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Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal,...

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Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez- Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG report Valencia - SuperB Workshop VI
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Page 1: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Sharpening the Physics case for Charm at SuperB

D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi

Charm AWG reportValencia - SuperB Workshop VI

Page 2: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 2

From Bigi’s talk

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Page 3: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 3

Physics case for charm: search for New Physics

• The real certainty in charm physics is that CP, either in decay or in mixing or in interference, is the way to search for New Physics.

• At SuperB precision measurements of mixing should be considered as a tool for searches for CP.

Page 4: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 4

Mixing and CP toolkitD1,20 =p D0 ±q D0Mass eigenstates

flavor eigenstates:

A f = f H D0 A f = f H D0 Af

A f≠1

rm =qp ϕ f = arg

q

p

A fA f

⎝⎜

⎠⎟

CP in mixing CP in interference of mixing and decay

rm ≠1 ϕ f ≠ 0

CP in decay

Page 5: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 5

New Physics via CP

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Page 6: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 6

Mixing and CP violation observables

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Asl =q 4 − p 4

q 4 + p 4D0 → l−νX

D0 → CP

D0 → KSh+h−

D0 → K +π −

Page 7: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 7

Output from this workshop

Page 8: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 8

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Ikaros first homework

Page 9: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 9

– SuperKEK: besides lumi difference ~10x smaller, there is no possibility to run at threshold. Expected larger background, possible impact on systematics.

– LHCb: statistics not a problem. Systematics not evaluated in sensitivity studies, possibly limiting precise measurements. Decays with neutrals, neutrinos and Ks very challenging. Coherent production not possible.

– BESIII: Coherent production. 100x smaller lumi.Not possible time-dependent measurements.– CLEO-c: same considerations for BESIII. 26x smaller

data sample wrt BESIII.

Comparison with different running experiments

SuperB will offer the opportunity of:• Improving precision on almost all measurements.• Wider range of possible measurements.

Page 10: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 10

Question 1: sensitivity to charm mixing

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Estimates from CDR. Systematic uncertainties assumed to be kept under control. More comments later.

Page 11: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 11

Comparison with other experiments

Exp. sensitivities yCP(10-3) y’ (10-3) x’2 (10-4) cos

B-factories (2ab-1) 2-3 2-3 1-2 -

SuperB (75 ab-1) 0.4-0.5 0.7 0.3 -

CLEO-c (750 pb-1) 10 - 2-3 0.1-0.2

BESIII (20fb-1) 4 - 0.5-1 0.05

SuperB - 4 GeV (0.3 ab-1 or 2 month)

1-2 ? 0.5-1 0.01-0.02

LHCb 10fb-1 0.5(stat only)

0.9(stat only)

0.64(stat only)

-

Page 12: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 12

Question 2: running at (4S) vs DD threshold

• Charm events at threshold are very clean: pure DD, no additional fragmentation

• High signal/bkg ratio: optimal for decays with neutrinos.• Quantum Coherence: new and alternative CP violation

measurement wrt to (4S). Unique opportunity to measure D-D relative phase.

• Increased statistics is not an advantage running at threshold: cross-section 3x wrt 10GeV but luminosity 10x smaller.

• SuperB lumi at 4 GeV = 1035 cm-2s-1 to be compared with 1033 cm-2s-1 of BESIII. Possibility to improve BESIII results by sizeable amount in few months running.

• Time-dependent measurements at 4 GeV only possible at SuperB, to be assessed.

Page 13: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 13

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Page 14: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 14

Question 3: time dependent measurements at threshold

• Vertex resolution affected by increase of multiple scattering. D->Kπ decay mode as an example:

Average flight distance similar to vertex resolution t~

Error on lifetime (wrt perfect resolution)

≈ 2 + σ t

2

N= 2

τ

N

Page 15: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 15

Question 4: EPR correlations

• Clean aSL measurement. SL (D0l-νK+ vs D0l-

νK+) and also Hadronic (D0K+π- vs D0 K+π-). In later case only possible if mixing induced (no DCSD).

• Using CP tagged events it is a unique possibility to measure relative D-D strong phase.

• In 3-body decays (e.g. Kshh) allows to keep under control dalitz model systematics. To be assessed.

• Time-dependent measurement at threshold:– Time-dependent measurements can distinguish

between different types of CP violation. – Interest besides statistics to be assessed.

