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Flavor physics in the LHC era Zoltan Ligeti Lawrence Berkeley Lab - PowerPoint PPT Presentation

Flavor physics in the LHC era Zoltan Ligeti Lawrence Berkeley Lab Flavor physics in the LHC era Zoltan Ligeti Lawrence Berkeley Lab Introduction Current status: sizable NP contributions allowed Some key probes at LHCb and


  1. Flavor physics in the LHC era Zoltan Ligeti Lawrence Berkeley Lab

  2. Flavor physics in the LHC era Zoltan Ligeti Lawrence Berkeley Lab • Introduction • Current status: sizable NP contributions allowed • Some key probes at LHCb and super-(KEK) B • High- p T flavor physics • Conclusions

  3. Why is flavor physics interesting? • SM flavor problem: hierarchy of masses and mixing angles; why ν ’s are different • Empirical evidence that SM is incomplete: baryon asymmetry, dark matter, neutrino mass — at least two related to flavor • NP flavor problem: TeV scale (hierarchy problem) ≪ flavor & CPV scale ǫ K : ( s ¯ ∆ m B : ( b ¯ d ) 2 d ) 2 s ) 2 ∆ m Bs : ( b ¯ ∼ 10 4 TeV , ∼ 10 3 TeV , ∼ 10 2 TeV ⇒ Λ > ⇒ Λ > ⇒ Λ > Λ 2 Λ 2 Λ 2 – Many extensions of the SM have new sources of CP and flavor violation – The observed baryon asymmetry of the Universe requires CPV beyond the SM Not necessarily in flavor changing processes, nor necessarily in quark sector Flavor suppression destroys KM baryogenesis; flavor matters for leptogenesis • Flavor sector can be tested a lot better, many NP models have observable effects ZL — p.1

  4. The name of the game in the LHC era • The question has been who sees NP first; once it’s seen, how to understand it? [Assume the LHC sees more than a Higgs ... ] • Concentrate on flavor physics topics where sensitivity can improve significantly (by an order of magnitude, or at least a factor of many) – Skip B → X s γ rate, near “hitting the theory wall” (best bound on many models) – ... some tension between sin 2 β and | V ub | [emphasized, e.g., by UTfit] – ... > 3 σ tension between LQCD f D s and D + s → ℓ + ν [Dobrescu & Kronfeld, arXiv:0803.0512] – Many measurements with complementary sensitivity will improve a lot – If all flavor effects < 1% in your favorite model (what is it?), I’ll have little to say • Lack of a “flavor theory” — there isn’t an obviously right / natural way for TeV-scale NP to duplicate GIM and CKM suppressions ZL — p.2

  5. SUSY contributions to K 0 – K 0 mixing � 1 TeV � 2 � ∆ ˜ � 2 • (∆ m K ) SUSY m 2 � � (∆ m K ) exp ∼ 10 4 12 ( K d L ) 12 ( K d Re R ) 12 m 2 m ˜ ˜ K d L ( R ) : mixing in gluino couplings to left-(right-)handed down quarks and squarks Constraint from ǫ K : 10 4 Re � � ⇒ 10 6 Im � � ( K d L ) 12 ( K d ( K d L ) 12 ( K d R ) 12 R ) 12 • Classes of models to suppress each factors (i) Heavy squarks: ˜ m ≫ 1 TeV (e.g., split SUSY) m 2 (e.g., gauge mediation) (ii) Universality: ∆ m 2 D ≪ ˜ Q, ˜ ˜ (iii) Alignment: | ( K d L,R ) 12 | ≪ 1 (e.g., horizontal symmetries) • All SUSY models incorporate some of the above ZL — p.3

  6. Where are we now?

  7. The standard model CKM fit • Very impressive accomplishment • The level of agreement between the various measurements is often misinterpreted • Plausible TeV scale NP scenarios, consistent with all low energy data, w/o minimal flavor violation (MFV) • CKM is inevitable; the question is not if it’s correct, but is it sufficient? ZL — p.4

