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SM expectations on sin2 b(f 1 ) from b → s penguins. Chun-Khiang Chua Academia Sinica FPCP 2006 9 April 2006, Vancouver. Mixing induced CP Asymmetry. Bigi, Sanda 81. Quantum Interference. Both B 0 and B 0 can decay to f: CP eigenstate . If no CP (weak) phase in A: A= ±A
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SM expectations on sin2b(f1) from b → s penguins Chun-Khiang Chua Academia Sinica FPCP 2006 9 April 2006, Vancouver
Mixing induced CP Asymmetry Bigi, Sanda 81 Quantum Interference • Both B0 and B0 can decay to f: CP eigenstate. • If no CP (weak) phase in A: A=±A Cf=0, Sf=±sin2b Oscillation, eiDm t (Vtb*Vtd)2 =|Vtb*Vtd|2 e-i 2b Direct CPA Mixing-induced CPA
The CKM phase is dominating • The CKM picture in the SM is essentially correct: • WA sin2b=0.687±0.032 Thanks to BaBar, Belle and others…
New CP-odd phase is expected… • New Physics is expected • Neutrino Oscillations are observed • Present particles only consist few % of the universe density What is Dark matter? Dark energy? • Baryogenesis nB/ng~10-10 (SM 10-20) • It is unlikely that we have only one CP phase in Nature NASA/WMAP
The Basic Idea • A generic b→sqq decay amplitude: • For pure penguin modes, such as fKS, the penguin amplitude does not have weak phase [similar to the J/yKS amp.] • Proposed by Grossman, Worah [97] A good way to search for new CP phase (sensitive to NP).
The Basic Idea (more penguin modes) • In addition to fKS, (h’KS, p0KS, r0KS, wKS, hKS) were proposed by London, Soni [97](after the CLEO observation of the large h’K rate) • For penguin dominated CP mode with f=fCP=M0M’0, • cannot have color allowed tree (W± cannot produce M0 or M’0) • In general Fu should not be much larger than Fc or Ft • More modes are added to the list: f0KS, K+K-KS, KSKSKS Gershon, Hazumi [04], …
D sin2beff • To search for NP, it is important to measure the deviation of sin2beff in charmonium and penguin modes • Deviation NP • How robust is the argument? • What is the expected correction?
Sources of DS: • Three basic sources of DS: • VtbV*ts = -VcbV*cs-VubV*us =-Al2 +A(1-r)l4-ihAl4+O(l6)(also applies to pure penguin modes) • u-penguin (radiative correction): VubV*us(also applies to pure penguin modes) • color-suppressed tree • Other sources? • LD u-penguin, CA tree?
Corrections on DS • SinceVcbV*cs is real, a better expression is to use the unitary relation lt=-lu-lc(define Au≡Fu-Ft,Ac≡Fc-Ft;; Au,Ac: same order for a penguin dominated mode): • Corrections can now be expressed as (Gronau 89) • To know Cf and DSf, both rf and df are needed. ~0.4 l2
Several approaches for DS • SU(3) approach (Grossman, Ligeti, Nir, Quinn; Gronau, Rosner…) • Constraining |Au/Ac| through related modes in a model independent way • Factorization approach • SD (QCDF, pQCD, SCET) • FSI approach (Cheng, CKC, Soni) • Others
SU(3) approach for DS • Take Grossman, Ligeti, Nir, Quinn [03] as an example • Constrain |rf|=|luAu/lcAc| through SU(3) related modes b→s b→d O(l2)
An example |rh’Ks|≡ DS<0.22
More SU(3) bounds (Grossman, Ligeti, Nir, Quinn; Gronau, Grossman, Rosner) • Usually if charged modes are used (with |C/P|<|T/P|), better bounds can be obtained. (fK- first considered by Grossman, Isidori, Worah [98] using fp-, K*0K-) • In the 3K mode U-spin sym. is applied. • Fit C/P in the topological amplitude approach ⇒DS |DSf|<1.26 |rf| |Cf|<1.73 |rf| Gronau, Grossman, Rosner (04) Gronau, Rosner (Chiang, Luo, Suprun)
DS from factorization approaches • There are three QCD-based factorization approaches: • QCDF: Beneke, Buchalla, Neurbert, Sachrajda [see talk by Alex Williamson] • pQCD: Keum, Li, Sanda[see talk by Satoshi Mishima] • SCET: Bauer, Fleming, Pirjol, Rothstein, Stewart [see talk by Christian Bauer]
(DS)SD calculated from QCDF,pQCD,SCET • Most |DS| are of order l2, except wKS, r0KS (opposite sign) • Most theoretical predictions on DS are similar, but signs are opposite to data in most cases • Perturbative phase is small DS>0 • QCDF: Beneke[results consistent with Cheng-CKC-Soni] • pQCD: Mishima-Li • SCET: Williamson-Zupan (two solutions)
A closer look on DS signs and sizes Beneke, 05 small large B→V large small small (h’Ks) large (hKs) constructive (destructive) Interference in P of h’Ks (hKs)
Direct CP Violations in Charmless modes Expt(%) QCDF PQCD Different m, FF… Cheng, CKC, Soni, 04 With FSI ⇒ strong phases ⇒ sizable DCPV FSI is important in B decays What is the impact on DS
FSI effects on sin2beff(Cheng, CKC, Soni 05) • FSI can bring in additional weak phase • B→K*p, Kr contain tree Vub Vus*=|Vub Vus|e-ig • Long distance u-penguin and color suppressed tree
FSI effects in rates • FSIs enhance rates through rescattering of charmful intermediate states [expt. rates are used to fix cutoffs (L=m + r LQCD, r~1)]. • Constructive (destructive) interference in h’K0 (hK0).
FSI effects on direct CP violation • Large CP violation in the rK, wK mode.
