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Imaging in Heavy-Ion Collisions D.A. Brown, A. Enokizono, M. Heffner, R. Soltz (LLNL) P. Danielewicz, S. Pratt (MSU) RHIC/AGS Users Meeting 21 June 2005 This work was performed under the auspices of the U.S. Department of Energy by University of California, Lawrence Livermore National Laboratory under Contract W-7405-Eng-48. Talk Outline: Background Nontrivial test problem Inverting a 3d correlation Implications for HBT Puzzle CorAL Status
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The Koonin-Pratt Formalism We will invert to get S(r) directly The pair’s final state wave- function, we can compute this if we know the interaction. This is the kernel K(q,r). The source function, it gives the probability of producing a pair a distance r apart in the pair CM frame Source function related to emission function: We work in Bertsch-Pratt coords., in pCM
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3d HBT at RHIC Boost may have interesting observable consequence (Rischke, Gyulassy Nucl. Phys. A 608, 479 (1996)): If there is a phase-transition, hydro evolution will slow in mixed phase. Will lead to long-lived source Huge difference in Outward/Sideward radii R out /R side == 1! (in LCMS) Experiment analysis wrong? Coulomb correction? Theory screwed up? Interpretation confused? Instant freeze-out? Gaussian fits?
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The Test Problem, part 1 T = 50 MeV -- source temperature R x = R y = R z = 4 fm = 20 fm/c, ballpark of lifetime (23 fm/c) Emission function is Gaussian with finite lifetime, in lab frame: (lab pair CM boost) + == non-Gaussian source!
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The Test Problem, part 2 Combine with + + kernel to get correlation using Scott Pratt’s CRAB code
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Breaking Problem into 1d Problems Where Expand in Ylm’s and Legendre polynomials:
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Breaking Up Problem, cont.
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Imaging Summary Use CorAL version 0.3 * Source radial terms written in Basis Spline representation – knots set using Sampling Theorem from Fourier Theory – use 3rd degree splines * Use full Coulomb wavefunction, symmetrized * Use generalized least-square for inversion * Use constraints to stabilize inversion * Cut off at finite l, q in input correlation
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Comparison to 1d Source Fits Fits & imaging extract same core parameters: R inv = 5.38 +/- 0.13 fm = 0.647 +/- 0.029 Same 30% undershoot for fits and images Gaussian fits can’t get halo CorAL Gaussian fit == “best” Coulomb correction
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3d Results Nail radii Height low by 30% Nail integral of source Resolve halo in L & O directions Measured Gaussian parameters (from source!): R S : 3.42 +/- 0.21 R O : 7.02 +/- 0.25 R L : 5.04 +/- 0.31 S(r=0): 10 +/- 1x10-5 : 0.442 +/- 0.067 Can extract the important physics!
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Core Halo Model Nickerson, Csörgo˝, Kiang, Phys. Rev. C 57, 3251 (1998). f is fraction of ’s emitted directly from core, effectively = f 2 in source function
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Core Halo Model, cont. From exploding core, with Gaussian shape: Flow profile simple, but adjustable: From decay of emitted resonances, has most likely lifetime (23 fm/c)
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Simple Model, Interesting Results Set R x =R y =R z =4 fm, f/o =10 fm/c, T=175 MeV, f=0.56 High velocity ’s get bigger boost. Boost + finite tail, but only modest core increase, in L,O directions.
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Focus on Outwards Direction Lifetime effects have dramatic affect on non-Gaussian halo in outwards direction.
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Focus on Outwards Direction … but only modest core changes. Gaussian R O fits: Baseline:5.63 Instant f/o:4.78 No :5.35 No lifetime:4.48 max =0.35:6.51 radii in fm, fit w/ r<15 fm, fit tolerance 1%
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Focus on Sidewards Direction Minor changes deep in tail reflecting geometry of induced halo. All curves have core radii ~ 4 fm.
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Focus on Longitudinal Direction Rapidity cut eliminates tail, otherwise similar to outwards direction.
