Looking Through the “Veil of Hadronization”: Pion Entropy & PSD at RHIC STAR John G.
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Looking Through the “Veil of Hadronization”: Pion Entropy & PSD at RHIC STAR John G. Cramer Department of Physics University of Washington, Seattle, WA, USA STAR Collaboration Meeting California Institute of Technology February 18, 2004 Phase Space Density: Definition & Expectations Phase Space Density - The phase space density f(p, x) plays a fundamental role in quantum statistical mechanics. The local phase space density is the number of pions occupying the phase space cell at (p, x) with 6-dimensional volume Dp3Dx3 = h3. The source-averaged phase space density is f(p)∫[f(p, x)]2 d3x / ∫f(p, x) d3x, i.e., the local phase space density averaged over the f-weighted source volume. Because of Liouville’s Theorem, for free-streaming particles f(p) is a conserved Lorentz scalar. Sinyukov has recently asserted that f(p) is also approximately conserved from the initial collision to freeze out. At RHIC, with about the same HBT source size as at the CERN SPS but with more emitted pions, we expect an increase in the pion phase space density over that observed at the SPS. STAR February 18, 2004 2 John G. Cramer Entropy: Calculation & Expectations Entropy – The pion entropy per particle Sp/Np and the total pion entropy at midrapidity dSp/dy can be calculated from f(p). The entropy S of a colliding heavy ion system should be produced mainly during the parton phase and should grow only slowly as the system expands and cools. It never decreases (2nd Law of Thermodynamics.) A quark-gluon plasma has a Entropy is conserved largeduring number of degrees of hydrodynamic freedom. It should generate a expansion and freerelatively large Thus, entropy streaming. thedensity, up to 12 to 16 times than that entropy of thelarger system of aafter hadronic gas. should freeze-out be close to the initial At RHIC,and if ashould QGP phase entropy grows with centrality provide a critical we would expect the entropy toearlygrow constraint on the strongly increasing stagewith processes of thecentrality and system. participant number. hep-ph/0212302 nucl-th/0104023 Entropy penetrates the “veil of hadronization”. STAR February 18, 2004 3 John G. Cramer Pion Phase Space Density at Midrapidity The source-averaged phase space density f(mT) is the dimensionless number of pions per 6-dimensional phase space cell h3, as averaged over the source. At midrapidity f(mT) is given by the expression: 3 2 λ(c π ) 1 1 d N f (m T ) E π 2 π m T dm T dy R S R O R L λ Average phase space density STAR Jacobian Momentum Spectrum to make it a Lorentz scalar February 18, 2004 4 HBT “momentum Pion volume” Vp Purity Correction John G. Cramer RHIC Collisions as Functions of Centrality At RHIC we can classify collision events by impact parameter, based on charged particle production. Frequency of Charged Particles produced in RHIC Au+Au Collisions 50-80% 30-50% 20-30% 10-20% 5-10% 0-5% of sTotal Participants Binary Collisions STAR February 18, 2004 5 John G. Cramer Corrected HBT Momentum Volume Vp /l½ 50-80% 2000 1500 Centrality 130 GeV/nucleon 40-50% Peripheral GeV3 1000 700 106 Vp 500 30-40% Fits assuming: Vp l-½=A0 mT3a (Sinyukov) 20-30% 10-20% 5-10% 0-5% 300 Central 200 150 0.05 0.1 0.15 0.2 mT - mp (GeV) STAR February 18, 2004 6 0.25 0.3 Vp λ (c π )3 λ R SR O R L John G. Cramer Global Fit to Pion Momentum Spectrum 1000 130 GeV/nucleon 500 100 d2N 2 mTdmTdy We make a global fit of the uncorrected pion spectrum vs. centrality by: (1) Assuming that the spectrum has the form of an effective-T Bose-Einstein distribution: d2N/mTdmTdy=A/[Exp(E/T) –1] and (2) Assuming that A and T have a quadratic dependence on the number of participants Np: 50 A(p) = A0+A1Np+A2Np2 T(p) = T0+T1Np+T2Np2 A0 A1 A2 T0 T1 T2 STAR Value 31.1292 21.9724 -0.019353 0.199336 -9.23515E-06 2.10545E-07 10 Error 14.5507 0.749688 0.003116 0.002373 2.4E-05 6.99E-08 February 18, 2004 5 0.1 0.2 0.3 mT 7 0.4 0.5 0.6 m John G. Cramer Interpolated Phase Space Density f at S½ = 130 GeV HBT points with interpolated spectra 0.4 NA49 f 0.3 0.2 } Note failure of “universal” PSD between CERN and RHIC. Central 0.1 Peripheral 0.1 STAR February 18, 2004 0.2 mT m 8 0.3 0.4 John G. Cramer Extrapolated Phase Space Density f at S½ = 130 GeV Spectrum points with extrapolated HBT Vp/l1/2 Central 0.2 Note that for centralities of 0-40% of sT, fchanges very little. f drops only for the lowest 3 centralities. f 0.1 0.05 0.02 Peripheral 0.01 0.1 STAR 0.2 February 18, 2004 0.3 mT m 9 0.4 0.5 John G. Cramer 0.6 Converting f to Entropy per Particle (1) Starting