FSI effect on DS • Theoretically and experimentally cleanest modes: h’Ks (fKs) • Tree pollutions are diluted for non pure penguin modes: wKS, r0KS
FSI effects in mixing induced CP violation of penguin modes are small • The reason for the smallness of the deviations: • The dominant FSI contributions are of charming penguin like. Do not bring in any additional weak phase. • The source amplitudes (K*p,Kr) are small (Br~10-6) compare with Ds*D (Br~10-2,-3) • The sources with the additional weak phase are even smaller (tree small, penguin dominate) • If we somehow enhance K*p,Kr contributions ⇒ large direct CP violation (AfKs). Not supported by data
Results in DS for scalar modes (QCDF) (Cheng-CKC-Yang, 05) • DS are tiny (0.02 or less): • LD effects have not been considered. Do not expect large deviation.
K+K-KS(L) and KSKSKS(L) modes • Penguin-dominated • KSKSKS: CP-even eigenstate. • K+K-KS: CP-even dominated, CP-even fraction: f+=0.91±0.07 • Three body modes • Most theoretical works are based on flavor symmetry. (Gronau et al, …) • We (Cheng-CKC-Soni) use a factorization approach
K+K-KS and KSKSKS decay rates • KS KS KS (total) rate is used as an input to fix a NR amp. (sensitive). • Rates (SD) agree with data within errors. • Central values slightly smaller. • Still have room for LD contribution.
It has a color-allowed b→u amp, but… b→s b→u • The first diagram (b→s transition) prefers small m(K+K-) • The second diagram (b→u transition) prefers small m(K+K0) [large m(K+K-)], not a CP eigenstate Interference between b→u and b→s is suppressed.
CP-odd K+K-KS decay spectrum • Low mKK: fKS+NR (Non-Resonance).. • High mKK: (NR) transition contribution.. b→s b→u
CP-even K+K-KS decay spectrum • Low mKK: f0(980)KS+NR (Non-Resonance). • High mKK: (NR) transition contribution. b→s b→u
K+K-KS and KSKSKS CP asymmetries • Could have O(0.1) deviation of sin2b in K+K-KS • It originates from color-allowed tree contribution. • Its contributions should be reduced. BaBar 05 • DS, ACP are small • In K+K-Ks: b→u prefers large m(K+K-) b→s prefers small m(K+K-), interference reduced small asymmetries • In KsKsKs: no b→u transition.
Conclusion • The CKM picture is established. However, NP is expected (Dmn, DM, nB/ng). • The deviations of sin2beff from sin2 = 0.6870.032 are at most O(0.1) in B0KS, KS, 0KS, ’KS, 0KS, f0KS, a0KS, K*0p0, KSKSKS. • The O(0.1) DS in B0→KKKS due to the color-allowed tree contribution should be reduced. A Dalitz plot analysis will be very useful. • The B0→h’KS, KS and B0→KSKSKS modes are very clean. • The pattern of DS is also a SM prediction. A global analysis is helpful. • Measurements of sin2beff in penguin modes are still good places to look for new phase(s) SuperB (d→0.1d).
A closer look on DS signs (in QCDF) M1M2: (B→M1)(0→M2)
Perturbative strong phases: penguin (BSS) vertex corrections (BBNS) annihilation (pQCD) • Because of endpoint divergences, QCD/mb power corrections in QCDF due to annihilation and twist-3 spectator interactions can only be modelled with unknown parameters A, H, A, H, can be determined (or constrained) from rates and Acp. • Annihilation amp is calculable in pQCD, but cannot have b→uqq in the annihilation diagram in b→s penguin.
Scalar Modes • The calculation of SP is similar to VP in QCDF • All calculations in QCDF start from the following projection: • In particular • All existing (Beneke-Neubert 2001) calculation for VP can be brought to SP with some simple replacements (Cheng-CKC-Yang, 2005).
FSI as rescattering of intermediate two-body state (Cheng, CKC, Soni 04) • FSIs via resonances are assumed to be suppressed in B decays due to the lack of resonances at energies close to B mass. • FSI is assumed to be dominated by rescattering of two-body intermediate states with one particle exchange in t-channel. Its absorptive part is computed via optical theorem: • Strong coupling is fixed on shell. For intermediate heavy mesons, • apply HQET+ChPT • Form factor or cutoff must be introduced as exchanged particle is • off-shell and final states are necessarily hard • Alternative: Regge trajectory, Quasi-elastic rescattering …
_ _ _ _ • For simplicity only LD uncertainties are shown here • FSI yields correct sign and magnitude for A(+K-) ! • K anomaly: A(0K-) A(+ K-), while experimentally they differ by 3.4 SD effects?[Fleischer et al, Nagashima Hou Soddu, H n Li et al.] • Final state interaction is important.
B B ﹣ _ _ _ • Sign and magnitude for A(+-) are nicely predicted ! • DCPVs are sensitive to FSIs, but BRs are not (rD=1.6) • For 00, 1.40.7 BaBar Br(10-6)= 3.11.1 Belle 1.6+2.2-1.6 CLEO Discrepancy between BaBar and Belle should be clarified.
Factorization Approach • SD contribution should be studied first. Cheng, CKC, Soni 05 • Some LD effects are included (through BW). • We use a factorization approach (FA) to study the KKK decays. • FA seems to work in three-body (DKK) decays CKC-Hou-Shiau-Tsai, 03. Color-allowed Color-suppressed
K+K-KS and KSKSKS (pure-penguin) decay amplitudes Tree Penguin
Factorized into transition and creation parts Tree Penguin
sin2beff in a restricted phase space of the K+K-KS decay • The corresponding sin2beff, with mKK integrated up to mKKmax. Could be useful for experiment. CP-even Full, excluding fKS