charm spectroscopy and rare decays
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Charm spectroscopy and rare decays Diego Milans , on behalf of the - PowerPoint PPT Presentation

Charm spectroscopy and rare decays Diego Milans , on behalf of the LHCb collaboration, including results from BaBar experiment LPNHE, Universit Pierre et Marie Curie, CNRS/IN2P3, Paris, France Flavor Physics and CP Violation 2013, Buzios,


  1. Charm spectroscopy and rare decays Diego Milanés , on behalf of the LHCb collaboration, including results from BaBar experiment LPNHE, Université Pierre et Marie Curie, CNRS/IN2P3, Paris, France Flavor Physics and CP Violation 2013, Buzios, Brazil

  2. Outline Heavy flavors factories ➡ Charm spectroscopy ➡ Excited D mesons @LHCb, LHCb-PAPER-2013-026 New ➡ Excited D s mesons @LHCb, JHEP1210(2012)151 ➡ Charm rare decays ➡ D 0 → μ + μ - @LHCb, LHCb-PAPER-2013-013 ➡ New D 0 → l + l’ - @BaBar, PRD86(2012)032001 ➡ D (s)+ → μ ∓ μ + π ± @LHCb, arXiv:1304.6365, Submitted to PRL ➡ D 0 → γγ @BaBar, PRD85(2012)091107(R) ➡ Conclusions ➡ D.Milanés, FPCP2013, Buzios, Brazil 2

  3. Heavy flavors factories L int ~3/fb pp collisions @7 and 8TeV Single arm spectrometer optimized for forward peaked heavy quark production @LHC. Large b b (~0.3mb) and c c production cross-sections (~1mb) Asymmetric e + e - B-factories @ Υ (4S) + scans in Υ (nS) e + e - @J/ ψ , ψ (2S), ψ (3770) c-factory, with the largest L int ~530/fb L int ~710/fb database on the charm σ (e+e- → c c )~1.3nb, >600M of c c pairs threshold. L int ~3/fb D.Milanés, FPCP2013, Buzios, Brazil 3

  4. Excited D states Charm spectroscopy provides a Godfrey & Isgur, PRD32(1985)189 powerful test for quark model predictions in the SM. D*(2760) → D π Many charmed states predicted in D(2750) → D* π the 80’s have not been found experimentally. Often discrepancies between prediction an measurements. Well stablished states Observed in B decays by B-factories New predictions account for Observed by BaBar in inclusive D ( * ) π possible bound states or unusual production PRD82(2010)111101 q q ’ mixtures ➟ BaBar observed D(2550) 0, D*(2600) 0 , D(2750) 0 , D*(2760) 0 and the isospin partners D*(2600) + and D*(2760) + , to be confirmed. ➟ Discrepancies between prediction and experiment up to ~50MeV. D.Milanés, FPCP2013, Buzios, Brazil 4

  5. Excited D s states Charm spectroscopy provides a BaBar, PRD80(2009)092003 Belle, PRL100(2008)092001 powerful test for quark model predictions in the SM. Many charmed states predicted in the 80’s have not been found experimentally. Often discrepancies between prediction an measurements. New predictions account for possible bound states or unusual q q ’ mixtures ➟ Large discrepancy between predictions* and experiment for D s0 *(2317) and D s1 (2460) ➟ High mass states observed in D (*) π (BaBar) and 3-body B decays (Belle). ➟ Controversial spin assignment for D sJ (2860). Angular analysis supports J P =3 - , but incompatible with the branching fraction ratio expectation. Overlap of states? *Godfrey, Isgur,PRD32(1985)189 Godfrey, Kokosky, PRD43(1991)1679 Isgur,Wise,PRL66(1991)1130 D.Milanés, FPCP2013, Buzios, Brazil 5

  6. Excited D (s) mesons at LHCb ➡ Analysis of inclusively prompt produced D (*) h pairs, using 1/fb sample collected during 2011 data taking ➡ Excited D mesons New ➡ preliminary results, LHCb-PAPER-2013-026 ➡ D 0 [K - π + ] π + , D + [K - π + π + ] π - , D* + [D 0 π + ] π - ➡ Excited D s mesons ➡ JHEP1210(2012)151 ➡ D 0 [K - π + ] Κ + , D + [K - π + π + ]K S [ π + π - ] ➡ D meson candidates reconstructed in CF modes ➡ Similar strategy used in both analyses D.Milanés, FPCP2013, Buzios, Brazil 6

  7. Selection of excited D (s) states i.e D 0 h + final state K - ➦ Large combinatorial background from random tracks produced in the D 0 IP primary vertex. Main source π + of systematic uncertainty ➦ Negligible contribution Primary vertex from fake D, giving their high Excited D (s) purity (>95%) production and decay h + Global selection criteria LHCb-PAPER-2013-026 ➟ Tracks and vertices quality ➟ Large D flight length Preliminary ➟ Large IP wrt PV for D daughter tracks M(D 0 ) ➟ Small IP wrt PV for the prompt track and D σ ~9 Μ eV ➟ Tight particle ID criteria in the prompt track ➟ Large cos θ . Reduction of about 90% of combinatorial background and wrong mass hypothesis tracks. D.Milanés, FPCP2013, Buzios, Brazil 7

