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Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR Spin Physics in NOMAD OUTLINE 1.Spin Problem of the Proton … for Pedestrians.

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Presentation on theme: "Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR Spin Physics in NOMAD OUTLINE 1.Spin Problem of the Proton … for Pedestrians."— Presentation transcript:

1 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Spin Physics in NOMAD OUTLINE 1.Spin Problem of the Proton … for Pedestrians  How to attack the problem?  Why strange hyperons?  Strange Particles Production 2.Other Spin Phenomena 1.NOMAD: experimental Observations and Analysis Procedure 2.Theoretical Description and Open Questions 3.Conclusions Introduction Data analysis

2 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Hyperon's Production and Polarization in Neutrino Nucleon Interactions OUTLINE 1.Spin Problem of the Proton … for Pedestrians  How to attack the problem?  Why strange hyperons?  Strange Particles Production 2.Other Spin Phenomena 1.NOMAD: experimental Observations and Analysis Procedure 2.Theoretical Description and Open Questions 3.Conclusions Introduction Data analysis

3 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Spin Problem of the Proton … for Pedestrians N S Spin being a relativistic object is qualitatively presented as a rotation of point-like particle… …circular charge flow is equivalent to a current circuit, thus a particle should have a magnetic moment Can we understand hadron’s magnetic moments which are bound states of u,d,s,… quarks? Yes! 1.Let us build QM wave functions of hadrons in terms of quarks 2.Given magnetic moment of each quark provides us an estimation of magnetic moment of a hadron 3.Compare to the data

4 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Building SU(6)=SU(3) F x SU(2) S non relativistic wave functions of octet baryons: p, n,  +,  0,  -,  0,  0,  - Cyclic permutations…)

5 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru  q = e q /2m q e q is quark charge m q is quark mass  q is quark spin operator Taking m u = m d = 336 MeV, m s = 510 MeV we can reasonable well describe the data: SU(6) prediction Magnetic momentformulavalueexperimentExp/SU(6) 1 1.028 1 0.91  0.004 1.12  0.02 0.87  0.01 1.33  0.06 1.05  0.12 Magnetic moment of a baryon (B) can be computed as:  (B) = QM operator of the hadron’s magnetic moment reads:  B =  q  q  q,

6 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Thus we can conclude that a non relativistic SU(6) model is adequate to describe the baryons magnetic moments through magnetic moments (proportional to the spin) of constituents quarks. It is natural to ask: “what is the quark’s contribution to the Proton Spin?”

7 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru 1.Evidence for point-like partons in the proton came from late 60s from SLAC e-p scattering. 2.R. Feynman formulated quark-parton model (QPM) of proton. 3.Gell-Mann created Quantum Color Dynamics (QCD) theory describing interactions between partons. How proton is made? …quarks, kinematics and all that k = (E,k) k’ = (E’,k’) Kinematic variables: In QPM x is a fraction of the proton momentum

8 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Deep inelastic cross-section is expressed via: Proton structure functionQuark (gluon) distributions in QPM F 1,F 2 unpolarized g 1,g 2 polarized q(x), G(x) unpolarized  q(x),  G(x), polarized Longitudinally polarized leptons off longitudinally polarized nucleon are to probe spin structure of the nucleon: g 1 (x,Q 2 ) = ½  i e 2 i  q(x) Experimentally measured: … known from hyperon  decays QCD corrections = [1/12 (  u-  d) + 1/36(  u+  d-2  s)]C ns + 1/9(  u+  d+  s)C s …proton spin carried by quarks

9 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Model independent Bjorken Sum Rule reads Corrections: QCD Final target mass Higher twist effects Theory Experiment 4% difference and well agrees within errors Bjorken Sum Rule is OK! Ellis-Jaffe Sum Rule (assuming  s=0 and exact SU(3) ) is violated… Quark’s contribution to the Proton Spin  u+  d+  s = 0.27  0.04 Naïve SU(6) gives:  u p = 4/3,  d p =-1/3, with  u+  d+  s = 1  s p = 0 Ellis-Jaffe expected:  u+  d+  s = 0.579 Theory Experiment …if  G=0

