Recent Developments of A Multi-Phase Transport Model Zi-Wei Lin Department of Physics East Carolina University AMPT Collaborators: Che Ming Ko (Texas A&M University) Bao-An Li (Texas A&M University-Commerce) Subrata Pal (Tata Institute of Fundamental Research, India) Bin Zhang (Arkansas State University) Acknowledgements to Helmholtz International Center for FAIR, Workshop organizers XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 1/31 Outline Structure of A Multi-Phase Transport (AMPT) model Present status of AMPT Recent developments Possible future directions Summary All the best, Kryzrof XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 2/31 What do we need for simulations of high energy heavy ion collisions? We need: Initial particle/energy production Options: Soft+hard model, CGC, pQCD, ... Partonic interactions, thermalization & evolution Parton cascade (ZPC, MPC, BAMPS), (ideal, viscous) hydrodynamics, dE/dx, ... Hadronization /QCD phase transition String fragmentation, quark coalescence/parton recombination, statistical hadronization, Cooper-Frye, independent fragmentation, rate equations, ... Hadronic interactions Hadron cascade (ART, RQMD, UrQMD, ...), thermal model (w/ freezeout temperatures), … The AMPT model currently includes the green components. In particular, it can be used to study fluctuation, quark coalescence, multi-particle correlation, … XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 3/31 Structure of AMPT v1.xx (default version) A+B HIJING (parton dist. functions, nuclear shadowing): minijet partons, excited strings, spectators ZPC (parton cascade) Partons freeze out Hadronization (Lund string fragmentation) Extended ART Hadrons freeze out (at a global cut-off time); strong-decay all remaining resonances Final particle spectra XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 4/31 A central Au+Au event at 200AGeV from the default AMPT model after the primary AA collisions Only formed particles are shown 60fm box Beam axis 1st frame: spectator nucleons. Dynamics is time-delayed at large rapidities XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 5/31 A central Au+Au event at 200AGeV from the default AMPT model View on the beam axis E.g. at middle right: rho (green) decayed at 7.0 fm/c at lower right: K*bar is produced at 16.6 fm/c & vanishes at 20.8fm/c. XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 6/31 Why string melting version of AMPT? Estimate the initial energy density in AA collisions: dET / dy dET / dy e0 ~ » 6 2 3 ~ 2.5 p R t 0 150 fm SPS RHIC Nuclear radius 20 GeV/fm3 LHC >>critical energy density Proper formation time, for QCD phase transition: taken as 1 fm/c εc ~ O(1) GeV/fm3 At high-enough energies, hadronic matter such as strings cannot exist early on, they should be represented by a high density partonic matter: the string melting version of AMPT XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław Lin&Ko, PRC65 June 15, 2013 7/31 Structure of AMPT v2.xx (String Melting version) A+B HIJING (parton dist. functions, nuclear shadowing): minijet partons, excited strings, spectators "Melt" to q & qbar via intermediate hadrons ZPC (parton cascade) Partons freeze out Hadronization (Quark Coalescence) Extended ART Hadrons freeze out (at a global cut-off time); strong-decay all remaining resonances Final particle spectra XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 8/31 A central Au+Au event at 200AGeV from the String Melting AMPT σp=3mb 60fm box Beam axis E.g. middle region (near mid-rapidity): coalescence of q (red) and qbar (cyan) XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 9/31 A central Au+Au event at 200AGeV from the String Melting AMPT View on the beam axis XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 10/31 Compare the same event default AMPT vs String Melting AMPT At t=5 fm/c: With string melting: many more partons, parton stage dominates; hadron stage starts much later XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 11/31 Present status of AMPT First public release of AMPT codes: ~ April 2004. Detailed physics descriptions in the long paper: Lin, Ko, Li, Zhang & Pal, PRC 72, 064901 (2005). "Official" versions v1.11/v2.11 (2004) and v1.21/v2.21 (2008) are available at https://karman.physics.purdue.edu/OSCAR More versions, including recent & test versions, are available at http://personal.ecu.edu/linz/ampt/ v1.25t3/v2.25t3 (8/2009) v1.25t7/v2.25t7 (9/2011) v1.25t7d/v2.25t7d (4/2012) v1.26t1/v2.26t1 (9/2012) The webpage looks like this XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław Juneor 15,this 2013 (offline) 12/31 The heavy ion community is also using AMPT as a valuable tool Simplified Picture What really happens in an event Example: Triangular Flow discovered using AMPT: Alver & Roland, PRC81 From Alver’s talk: XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 13/31 A b=10fm Au+Au event at 200AGeV from String Melting AMPT View on the beam axis Initial overlap region has an irregular geometry XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 14/31 Summary of modifications in AMPT (1) 9/2012 test version v1.26t1/v2.26t1: