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Statistical Model Description of Particle Production in HIC Krzysztof Redlich University of Wroclaw & EMMI GSI Modelling Statistical Operator: implementic conservation laws canonical & grand canonical model: comparisons with particle yields data in: e e A-A, p-p, and collisions Probing thermalisation with fluctuations of net baryon number model & experiment (STAR data) Essential role of higher order moments and their ratios to probe chiral cross-over transition at LHC and RHIC T LHC A-A collisions fixed s Quark-Gluon Plasma Chiral symmetry restored Hadronic matter Chiral symmetry broken x B Thermal nature of particle production in HIC i Q e He i Q H [Q, H ] 0 All properties of a thermodynamc ensemble in thermal equilibrium are derived from part. function Z (T ,V , ) Tr[e ( H Q) To get a specific value of Qi one fixes ] i from Qi T [ ln Z(T,i )]/i The equilibrium number of particles carrying q N q Ve GC q d 3 pe - E 2 q VmT e m K2 ( ) T 2 Statistical operator and mass spectrum resonance dominance: Rolf Hagedorn 2 ln Z GC Vp (T , ) 2 dpdm (m)e ( 2 + approximate Hagedorn mass spectrum p 2 m2 Qm ) (m) m e a m /TH (m) by experimentally known mass spectrum and include finite width of resonaces VT ln Z (T , ) 2 2 ihadrons di e Qi T s B W ds s K 2 ( T ) F (mi , s) Breit-Wigner resonaces 3 Particle Yields and model parameters Minimal setup of model parameters particle yield thermal density BR thermal density of resonances Ni V [nith (T , B ) K i nithRe s. (T , B )] K 3-parameters needed to fix all particle yields To account for chemical off-equilibrium effects introduce fugacity parameters in particle momentum distributions: ni i ni for all particles? J. Rafelski et. al. => introduce on the quark level: Density nh of hadrons composed of ku , kd , ks numbers of k k k u,d,s quarks gets a factor: nh u u d d s s nh 6-parameters needed to fix all particle yields 4 Hagedorn resonance gas and particle multiplicity ratios at RHIC Particle multiplicity ratios A. Andronic, P. Braun-Munzinger & J. Stachel MODEL DATA P. Braun Munzinger, D. Magestro, J. Stachel & K.R Good description of particle yields, with the statistical operator of HRG formulated in GC- ensemble, in central heavy ion collisions from top AGS up to RHIC . Problems with strangeness yields in non-central collisions at high energy and in central collisions from SIS-AGS. K – yields differ by a factor of almost 20 at SIS! 5 Kinetics of abelian charges C.M. Ko, V. Koch, Z. Lin, M. Stephanov, Xin-Nian Wang, K.R T,V Consider: d NK Rate equation NK N N K dt NK NK N and N Z GC Vm K TK 2 ( mK T (T ,V , ) Tr[e 2 N K 1 2 G L N N K N V V 2 Size of fluctuations GC K ) N C K ( H Q) ] Equilibrium limit N K 1 2 K NK m Vm TK 2 ( ) Vc m TK 2 ( ) T T mK 2 K 2 Z (T ,V ) TrS [e C H ] 6 i S i S e He H [S , H ] 0 conservation on the average Z (T , S ,V ) Tr [e GC Z GC S e S S S / T Z C S ( H S S ) exact conservation ] Z (T ,V ) TrS [e 1 Z S (T ,V ) 2 Consider thermal system with Total Strangenes “S”=0 A A A A nSC Ss nGC C S 2 d e iS Z GC S (T , T 0 H ] i ) S= -1 S=1 VC Vh Apart GC IS( s 2VC nsGC n 1 s 1 ) GC I 0 ( s 2VC nsGC n 1 s 1 ) same suppression factor 1 for S and S N GC N C suppression increases with S and with decreasing collision energy Apart 2 part A 7 i) Strong, quadratic dependence of |S|=1 particles with Apart at SIS ii) strange anti-particle/particle ratios independent of Apart N K C K Y Apart e( m B ) / T Ap2art emk / T e( mY B )/ T J. Cleymans, H. Oeschler & K.R. KaoS (GSI-SIS) 8 iii) Scaling properties of particle production yields Excellent description of kaon production from SIS to AGS subthreshold J. Cleymans, H. Oeschler & K.R. N K [ K ] [] [ ] [K ] K N [N ] [] Scaling: [K ] [ ] [K ] [N ] similar scaling for [ ]/[ K ] [ K ]/[ N ] : A. Andronic, P. Braun-Munzinger & K.R. 9 Strangeness Enhancement from pp to AA increases with: i) strangeness content of the particle ii) with decreasing collision energy A. Tounsi & K.R NA57 STAR Apart Decrease of enhancements from SPS to RHIC as predicted in the model Consistent predictions for order of magnitude of