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Take Home Messages from Model * Need emission duration + particle motion to get lifetime effect * Finite lifetime can create tail, w/o changing core radii substantially * RHIC HBT puzzle could be Gaussian fit missing tail from long lifetime * Resonance effects detectable, but similar to freeze-out duration effects * Don’t be fooled by acceptance effects Since source tails hide in Coulomb hole of correlation, imaging RHIC data should shed light on puzzle
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CorAL Features * Variety of kernels: – Coulomb, NN interactions, asymptotic forms – Any combination of p, n, , K +-, , plus some exotic pairs * Fit a 1d or 3d correlation w/ variety of Gaussian sources * Directly image a correlation, in 1d or 3d * Build model correlations/sources from – OSCAR formatted output, – Blast Wave, – variety of simple models * Build model correlations/sources in Spherical or Cartesian harmonics
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CorAL Status * Merging of three related projects: – original CorAL by M. Heffner, fitting correlations w/ source convoluted w/ full kernel – HBTprogs in 3d by D. Brown, P. Danielewicz, imaging sources from correlation data w/ full kernels – CRAB (++) by S. Pratt, use models to generate correlations, sources w/ full kernels * Rewritten in C++, open source, nearly stand alone (depends on GSL only) * Developed on MacOS X, linux, cygwin * Time scale for 1.0 release: end of summerish (sorry, probably not in time for QM2005)
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Extra Slides
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Low Relative Momentum Correlations Signal, pairs from same event (these guys are entangled) Background, pairs from different event, same cuts (looks like signal, but no entanglement) When C=1, there is no correlation Removes features in spectra not caused by entangled particles A versatile observable: can use nearly any type of pair
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3d HBT at RHIC Work in Bertsch-Pratt coordinates in pair CM frame: Boost from lab pair CM means lifetime effects transformed into Outwards/Longitudinal direction. Long (beam) Out Side
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What do the terms mean? l = 0 : Angle averaged correlation, get access to R inv l = 1 : Access to Lednicky offset, i.e. who emitted first (unlike only) l = 2 : Shape information: access to R O, R S, R L: C 20 R L C 00 -(C 20 ±C 22 ) R S,R O l = 3 : Boomerang/triaxial deformation (unlike only) l = 4 : Squares off shape
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Sampling Theorem If we can ignore FSI, the 1-dimensional kernels are: The l = 0 term is just a Fourier Transform. Sampling Theorem says for a given binning in q-space, source uniquely determined at certain r points (termed collocation points) spaced by: Sampling Theorem may be generalized to the l > 0 terms giving Here the l n are the zeros of the Spherical Bessel function.
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To reconstruct the source at these collocation points, choose knots: In general the spin-zero like pair meson kernel is much more complicated than this: and these knots are only an approximation to the best knots. Setting knots
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Representing terms in source We use basis splines to represent the radial dependence of each source term: Basis splines are piece-wise continuous polynomials: Setting knots for the splines is crucial for representing source well 0 th -order 1 st -order 2 nd -order …
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Representing the Source Function Radial dependence of each term in terms of Basis Splines: Generalized Splines: – N b =0 is histogram, – N b =1 is linear interpolation, – N b =3 is equivalent to cubic interpolation. Recursion relations == fast to evaluate, differentiate, integrate Resolution controlled by knot placement R Form basis for R 2, but not orthonormal
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The inversion process Koonin-Pratt eq. in matrix form: kernel not square kernel possibly singular noisy data error propagation this is an ill-posed problem Practical solution to linear inverse problem, minimize : Most probable source is: With covariance matrix:
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Constraints for 3d problem(s) Inversion can be stabilized with constraints. Constraints we use:
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Outwards/Sidewards Ratio Gaussian fits driven by r < 10 fm where ratio close to unity.
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Simple Model, Interesting Results Turn off resonance production (f=1) L,O tail reduced somewhat, S tail gone. Core lifetime causes tail same size as resonances.
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Simple Model, Interesting Results Instant freeze-out ( f/o =0 fm/c) Kills core-induced non-Gaussian tail, but resonance induced tail of similar magnitude.
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Simple Model, Interesting Results No resonances (f=1), instant freeze-out ( f/o =0 fm/c) Essentially kills non-Gaussian tail. Obviously need finite time effect for tail.
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Simple Model, Interesting Results Apply PHENIX acceptance cut of max =0.35 Kills contribution from high p L pairs, so kills core’s tail in L direction
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Simple model, interesting results No flow Lowers source, but not much else
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Simple model, interesting results Small temperature NO PLOT YET, HARD TO SAMPLE FROM SMALL TEMPERATURES
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Simple model, interesting results No flow, small temperature NO PLOT YET, HARD TO SAMPLE FROM SMALL TEMPERATURES
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