  8. The Dh spectra D 1 (2420) D 1 (2420) → D*[D π ,D γ ] π partially reco D 2 *(2460) → D*[D π ,D γ ] π partially reco LHCb-PAPER-2013-026 D 2 *(2460) Preliminary Preliminary Preliminary M(D 0 π + ) M(D + π - ) M(D* + π - ) WS WS WS D s2 *(2573) → Already several contributions in D s1 (2536) → D*[D π ,D γ ]K partially reco the high mass tails are observed → Signal described with Breit-Wigner M(D + K S ) M(D 0 K + ) distributions → Largest component is bkg (and so systematic). Bkg described with empiric piece-wise function made of exponentials times a threshold function, in D π , while for DK a linear combination of Chebyshev polynomials is used JHEP1210(2012)151 D.Milanés, FPCP2013, Buzios, Brazil 8

  9. D* π angular analysis New LHCb-PAPER-2013-026 Split of the D* π sample in ranges of the helicity angle Preliminary Enhanced natural parity, |cos θ H |<0.5, J P =0 + ,1 - ,2 + ,... Enhanced unnatural parity, |cos θ H |>0.5, J P =0 - ,1 + ,2 - ,... Components found in the high mass tail D J *(2650) D J *(2760) D J (2580) D J (2740) D J (3000) D* π |cos θ H |<0.5 Bkg subtracted LHCb Preliminary Preliminary M(D* π ) D* π |cos θ H |>0.5 D 1 (2420) 0 LHCb Preliminary D 2* (2460) 0 D.Milanés, FPCP2013, Buzios, Brazil 9

  10. D* π angular analysis New Flat efficiency in cos θ . LHCb Preliminary Spin-parity analysis in bins of the 1+hcos 2 θ helicity angle. sin 2 θ For well stablished states, data is well described with the expected hypothesis, D 1 (2420) a J P =1 + , and D 2 *(2460) a J P =2 + state. Natural parity assignment confirmed for D J *(2650) 0 and D J *(2760) 0 . Unnatural parity assignment confirmed for D J (2580) 0 , D J (2740) 0 and suggested for D J (3000) 0 . LHCb-PAPER-2013-026 D.Milanés, FPCP2013, Buzios, Brazil 10

  11. D π spectra New Preliminary Preliminary D J *(2760) 0 D J *(3000) 0 D J *(2760) + D J *(3000) + M(D + π - ) M(D 0 π + ) ➟ Natural parity states LHCb-PAPER-2013-026 ➟ An iterative separate fit between both spectra, using as input information from D* π ➟ Feed-down from partially reconstructed structures (Missing π , γ ). Yields for high mass feed- downs are scaled from yields extracted for large structures in D* π to the same type of feed- down in D π , D 1 (2420) and D 2 *(2460). Shape extracted from MC simulation. ➟ High mass populated with D J *(2760) 0,+ and D J *(3000) 0,+ (natural parity). D J *(2650) 0,+ very hard to extract given feed-downs D.Milanés, FPCP2013, Buzios, Brazil 11

  12. DK spectra JHEP1210(2012)151 Simultaneous fit to D + K S and D 0 K + samples D s1 *(2700) + D s1 *(2700) + D sJ *(2860) + D sJ *(2860) + M(D + K S ) M(D 0 K + ) Bkg subtracted Bkg subtracted M(D + K S ) M(D 0 K + ) D.Milanés, FPCP2013, Buzios, Brazil 12

  13. Summary on spectroscopy Largest systematic uncertainties from bkg model. Different models used as well as toy MC. Results have been largely cross-checked. New LHCb Preliminary LHCb-PAPER-2013-026 Unnatural parity Natural parity Seen only in D* π , 1 - 2S D 1 (2618) Ν atural parity Seen by BaBar, unnatural parity 0 - Unnatural parity, 1 - like 1D D 1 (2796) NEW compatible with unnatural par. Natural parity Natural parity, 2 - like 1D D 2 (2801) NEW Natural parity Natural parity, 2 - like 1D D 2 (2801) NEW First observation of D s1 *(2700) + and D sJ *(2860) + in hadronic collisions. Resonances observed in BaBar and Belle have been confirmed. All results within agreement. Additional D*K analysis needed to rule out spin parity puzzle on D sJ *(2860) + state. LHCb, JHEP1210(2012)151 D.Milanés, FPCP2013, Buzios, Brazil 13

  14. Charm rare decays ➟ Many charm decays are forbidden or highly suppressed in the SM. Usually FCNC, LFV, LV, BV decays. ➟ Very rare decays help to constrain effects from physics BSM ➟ BSM models enhance BF of some of these decays Experimental 90% CL upper limits on branching fractions HFAG arXiv:1207.1158 LF L L FCNC FCNC FCNC D + D 0 D s+ D.Milanés, FPCP2013, Buzios, Brazil 14

  15. D 0 → l + l - l + l + l _ _ l - l - Leading non-perturbative long SM prediction* l + distance term. BF(D 0 → e + e - )~10 -23 BF(D 0 → µ + µ - )~10 -13 l + Much smaller BF than current experimental sensitivity (~10 -7 ). FCNC process GIM and helicity ~10 -5 BF(D 0 → γγ ) l - suppressed in SM Some R-parity violating SUSY models enhance BF(D 0 → µ + µ - ) up to current experimental levels, tree decay diagrams via squark exchange. Window of several orders of for NP. Great scenario for SUSY searches, exploited prior 2010 by many experiments http://www.slac.stanford.edu/xorg/hfag/charm/ICHEP12/Rare/rare_d0.html *Burdman, et.al, Phys. Rev. D 66, 014009 (2002). D.Milanés, FPCP2013, Buzios, Brazil 15

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