enhancements of Omega and Xi at RHIC Centrality dependence not correct when assuming Vcor . Apart ,however Vcordoes not need . to scale linearly. Assume: Vcor ( Apart / 2) V0 with 1 10 Canonical statistical model in pp collisions: Using Canonical description of strangeness and Grand Canonical for baryon number and electric change conservations in p-p collisions is a good approximation Using correlation volume instead of strangeness undersatuaration factor could be equivalent: see also I. Kraus H. Oeschler; F. Becattini et al. P. Braun-Munzinger et al. from “QGP” 3 11 Canonical statistical model in pp collisions: Using Canonical description of strangeness and Grand Canonical for baryon number and electric change conservations in p-p collisions is a good approximation LHC H. Oeschler et al. Observed deviations from Thermal Model predictions !! P. Braun-Munzinger et al. from “QGP” 3 12 Fixing thermal parameters: p-p C-C Si-Si J. Cleymans et al. Pb-Pb I. Kraus et al. Temperature approximately independent of system size and centrality Strong variation of baryon chemical potential with centrality and system size for mid-rapidity data 13 Energy dependence of thermal parameters at chemical freeze-out J. Cleymans et al. A. Andronic et al. 14 Particles excitation functions in HG model Braun-Munzinger, Cleymans, Oeschler &K.R. Andronic, Braun-Munzinger &Stachel (09) Nu Xu & K.R. H.Oeschler et al. Problem with canonical description of HADES data: data deviate by factor five from model predictions!! HADES 15 The Yields of anti-hypernuclei at RHIC N. Sharma et al., A. Andronic et al. First observation of hypernuclei 1952 by Danysz and Pniewski First observation of anti-hypernuclei by STAR in AU-AU coll. Can we understand yields within the SM? Statistical Model Results 3 p p 2 3 He p exp( [6 2 ] / T ) B S 3 He p 3 He exp(6 B / T ) 3 He Coalesence Model Results 3 He p pn p 3 He ppn p 3 3 3 2 pn p He pn p He 16 Charm production in e e annihilation Jet structure of hadrons production Flavor content of the jets: up type quarks (u, c) down type quarks (d , s, b) Can we quantify light and heavy flavor particles within Statistical Model ?? 17 Most hadronic events in high energy e+e collisions are two-jet events Each jet represents an independent fireball T 158 0.5 V 30 1 S 0.8 2 / dof 558 / 28 Problem: Open Charm and Bottom shows dramatic deviations from data N B mod el / data 1020 2-jets with Q 0 N D mod el / data 102 Subtract the contributions from charm and bottom to lighter particles e.g. C,B contributions to 11.7%, K 30.0% K *0 (892) 16.5%, (1020) 68.0% 2-jets with Q 0 sub. decays of “C” and “B” T 169 0.5 V 18 1 S 0.68 2 / dof 686 / 28 18 Canonical effects and charm/bottom mesons Qi di 3 d p exp( ( Ei bi i ) 3 (2 ) zi I ( 2 V x ) Z Q 1 N i QQi 1 V ziQi 1 Qi 1 x I ( 2 V x ) Z 1 zi Q Charge of the particle Charge of the system x Z 1Z1 i Q0 Total charge of the system And small 2Vc x 1 Ni QQi0 1 V zi V Z1 Strong Suppression of thermal particle phase-space Q 1 Ni Q 1 Qi 1 V zi V Z 1 Strong Enhancement of thermal particle phase-space 19 Charm and Bottom particles at LEP, 91 GeV D DS* D0 S D D* c1 J / ' B BS 0 B* Y c Ds1 0B Open charm and bottom well described by thermalisation of thermal fireball with overall Charm= 1 and Bottom= 1 J / , ' and c are entirely coming from Bottom’s decays and agree with model Hidden charm, Y is of non-thermal origin, thus, it does not fit to model systematic!20 Production cross section of relative to J / ' A. Andronic, F. Beutler, P. Braun-Munzinger, J. Stachel &K.R. NA50 The ratio for the Tevatron energy was derived from the CDF data on J / and ' and is for pt 1.25 GeV : ' We have extrapolated the measurements from pt 2 GeV down to 1.25 GeV Strong suppression of / ( J / ) ratio in PbPb relative to pA , pp and pp different production mechanism in elementary and heavy ion collisions ' RHIC CDF The nuclear modification canceled ' out in the / ( J / ) ratio as the pp value is the same as in the pA Data pA compilation by: Good agreement of Statistical Model and data in PbPb collisions 21 STAR DATA ON MOMENTS of B p p FLUCTUATIONS NB NB M B Phys. Rev. Lett. 