4 9.1

7.1

9.02.4

8.06.35.5

7.07.3

6.03.35.12

5.04.3

0.17.26.5

9.00.5 7.2

3.2

5.00.4 4.2

0.2

BELLE: 598 fb-1

BaBar: 423 fb-1 Phys.Rev.D78:112001,2008

Phys.Rev.Lett.101:111801,2008, Erratum-ibid.101:129904,2008

Page 22: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 22Bruce SchummBaBar

|V|Vtdtd/V/Vtsts| from Exclusive (| from Exclusive (,,) Decays) Decays

70.3

8.210)6.13.16()),((B

B

015.0195.0|/| 020.0019.0

tstdVV

022.0025.0021.0024.0

233.0|/|

tstdVV

BELLE:

assuming the world-average

Combining, for exclusive radiative decay overall:

70.1

2.110)0.24.11()),((B

B

BaBar:

yielding

yielding

5* 10)17.016.4()(B KB

018.0015.0210.0|/| tstdVV

Assuming startic quark model, SU(3)F symmetry, can combine to get “isospin-averaged” BF, and then |Vtd/Vts|:

Page 23: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 23Bruce SchummBaBar

Semi-Inclusive Approach: B Semi-Inclusive Approach: B X Xdd (Preliminary) (Preliminary)

|Vtd/Vts|2 related to (bd)/(bs) with ~1% theoretical uncertainty [Ali, Asatrian, Greub, Phys. Lett. B 429, 87 (1998)]

However, must correct for unmeasured regions:

• Higher-multiplicity final states

• Higher-mass hadronic component (i.e. MXd > 1.8 GeV/c2)

“New” Approach (BaBar): Reconstruct seven exclusive final states Xd in range 0.6 GeV/c2 < MXd < 1.8 GeV/c2

Page 24: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 24Bruce SchummBaBar

Measured Regions for B Measured Regions for B X Xd(s)d(s)

(,,K*) 1.0 < Mhad < 1.8 1.8 < Mhad

XS

Xd

MEASURED

UNMEASURED

and Xd analyses

Xd analysis only

Mhad (MXd)

# 0

# bodies

Page 25: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 25Bruce SchummBaBar

B B X X(s,d)(s,d) Partial Branching Fraction Results Partial Branching Fraction Results

Fit in high-mass Xd region (first time measured):

Yields and partial branching fractions:

High-mass b

Xd

Continuum background

Xs, MisID background

BABAR

BABAR

PRELIMINARY

Page 26: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 26Bruce SchummBaBar

Correction for Missing ModesCorrection for Missing Modes

Dominant systematic error for 1.0 < MX < 1.8 GeV/c2

Most difficult for B Xd (not constrained by data)

Can improve with statistics (internal constraints)

Errors: Statistical Experimental Systematic

Try several models:

• MX given by “KN Model” Kagan & Neubert, Phys. Rev. D 58,

094012 (1998), with phase-space fragmentation

• As above, but with 50% replaced by mix of resonances

• Fix to measured b s fragmentation

Primary experimental result

BABAR

PRELIMINARY

Page 27: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 27Bruce SchummBaBar

Ratio of Total Widths and |VRatio of Total Widths and |Vtdtd/V/Vtsts||

arXiv:0807.4975 [hep-ex]; submitted to PRL

Precise (~1%) expression for |Vtd/Vts| [Ali, Asatrian, Greub] is based on ratio of full widths (bd)/(bs)

Measured region 0.6 < MX < 1.8 is ~50% of width

Extrapolate to full mass region via “KN Model”; KN calculation suggests negligible difference and uncertainty in extrapolation of the ratio (because ms,md << 1.8 GeV/c2?)

Ali

Asatrian

Greub

)(

)(

sb

db

009.0013.0033.0

|/|tstdVV

001.0043.0177.0

Expt. Theory

BABARBABAR PRELIMINARY

PRELIMINARY

Page 28: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 28Bruce SchummBaBar

Global Status of |VGlobal Status of |Vtdtd/V/Vtsts||

No evidence for non-Standard Model contribution to the decay width.

*

PRELIMINARY*

Page 29: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 29Bruce SchummBaBar

Concluding RemarksConcluding Remarks

Radiative measurements of |Vtd/Vts| are becoming precise:

| Vtd/Vts|rad = 0.203 0.020

Semi-inclusive approach works, and is independent of exclusive approach, with small theoretical uncertainty

Agreement with SM (as constrained by B mixing) is good

In principle, the severe SM suppression of this radiative process (x10-6 of B mixing) should make it very sensitive to new physics contributions.

Have we fully thought through the meaning of this constraint?

B s continues to be leading constraint on MSSM parameter space

More data exists (~80% of BaBar sample) to improve measurement, but “inclusive” approach starting to be limited by difficult systematics

“Semi-inclusive” approach has systematics independent of inclusive approach; very little of existing sample has been analyzed in this way.

Page 30: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 30Bruce SchummBaBar

Backup Slides

Page 31: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 31Bruce SchummBaBar

Isopsin-Averaged Branching FractionsIsopsin-Averaged Branching Fractions

)(2)(2)( 000 BBB

dduu 2

1 dduu 2

10

)()(B)(B2

1]),([B 000

0

BBBBBB

B

Assuming SU3(F) symmetry [B(B0) ~ B(B)] and

(approximately true by static quark model) we can write

from which it follows

Can combine +, 0, results to derive |Vtd/Vts| from

RMm

Mm

V

V

KB

B

BK

B

ts

td

1/1

/1

)(B

)),((B 2

22

222

*

*

Page 32: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 32Bruce SchummBaBar

Page 33: For the BaBar and Belle Collaborations Miami 2008 Topical Conference on Elementary Physics, Astrophysics, and Cosmology Fort Lauderdale, FL, Dec 16-21,

Miami 2008: b s(d) Transition Rates 33Bruce SchummBaBar