10 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru A.Efremov, O.Teryaev. G.Altarelli, G.Ross. R.Carlitz,J.Collins,A.Mueller showed that a possible gluon polarization gives:  q   q -  s /(2  )  G Proton Spin Sum Rule: ½ = ½(  u+  d+  s)+ orbital momentum of partons +  G  G=2 is enough to explain the data with  s=0 and  u+  d+  s = 0.27 … Important questions: 1.Are gluons polarized? 1.Are strange (and sea) quarks polarized? 1.Is there a spin problem for hyperons? “Prompt” measurement in (anti) neutrino (quasi)elastic scattering, strange hyperons polarization Today COMPASS and HERMES attack  G problem

11 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru  s can be measured directly in (anti)neutrino (quasi) elastic scattering… (by W.Alberico,S.Bilenky, C.Guinti) This is challenging experimentally! Strong force in 0 - channel ( ,  ) Negative proton strangeness should give a negative Lambda polarization in target fragmentation region  Polarization in DIS is sensitive indirect tool to probe  s Expected spin anti-correlation J.Ellis, et al. suggested a qualitative model for negative strangeness in the proton

12 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru R.L.Jaffe suggested to measure  polarization in the quark (current) fragmentation region. …if spin problem for proton then on the same foot spin problem for  and other hyperons. Naïve SU(6) predicts:  u=  d=0  s=1 Spin Problem for  predicts:  u=  d  -0.2 Contributions from  * and  are of great importance: Yields of strange hadrons and resonances has to be measured  polarization is being measured in: 1.e + e - at Z 0 pole (LEP) 2.Lepton nucleon DIS (E665,HERMES,COMPASS) 3.(anti) neutrino nucleon DIS(old bubble chambers, NOMAD) Why  ?   p  - weak decay provides information on  polarization vector

13 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Parity conservation forbids to produce longitudinally polarized Lambda hyperons if beam or target are unpolarized. However Lambda hyperons can be transversally polarized (orthogonal to the production plane). Unpolarized hadron hadron DIS Transverse polarization in HERMES  No transverse polarization found in old bubble chambers experiments  No transverse polarization found in e + e - at Z 0 pole

14 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Hyperon's Production and Polarization in Neutrino Nucleon Interactions OUTLINE 1.Spin Problem of the Proton … for Pedestrians  How to attack the problem?  Why strange hyperons?  Strange Particles Production 2.Other Spin Phenomena 1.NOMAD: experimental Observations and Analysis Procedure 2.Theoretical Description and Open Questions 3.Conclusions Introduction Data analysis

15 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Hyperon's Production and Polarization in Neutrino Nucleon Interactions OUTLINE 1.Spin Problem of the Proton … for Pedestrians  How to attack the problem?  Why strange hyperons?  Strange Particles Production 2.Other Spin Phenomena 1.NOMAD: experimental Observations and Analysis Procedure 2.Theoretical Description and Open Questions 3.Conclusions Introduction Data analysis

16 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Why Neutrinos? 1.are naturally polarized particles 2.interact with left handed quarks and right handed anti-quarks 3.interact with quarks and anti-quarks of specific flavor Neutrinos Thus… Neutrino beams are clean and power tools for the Spin Physics

17 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru A (short) history of neutrino detectors Anti- +p  e + +n e + +e -   15  s after: n+Cd   +... Reactor anti-Neutrino detection by Reines and Cowan (1953)

18 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru A (short) history of neutrino detectors Neutrinos come to CERN CDHS CHARM CHARMII BEBC CHORUS NOMAD

19 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru

20 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru NOMAD had wide neutrino beam mainly made of muon neutrinos NOMAD simulation chain

21 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru V 0 Mass resolution V 0 yields (in %) Yields in data are 40-60% below than default JETSET

22 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru V 0 integral yields in NOMAD compared to previous measurements

23 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru V 0 differential yields in NOMAD KsKs LambdaAnti Lambda x F = 2p L /W*