from quantum statistical mechanics, we define: f f ( x , p); dS6 - f Log ( f ) ( f 1) Log ( f 1) - f Log ( f ) f 12 f 2 - 16 f 3 965 f 4 ... +0.2% An estimate of the average pion entropy per 3particle S/N can be obtained O(f) O(f )over the local phase space O(f4) from a 6-dimensional space-momentum integral density f(x,p): 0.1% dS6(Series)/dS6 dp 3dx 3dS ( p , x ) 6 - S N1.000 3 3 dp dx f ( p, x ) - dp 3dx 3[- f Log ( f ) f 12 f 2 - 16 f 3 965 f 4 - - dp 3dx 3 f To perform the space integrals, we assume that f(x,p) = f(p) g(x), 3 2 2 2 2 2 2 where g(x) = 2 Exp[-x /2Rx -y /2Ry -z /2Rz ], i.e., that the source has -0.1%shape based on HBT analysis of the system. Further, we make the a Gaussian Sinyukov-inspired -a assumption that the three radii have a momentum dependence proportional to mT . Then the space can be performed analytically. O(f2integrals ) This gives the numerator3 and-3adenominator integrands of the above expression factors-0.2% of RxRyRz = Reff mT . (For reference, a~½) f STAR February 18, 2004 10 John G. Cramer Converting f to Entropy per Particle (2) The entropy per particle S/N then reduces to a momentum integral of the form: dp dx dS 6 ( p, x ) - S N 3 3 dp dx f ( p, x ) 3 3 (6-D) - 3 - dp mT -3a [- f Log f f 1 2 3 - 0 dpT pT mT 1-3a 5- Log ( 8 ) 2 dp mT -3a f 2 0 dpT pT mT 3 f 3 5 24 2 f 4 ] (3-D) f (8) [- f Log f 12 f 5- Log f 2 -9 4 1-3a 2 - 9 43 f 3 245 2 f 4 ] f We obtain a from the momentum dependence of Vpl-1/2 and perform the momentum integrals numerically using momentum-dependent fits to f -1/2 or fits to Vpl and the spectra. STAR February 18, 2004 11 John G. Cramer (1-D) Entropy per Pion from Vp /l½ and Spectrum Fits 4.6 Peripheral 4.4 Line = Combined fits to spectrum and Vp/l1/2 S N 4.2 4 3.8 Central 3.6 50 STAR 100 February 18, 2004 150 200 Np participants 12 250 300 350 John G. Cramer Thermal Bose-Einstein Entropy per Particle The thermal estimate of the p entropy per particle can be obtained by integrating a Bose-Einstein distribution over 3D momentum: S/N 0 pT 2 dpT [( f BE 1) Ln( f BE 1) - f BE Ln( f BE )] 0 0.2 0.4 0.6 0.8 1. 1.2 1.4 1.6 1.8 2. p/mp 0 7.80625 5.48443 4.75415 4.40528 4.2043 4.07531 3.98644 3.92204 3.87358 3.83602 0.3 6.29571 4.69072 4.19131 3.95892 3.82985 3.75054 3.69848 3.6627 3.63726 3.61869 1 Exp[(mT - p ) / T ] - 1 10 0.6 4.74597 3.83487 3.56733 3.45659 3.40494 3.38033 3.36949 3.36614 3.36702 3.37031 0.9 2.94368 2.74168 2.74029 2.78018 2.82925 2.87817 2.92397 2.96584 3.00378 3.03804 8 p = 0 6 SN T/mp pT 2 dpT f BE where f BE 4 2 p = mp 0 0.5 Note that the thermal-model entropy per particle usually decreases with increasing temperature T and chemical potential p. STAR February 18, 2004 13 1 Tm 1.5 John G. Cramer 2 Entropy per Particle S/N with Thermal Estimates T 90 MeV 4.6 Peripheral S N 4.4 T 120 MeV Solid line and points show S/N from spectrum and Vp/l1/2 fits. 4.2 T 200 MeV 4 For T=120 MeV, S/N implies a pion chemical potential of p=63 MeV. Dashed line indicates systematic error in extracting Vp from HBT. 3.8 3.6 Landau Limit: m 0 Central 3.4 50 STAR 100 February 18, 2004 200 150 Np participants 14 250 300 John G. Cramer 350 Total Pion Entropy dSp/dy 2500 Dashed line indicates systematic error in extracting Vp from HBT. 2000 dS dy 1500 P&P Why is dSp/dy linear with Np?? Dot-dash line indicates dS/dy from BSBEx fits to interpolated <f>. 1000 P&P 500 Snuc Entropy content of nucleons + antinucleons 50 STAR 100 150 200 250 300 Np February 18, 2004 15 John G. Cramer 350 Total Pion Entropy per Participant (dSp/dy)/Np Central 6.7 dS dy Np 6.6 6.5 Average 6.4 6.3 6.2 6.1 Peripheral 50 100 150 200 250 300 350 Np STAR February 18, 2004 16 John G. Cramer Conclusions 1. The source-averaged pion phase space density f is very high, in the low momentum region roughly 2 that observed at the CERN SPS for Pb+Pb at Snn=17 GeV. 2. The pion entropy per particle Sp/Np is very low, implying a significant pion chemical potential (p~63 MeV) at freeze out. 3. For central collisions at midrapidity, the entropy content of all pions is ~5 greater than that of all nucleons+antinucleons. 4. The total pion entropy at midrapidity dSp/dy grows linearly with initial participant number Np. (Why?? Is Nature telling us something?) 5. The pion entropy per participant (dSp/dy)/ Np , which should penetrate the “ veil of hadronization”, has a roughly constant value of 6.5 and shows no indication of the increase expected with the onset of a quarkgluon plasma. 6. Our next priority is to obtain similar estimates of (dSp/dy)/ Np for the d+Au and p+p systems at RHIC. STAR February 18, 2004 17 John G. Cramer The End STAR February 18, 2004 18 John G. Cramer