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WPCF 2007 - Aug. 1-3, 2007 1 Conservation Laws in low-multiplicity collisions Zbigniew Chajęcki and Michael A. Lisa The Ohio State University
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WPCF 2007 - Aug. 1-3, 2007 2 Outline Introduction / Motivation –Non-femtoscopic correlations in low-multiplicity collisions : OPAL, NA22, STAR, … * data features not under control: Energy-momentum conservation? Analytic calculation of Energy and Momentum Conservation Induced Correlations for –single particle spectra –two-particle correlations Experimentalists’ recipe: Fitting correlation functions –M inv correlation function & background subtraction –V 2 –Two-particle correlations –Resonance contribution to non-femtoscopic correlations - (π +,π - ) –(π +,π - ) correlations in p+p( p) at 200 GeV collisions from PYTHIA Conclusion
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WPCF 2007 - Aug. 1-3, 2007 3 Non-femtoscopic correlations : OPAL OPAL, CERN-PH-EP/2007-025 (submitted to Eur. Phys. J. C.) 1D projections of 3D CF Femtoscopic correlations should go to the constant number at large Q (no directional dependence!) Q x <0.2 GeV/c
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WPCF 2007 - Aug. 1-3, 2007 4 Non-femtoscopic correlations : NA22 NA22, Z. Phys. C71 (1996) 405 1D projections of 3D CF
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WPCF 2007 - Aug. 1-3, 2007 5 Non-femtoscopic correlations : STAR d+Au: peripheral collisions STAR preliminary Non-femtoscopic q-anisotropic behaviour at large |q| does this structure affect femtoscopic region as well? Q x <0.12 GeV/c STAR, NPA 774 (2006) 599 Clear interpretation clouded by data features
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WPCF 2007 - Aug. 1-3, 2007 6 Spherical harmonic decomposition Q OUT Q SIDE Q LONG Q : [0,2 ] : [0, ] Z.Ch., Gutierrez, Lisa, Lopez-Noriega, nucl-ex/0505009
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WPCF 2007 - Aug. 1-3, 2007 7 Non-femtoscopic correlations : STAR Baseline problem is increasing with decreasing multiplicity STAR preliminary
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WPCF 2007 - Aug. 1-3, 2007 8 MC simulations ‘ad-hoc’ parameterizations OPAL, NA22, … Common approaches to „remove” non-femtoscopic correlations A possibility: energy-momentum conservation? –must be there somewhere! –but how to calculate / model ? (Upon consideration, non-trivial...) “zeta-beta” fit by STAR [parameterization of non-femtoscopic correlations in A lm ’s]
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WPCF 2007 - Aug. 1-3, 2007 9 GenBod Phase-Space Event Generator
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WPCF 2007 - Aug. 1-3, 2007 10 GenBod: Phase-space sampling with energy/momentum conservation F. James, Monte Carlo Phase Space CERN REPORT 68-15 (1 May 1968) Sampling a parent phasespace, conserves energy & momentum explicitly –no other correlations between particles ! Events generated randomly, but each has an Event Weight WT ~ probability of event to occur P conservation Induces “trivial” correlations (i.e. even for M=1) Energy-momentum conservation in n-body system
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WPCF 2007 - Aug. 1-3, 2007 11 N=9, K =0.5 GeV, LCMS Frame - no cuts The shape of the CF is sensitive to: kinematic cuts frame particle multiplicity total energy : √s
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WPCF 2007 - Aug. 1-3, 2007 12 Findings Energy and Momentum Conservation Induced Correlations (EMCICs) “resemble” our data so, EMCICs... on the right track... But what to do with that? –Sensitivity to s, multiplicity of particles of interest and other particles –will depend on p 1 and p 2 of particles forming pairs in |Q| bins risky to “correct” data with Genbod... Solution: calculate EMCICs using data!! –Danielewicz et al, PRC38 120 (1988) –Borghini, Dinh, & Ollitraut PRC62 034902 (2000) we generalize their 2D p T considerations to 4-vectors
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WPCF 2007 - Aug. 1-3, 2007 13 k-particle distributions w/ phase-space constraints single-particle distribution w/o P.S. restriction k-particle distribution (k<N) with P.S. restriction observed P - total 4-momentum
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WPCF 2007 - Aug. 1-3, 2007 14 Central Limit Theorem k-particle distribution in N-particle system For simplicity we will assume that all particles are identical (e.g. pions) and that they share the same parent distribution (same RMS of energy/momentum) Then, we can apply CLT (the distribution of averages from any distribution approaches Gaussian with increase of N) Can we assume that E and p are not correlated ?
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WPCF 2007 - Aug. 1-3, 2007 15 E - p correlations?