105, 022302 (2010) Mean M B N p N p Variance B 2 ( N B )2 Skewness S B ( N B )3 / B 3 Kurtosis B ( N B ) / B 3 4 4 Properties of fluctuations in HRG F. Karsch & K.R. B( n ) n ( P(T , B ) / T 4 ) (B / T )n Calculate generalized susceptibilities: from Hadron Resonance Gas (HRG) partition function: P HRG Pmesons Pbaryons and Pbaryons T 4 F (m / T ) cosh(3q / T ) baryons B( 4) 1 (2 ) B B(3) 1 (1) B ( 4) resulting in: B B2 B( 2 ) B B(2) B(3) coth( B / T ) and tanh( B / T ) (1) (2) B B B2 B(2) (1) M B B S B B 2 B(3) ( 2) B Compare this HRG model predictions with STAR data at RHIC: Comparison of the Hadron Resonance Gas Model with STAR data Frithjof Karsch &K.R. K.R. RHIC data follow generic properties expected within HRG model for different ratios of the first four moments of baryon number fluctuations Can we also quantify the energy dependence of each moment separately using thermal parameters along the chemical freezeout curve? Mean, variance, skewness and kurtosis obtained by STAR and rescaled HRG STAR Au-Au s 200 M p p 8.5 STAR Au-Au s 200 M p p 1.8 these data, due to restricted phase space: Account effectively for the above in the HRG model by rescaling the volume parameter by factor 1.8/8.5 QCD phase boundary & Heavy Ion Data Particle yields and their ratios, well described by the Hadron Resonance Gas QCD phase boundary appears near freezeout line Thus: HRG has to be a good description of regular part of QCD partition function in hadronic phase Thus: HRG has to describe LGT thermodynamics Kurtosis as an excellent probe of deconfinement S. Ejiri, F. Karsch & K.R. 1 c4 9 c2 Kurtosis R4,2 B HRG factorization of pressure: PB (T , q ) f [T , (m)]cosh(3q / T ) F. Karsch, Ch. Schmidt consequently: c4 / c2 9 in HRG 2 In QGP, SB 6 / Kurtosis=Ratio of cumulants c4q / c2q B The R4,2 measures the quark content of particles carrying baryon number ( N q )4 ( N q )2 3 ( N q )2 excellent probe of deconfinement Higher moments of baryon number fluctuations J. Engels, F. Karsch, B. Friman, V. Skokov & K.R. If freeze-out in heavy ion collisions occurs from a thermalized system close to the chiral crossover temperature, this will lead to a negative sixth and eighth order moments of net baryon number fluctuations. These properties are universal and should be observed in HIC experiments at LHC and RHIC Figures: results of the PNJL model obtained within the Functional Renormalisation Group method 28 Fluctuations of 6th and 8th order moments exhibit strong variations from HRG results: Their negative values near chiral transition to be seen in heavy ion collisions at LHC and RHIC The range of negative fluctuations near chiral cross-over: PNJL model results with quantum fluctuations being included : These properties are due to O(4) scaling , thus should be also there in QCD. 29 Conclusions The Hagedorn partiction function of the Hadron Resonance Gas is a very good approximation of the regular part of the QCD partiction function: => it reproduces bulk of particle yields meassured form SIS up to LHC energy => it reproduces net proton fluctuations up to 4th order measured at RHIC => It reproduces fully ratios of different susceptibilities obtained on the lattice => it reproduces thermodynamics up to very near T_c obtained on the lattice for different quark masses The 6th and 8th order moments of baryon number fluctuations are excellent probes of chiral cross-over 30 transition in HIC at the LHC and RHIC Centrality dependence of baryon chemical potential For NA57 the temperature is fixed to T 168 MeV from central Pb-Pb collisions: ( the value consistent with recent analysis of A. Andronic et al.) 31 Strangeness enhancement from p-Be to central Pb-Pb collisions at s 17.3 GeV NN Canonical model with exact strangeness conservation at fixed T 168 MeV and B being centrality dependent provides good description of NA57 data if the correlation volume scales as: V ( A / 2) with 1/ 3 part 32 Multistrange particle enhancement at RHIC Calculations done at fixed T 164MeV , 20MeV (Nu Xu et al.) for all centrality Overall agreement is not satisfactory, particularly for Lambda yields 33