24 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Strange resonances in NOMAD Resonance/V 0 in data and default JETSET: Factor 1.5–2 difference Resume: Before doing a polarization Analysis  tune JETSET After JETSET tuning MC is well describing strange particles in NOMAD  ready for polarization study! K* + K* - *+*+ *-*- -- … by Artyom Chukanov (see his PhD)

25 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Polarization Analysis

26 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru General Results  polarization General Results  polarization _

27 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Lambda Polarization Vector in Target and “Current” Fragmentation Regions

28 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Strong dependence on W 2 Controversial theoretical descriptions at x F >0 …

29 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Longitudinal Lambda Polarization – Theoretical Description d d u u d d u d s u s _ q q q _ q _ J.Ellis et al. model Current direction Negatively polarized  d d u

30 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Spin transfer from: a)quark fragmentation  In SU(6) model  In Burkhardt-Jaffe model b)Di-quark fragmentation  J.Ellis et al. model  SU(6) model c)heavier strange hyperons decays Simulation chain: JETSET7.4 with NOMAD tuned parameters LEPTO6.1 (a bug corrected): adequately describes all unpolarized distributions in the NOMAD data Spin transfer from: a)quark fragmentation  In SU(6) model  In Burkhardt-Jaffe model b)Di-quark fragmentation  J.Ellis et al. model  SU(6) model c)heavier strange hyperons decays Spin transfer from: a)quark fragmentation  In SU(6) model  In Burkhardt-Jaffe model b)Di-quark fragmentation  J.Ellis et al. model  SU(6) model c)heavier strange hyperons decays Spin transfer from: a)quark fragmentation  In SU(6) model  In Burkhardt-Jaffe model b)Di-quark fragmentation  J.Ellis et al. model  SU(6) model c)heavier strange hyperons decays

31 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru qqq  Rank from diquark Rank from quark Tagging scheme for a hyperon Which contains: R qq =1 (A) R qq  1 & Rq  1 (B) R q =1 (A) R q  1 & Rqq  1 (B) Remnant diquarkStruck quark

32 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Conclusion: Current energies of all experiments in game today are too low to access quark fragmentation to hyperons… The diquark fragmentation is dominant

33 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Fixing free parameters of the model

34 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Compare to NOMAD data: Absolute value OK Functional Dependencies OK  Proton/neutron targets No

35 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Compare to HERMES (ep @27.5 GeV) Compare to E665 (  p @470 GeV) Small statistics yet… …Waiting new data by COMPAS, HERMES, NOMAD

36 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Transverse Polarization

37 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Transverse Polarization

38 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru d d u d u u d u u d u u q _ q d u u q _ q q q _ d u u q _ qq _ q L SzSz  s s _ PTPT PTPT A qualitative picture for polarization vs P T

39 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Before my conclusions… Starting from a hypothetical particle by Pauli, passing through an almost undetectable particle by Bethe and Pierls nowdays neutrinos provide a precise and powerful tool for Particle physics. NOMAD worked on: 1.Neutrino oscillation exclusion region 2.Strange particles production and polarization 3.Charm particles production, m c measurement 4.Diffractive physics 5.Bose-Einstein Correlations 6.Many Others… NOMAD is still working on: 1.Sin  W measurement 2.Quasi Elastic cross section and M A measurement 3.K * spin alignment 4.Strange Particles and Spin Physics in Neutral Currents (Z 0 boson exchange) 5.Penta Quark Search by Vladimir Lyubushkin by Artyom Chukanov

40 Pisa, INFN, October 21, 2003 Dmitry Naumov, LNP JINR naumov@nusun.jinr.ru Conclusions 1.Measurement of hyperon’s and meson’s yields is a milestone for Monte Carlo generators tuning… 2.Spin Problem of the Proton is still not resolved finally while much more better understood today. 1.COMPAS (CERN) and HERMES (DESY) attack this problem 2.NOMAD data favors that s quarks in the nucleon sea are negatively polarized… shadowing the valence quark spin of the nucleon 3.The transverse polarization of strange hyperons is clearly observed in NOMAD (for the first time in neutrino experiments). 1. the polarization originates in the string fragmentation 2.There is no good theory of this polarization 4.Many other exciting and top level things can be done within neutrino detector like the NOMAD and some of them are under investigation


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