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WPCF 2007 - Aug. 1-3, 2007 16 EMCICs in single-particle distribution What if all events had the same “parent” distribution f(p), and all multiplicity (centrality) dependence of spectra was due just to loosening of P.S. restrictions as N increased?
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WPCF 2007 - Aug. 1-3, 2007 17 EMCIC’s in spectra For N
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WPCF 2007 - Aug. 1-3, 2007 18 EMCICs: Ratio of particle spectra Phys. Rev. D 74 (2006) 032006p+p @ 200GeV, STAR p T spectra from GenBod Simulations: Ratio of p T spectra for N=9 and N=18. Ratio of p T spectra in p+p@STAR for the lowest and the highest multiplicity events
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WPCF 2007 - Aug. 1-3, 2007 19 k-particle correlation function Dependence on “parent” distrib f vanishes, except for energy/momentum means and RMS 2-particle correlation function (1 st term in 1/N expansion) 2-particle correlation function
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WPCF 2007 - Aug. 1-3, 2007 20 2-particle CF (1st term in 1/N expansion) “The p T term” “The p Z term” “The E term” Names used in the following plots
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WPCF 2007 - Aug. 1-3, 2007 21 EMCICs An example of EMCICs: Effect of varying multiplicity Same plots as before, but now we look at: p T ( ), p z ( ) and E ( ) first-order terms full ( ) versus first-order ( ) calculation simulation ( ) versus first-order ( ) calculation
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WPCF 2007 - Aug. 1-3, 2007 22 N=9, K =0.9 GeV, LabCMS Frame - no cuts
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WPCF 2007 - Aug. 1-3, 2007 23 N=18, K =0.9 GeV, LabCMS Frame - no cuts
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WPCF 2007 - Aug. 1-3, 2007 24 Findings CF from GenBod (as well as EMCICs) depends on –multiplicity –frame –energy of the collisions first-order and full calculations agree well for N>9 –will be important for “experimentalist’s recipe” Non-trivial competition/cooperation between p T, p z, E terms –all three important p T1 p T2 term does affect “out-versus-side” (A 22 ) p z term has finite contribution to A 22 (“out-versus-side”) calculations come close to reproducing simulation for reasonable (N-2) and energy
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WPCF 2007 - Aug. 1-3, 2007 25 N =12,N K =3,N p =3, K =0.9 GeV, LCMS Frame - no cuts
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WPCF 2007 - Aug. 1-3, 2007 26 The Experimentalist’s Recipe Fitting formula: - average of X over # of pairs for each Q-bin
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WPCF 2007 - Aug. 1-3, 2007 27 EMCIC’s FIT: N=18, K =0.9GeV, LCMS
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WPCF 2007 - Aug. 1-3, 2007 28 The Complete Experimentalist’s Recipe or any other parameterization of CF 9 fit parameters - 4 femtoscopic - normalization - 4 EMCICs Fit this …. or image this …
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WPCF 2007 - Aug. 1-3, 2007 29 M inv distribution w/ background subtraction N=18
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WPCF 2007 - Aug. 1-3, 2007 30 EMCICs contribution to v 2 for v 2 n=2 no contribution to v 2 from 1/N term contribution to v 2 from 1/N 2 term contribution to v 2 from 1/N 3 term
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WPCF 2007 - Aug. 1-3, 2007 31 Non-id correlations (Resonance contrib.)
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WPCF 2007 - Aug. 1-3, 2007 32 Non-id correlations (PYTHIA@200 GeV)
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WPCF 2007 - Aug. 1-3, 2007 33 Summary understanding particle spectra, two-particle correlations, v 2, resonances in small systems –important physics-wise –should not be attempted until data fully under control Restricted P.S. due to energy-momentum conservation –sampled by GenBod event generator –generates EMCICs [femtoscopy : quantified by A lm ’s] –stronger effects for small multiplicities and/or s Analytic calculation of EMCICs –k-th order CF given by ratio of correction factors –“parent” only relevant in momentum variances –first-order expansion works well for N>9 –non-trivial interaction b/t p T, p z, E conservation effects Physically correct “recipe” to fit/remove EMCICs [femtoscopy] –4 new parameters, determined @ large |Q|
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WPCF 2007 - Aug. 1-3, 2007 34 Thanks to: Alexy Stavinsky & Konstantin Mikhaylov (Moscow) [suggestion to use Genbod] Jean-Yves Ollitrault (Saclay) & Nicolas Borghini (Bielefeld) [original correlation formula] Adam Kisiel (Warsaw) [don’t forget energy conservation] Ulrich Heinz (Columbus) [validating energy constraint in CLT] Mark Baker (BNL) [local momentum conservation] Dariusz Miskowiec (GSI) [multiply (don’t add) correlations]
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