  8. New Physics in FCNC processes • Mixing × ⇒ AND? OR Simple parameterization for each neutral meson: M 12 = M SM 12 (1 + he 2 iσ ) • Penguin decays γ γ b R s L b R s L t t × ⇒ AND? OR W H − Many operators for b → s transitions — no simple parameterization of NP • V td, ts only measurable in loops; likely also subleading couplings of new particles • Isolating modest NP contributions requires many measurements Compare NP-independent (tree) with NP-dependent (loop) processes ZL — p.5

  9. Constraints on NP in B 0 d mixing • Overconstraining (“redundant”) measurements are crucial to bound new physics ρ, η determined from (effectively) tree level and loop-induced pro- cesses, separately M 12 = M SM 12 (1 + he 2 iσ ) aOnly the SM-like region is allowed, NP ∼ SM is still allowed; Think “MFV”: h ∼ (4 πv/ Λ flav . ) 2 ; is Λ flav . ≫ Λ EWSB ? even in the presence of NP in mixing • 10 – 20% non-SM contributions to most loop-mediated transitions are still possible ZL — p.6

  10. B s mixing — ∆ m s • B 0 s – B 0 s oscillate 25 times on average before they decay — challenge to measure -1 CDF Run II Preliminary L = 1.0 fb 2 Amplitude -1 data ± 1 σ 95% CL limit 17.2 ps 1.5 -1 1.645 σ sensitivity 31.3 ps data 1.645 ± σ 1 data 1.645 (stat. only) ± σ 0.5 0 -0.5 -1 -1.5 -2 0 5 10 15 20 25 30 35 -1 ∆ m [ps ] s • ∆ m s = (17 . 77 ± 0 . 10 ± 0 . 07) ps − 1 √ B s Largest uncertainty: ξ = f Bs √ [CDF , hep-ex/0609040] f Bd B d Uncertainty σ (∆ m s ) = 0 . 7% is already Lattice QCD: ξ = 1 . 24 ± 0 . 04 ± 0 . 06 smaller than σ (∆ m d ) = 0 . 8% ZL — p.7

  11. B s mixing phase — sin 2 β s • Next key measurement: time dep. CP asymmetry in B s → ψφ (as clean as sin 2 β ) In the SM: β s = arg( − V ts V ∗ tb /V cs V ∗ cb ) = 0 . 019 ± 0 . 001 • CDF & DØ disfavor large negative values: Testing a “squashed” UT: 0.10 CKM sol. w/ cos 2 β < 0 excluded area has CL > 0.95 CDF (no strong phase constraint & CL based on MC) (excl. at CL > 0.95) f i t t e r ε γ D0 (strong phase constraint & CL based on likelihood) K Pheno 2008 CKM fit sin 2 β 0.05 1.0 0.8 β s s 0.00 η 0.6 V α α 1 - CL ub m ∆ d 0.4 m & m ∆ ∆ -0.05 s d excluded at CL > 0.95 γ 0.2 CKM f i t t e r CDF, arXiv:0712.2397; DØ, arXiv:0802.2255 ε Pheno 2008 K -0.10 0.0 -0.10 -0.05 0.00 0.05 0.10 0.0 0.5 1.0 1.5 2.0 2.5 3.0 ρ 2 β (rad) s s Averaging complicated due to different assumptions, hopefully fixed by summer ZL — p.8

  12. The D meson system • Complementary to K, B : CPV, FCNC both GIM & CKM suppressed ⇒ tiny in SM – 2007: signal for mixing > 5 σ [HFAG combination] – Only meson mixing generated by down-type quarks (SUSY: up-type squarks) a ∼ 10 − 2 Γ , since doubly- – SM suppression: ∆ m D , ∆Γ D < Cabibbo-suppressed and vanish in flavor SU (3) limit – CPV (mixing or direct) ≫ 10 − 3 would be sign of NP ( x = ∆ m/ Γ , y = ∆Γ / 2Γ ) – To do: Precise values of ∆ m and ∆Γ ? To do: Is CPV absent in mixing and decays? (not yet known if | q/p | ≃ 1 ) • Particularly interesting for SUSY: ∆ m D and ∆ m K ⇒ if first two squark doublets are within LHC reach, they must be quasi-degenerate (alignment alone not viable) ZL — p.9