Page 16: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 16

Question 5: time dependent Dalitz plot

• Only method in literature sensitive to x, y directly. Sign of x is accessible.

• Golden channel if Dalitz model uncertainty is kept under control. Data at threshold, where evaluation of D-D relative phase is possible, are key ingredient.

• Need to understand if a Dalitz model independent measurement is feasible (as in the case of analysis) using data at threshold. Work started on this item.

Page 17: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 17

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Charm Physics Benchmarks

Page 18: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 18

Sensitivity to CP in mixingObservable sensitive to |q/p| (C=2) :

At threshold, time dependent asymmetry can reveal a new source of WS leptons (violation of SM selection rules).

Measurement can be performed:

• at threshold with D double-tagging. Clean environment, smaller systematics.

• at (4S) with D* tagging.

Asl =N++ −N−−

N++ + N−− =q 4 − p 4

q 4 + p 4

N ++ =D0 → l+νK −, N−− =D0 → l−νK + D0 =−,D0 =+, l± =±

Page 19: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 19

Sensitivity @ ’’(3770): (150/fb per month)

ACP=N++ - N--

N++ + N--

Sum of several exclusive channels: D0 K-π+, K-π+π0, K-π+π0, K-π+π+ π-, K-e+ν, K*-e+ν , K-µ+ν, K*-µ+ν, K+K-, π+π-

( (B) 22.7%)

Nmixed & tagged = ½N ’’ (x2+y2)/2 (B)2 1600 evts/month A 2.5%/month

(Only sl D0 K-l +ν A 9.5%/month )

4 months of running @ threshold (0.6 ab) A 1%

Advantage: closed kinematics

Page 20: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 20

Sensitivity @ (4S)

Advantage: tagged soft π* from D*Search for wrong sign leptons in sl decays D0 K-l +ν

Nws sl = 2NccPcD* π* B(D* D0π+) Kl B(D0 K-l +ν ) (x2+y2)/2 1350 evts/year

A 2.7%/year

5 years of running (75 ab) A 1%

But more bkg Possible to tag the other c

Page 21: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 21

Sensitivity to CP in interference between mixing and decay

Observable sensitive to (C=1 and C=2):

• Lifetime measurements in CP eigenstates: time distribution is exponential only approximately. Good approximation since mixing and CPV are small.

φ=argq

p

A fA f

⎝⎜

⎠⎟

2yCP =qp+

pq

⎝⎜⎞

⎠⎟±y( )cos φ( )−

qp−

pq

⎝⎜⎞

⎠⎟±x( )sin φ( )

2AΓ =qp−

pq

⎝⎜⎞

⎠⎟±y( )cos φ( )−

qp+

pq

⎝⎜⎞

⎠⎟±x( )sin φ( )

AΓ = D0 → CP( )− D0 → CP( ) D0 → CP( ) + D0 → CP( )

•Sensitivities with 75 ab-1: (cos) ~ 0.04%/y, (sin) ~ 0.03%/x

Page 22: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 22

Sensitivity to CP in decayEstimates from BaBar analysis to 75 ab-1:

•D0K+π- in time dependent analysis

•D0K+ K+, π- π+ in time independent analysis

• Dalitz plot analysis, time integrated (e.g. Kshh)

Strong phase variation over resonances of the Dalitz plot can improve the sensitivity to the asymmetry and help reducing systematic uncertainties.

AD =R D0 → K +π −( )−R D0 → K −π +( )R D0 → K +π −( ) + R D0 → K −π +( )

ACP =R D0 → K +K −( )−R D0 → K −K +( )R D0 → K +K −( ) + R D0 → K −K +( )

(AD)~0.4%

(ACP)~0.03%

Page 23: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 23

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Page 24: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 24

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Sensitivity to T violation ~ 0.04%with 75 ab-1

Page 25: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 25

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What theorist like to know

Page 26: Sharpening the Physics case for Charm at SuperB D. Asner, G. Batignani, I. Bigi, F. Martinez-Vidal, N. Neri, A. Oyanguren, A. Palano, G. Simi Charm AWG.

Valencia, Jan 7-15, 2008 Charm Working Group Report 26

Plans for the reportCP violation is the charm physics case for

SuperB:

• Refine estimates of sensitivities for CP violation.

• Evaluation of time-dependent measurements at threshold.

• Assess impact of threshold data on dalitz model uncertainty.

• Feasibility of dalitz model independent analysis for mixing and CP violation.


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