  13. The old/new B → Kπ puzzle ( T ) ( P ) • Q : new physics in CPV in B → Kπ ? A K + π − = − 0 . 097 ± 0 . 012 ( P + T ) ( C ) ( P ew ) A K + π 0 = 0 . 050 ± 0 . 025 ( P + T + C + A + P ew ) What is the reason for large difference? A K + π 0 − A K + π − = 0 . 147 ± 0 . 028 ( > 5 σ ) (Annihilation not shown) [Belle, Nature 452, 332 (2008)] SCET / factorization predicts: arg ( C/T ) = O (Λ QCD /m b ) and A + P ew small • A : huge fluctuation, breakdown of 1 /m exp., missing something subtle, new phys. • No similarly transparent problem with branching ratios, e.g., Lipkin sum rule looks Γ( B − → π 0 K − ) + ¯ Γ( B 0 → π 0 K 0 ) OK by now: ¯ 2 = 1 . 07 ± 0 . 05 (should be near 1 ) Γ( B − → π − K 0 ) + ¯ ¯ Γ( B 0 → π + K − ) ZL — p.10

  14. Forthcoming progress

  15. Questions we hope to gain insights on • The 3rd generation may differ from the 1st and 2nd by more than we know so far Large top Yukawa ⇒ maybe non-universal coupling to EWSB and NP sector Want to compare 3rd–1st and 3rd–2nd generation data with precision kaon data • Many processes have different sensitivities to various NP scenarios In SM: CPV only in flavor changing, charged current interactions of quarks With NP: possible in flavor diagonal processes, neutral currents, in lepton sector Does new physics give rise to operators forbidden (highly suppressed) in the SM? s σ µν F µν P R b vs. O ′ s σ µν F µν P L b E.g., O 7 = ¯ 7 = ¯ • Try to distinguish NP scenarios: One / many sources of CPV? Only in CC inter- actions? Couples to up / down sector? 3rd / all generations? ∆ F = 2 and / or 1 ? ZL — p.11

  16. sin 2 β eff , α , γ — large improvements possible B →ρπ (WA) sin(2 β eff ) ≡ sin(2 φ e ff ) vs C CP ≡ -A CP H F AG H F A G 1.2 CK M 1 B →ρρ (WA) COMBINED f i t t e r LP 2007 LP 2007 C CP ≡ -A CP B →ππ (WA) PRELIMINARY 1 0.8 0.8 0.6 1 – CL 0.6 0.4 CKM fit no α meas. in fit 0.2 0.4 0 0.2 b → ccs φ K 0 -0.2 η′ K 0 0 0 20 40 60 80 100 120 140 160 180 K S K S K S π 0 K S -0.4 α (deg) ρ 0 K S ω K S CKM D(*) K(*) GLW + ADS WA -0.6 f 0 K 0 f i t t e r D(*) K(*) GGSZ Combined π 0 π 0 K S FPCP 07 K + K - K 0 Full Frequentist treatment on MC basis -0.8 1 -0.4 -0.2 0 0.2 0.4 0.6 0.8 1 sin(2 β eff ) ≡ sin(2 φ e ff ) 0.8 1 1 - CL 1 - CL Contours give -2 ∆ (ln L) = ∆χ 2 = 1, corresponding to 60.7 % CL for 2 dof 0.6 • E.g., S ψK − S φK = 0 . 29 ± 0 . 17 ; also for α & γ : 0.4 want ∼ 10 × smaller error ⇒ ∼ 100 × more data CKM fit 0.2 no meas. in fit γ • Need both LHCb and e + e − super B factory 0 0 0 20 20 40 40 60 60 80 80 100 100 120 120 140 140 160 160 180 180 γ γ (deg) (deg) ZL — p.12

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