To avoid crash (segmentation fault due to s<0) at high energy such as LHC at large NT: use double precision in art1f.f when calculating sqrt(s), use double precision in linana.f to calculate β avoid NaN. use a more general formula in amptsub.f to calculate rapidity (valid for hadrons at large rapidities that have |PZ|≥E due to finite precision) 4/2012 test version v1.25t7d/v2.25t7d: Added an option to enable π0 electromagnetic decay after hadron cascade 2/2012 test version v1.25t7b/v2.25t7b: Added an option to enable random orientation of reaction plane XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 15/31 Summary of modifications in AMPT (2) 5/2011 test version v1.25t4/v2.25t5: Include finite widths of resonances (K* η ρ ω Φ Δ) when produced from quark coalescence in the string melting version, added for the purpose of resonance reconstruction using invariant mass. 7/2009 test version v1.25t2/v2.25t2: Added an option to enable users to modify nuclear shadowing smoothly between no-shadowing and the default HIJING shadowing 6/2009 test version v1.25t1/v2.25t1: Added an option of event selection so that each event will have at least 1 mini-jet parton above a set Pt value in the initial condition; added an option to embed a back-to-back high-Pt q/qbar pair in each event; write out Npart information (spatial coordinates and status of each incoming nucleon); added option to write complete parton information before & after parton cascade and the full parton collision history for the string melting version XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 16/31 Summary of modifications in AMPT (3) 3/2009 test version v1.23/v2.23: Included a subroutine to enable users to insert user-defined hadrons before the start of the hadron cascade 10/2008 test version v1.22/v2.22: Included deuteron(d) interactions in hadron cascade via d+M ↔ B+B (M or B represents a meson or a baryon), also included elastic collisions of d+M and d+B; similar anti-deuteron interactions are also included 10/2008 v1.21/v2.21: Added option to turn off φ meson decays at the end of hadron cascade i.e., at NT=NTMAX …… XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 17/31 Example: extension of AMPT to deformed Uranium (1) 0.8 This test version (v1.25t8/v2.25t8) is not online. 0.6 < e2> 2011: Added deformed Uranium U238 as projectile/target. U+U body U+U tip U+U side U+U Au+Au AMPT-Default (a) 0.4 0.2 0 0 100 200 300 400 500 Npart 0.8 < e3> 0.6 U+U body U+U tip U+U side U+U Au+Au AMPT-Default (b) 0.4 0.2 Considered a few special geometries and MB UU Rihan Haque, Lin & Mohanty, PRC 85 0 0 100 200 300 400 500 Npart Spatial anisotropy XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 18/31 Example: extension of AMPT to deformed Uranium (2) v2 closely resembles ε2 AMPT-SM |h|<0.5 0.8 (a) 0.1 0.6 < e2> <v2> 0.15 U+U body U+U tip U+U side U+U Au+Au U+U body U+U tip U+U side U+U Au+Au AMPT-Default (a) 0.4 0.05 0.2 0 0 100 200 300 400 500 0 0 Npart <v3> 0.03 0.8 U+U body U+U tip U+U side U+U Au+Au 200 300 400 500 Npart AMPT-SM |h|<0.5 0.6 < e3> 0.04 100 (b) 0.02 U+U body U+U tip U+U side U+U Au+Au AMPT-Default (b) 0.4 0.2 0.01 0 0 0 0 100 200 300 400 100 200 300 400 500 Npart 500 Npart XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 19/31 Ongoing work: fix charge conservation in AMPT (1) After fixing this problem, AMPT will be better suited for studies of charge fluctuation and balance functions. Why is charge conservation violated in AMPT? Problems come from hadron cascade of AMPT XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 20/31 Ongoing work: fix charge conservation in AMPT (2) History of hadron cascade in AMPT Based on the ART model Li&Ko, PRC52 Kbar interactions added Song,Li&Ko, NPA646 NNbar <> mesons Zhang et al, PRC61 BBbar <> mesons, explicit K* Lin et al, PRC64, NPA698 interactions Lin&Ko,PRC65 interactions Pal,Ko&Lin, NPA707 Multi-strange interactions ( ) Pal,Ko&Lin, NPA730 Deuteron interactions Oh,Lin&Ko, PRC80, NPA834 XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 21/31 Ongoing work: fix charge conservation in AMPT (3) Hadronization Why is charge conservation violated in AMPT? First reason: The hadron cascade has K+ and K- as explicit particles, but not K0 and K0-bar. K0 To let all kaons interact: • before hadron cascade, we change K0 to K+ (also: K0-bar to K-) • after hadron cascade, we change half of final K+ into K0. K- K+ K- K0-bar Hadron cascade K0 XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław K+ K+ K- K+ K- June 15, 2013 K0-bar 22/31 Ongoing work: fix charge conservation in AMPT (4) Why is charge conservation violated in AMPT? Second reason: Many reactions in the hadron cascade are not implemented for each possible isospin configuration: • isospin-averaged cross section is used, • final state particles have randomly-generated isospin. For example: p h ®p p each final-state pion could have +, 0, – charge in AMPT: so we can have p + h ® p + p 0 or p+ h ®p+ allowed XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław p- should be forbidden June 15, 2013 23/31 Ongoing work: fix charge conservation in AMPT (5) We need to: add K0 & K0-bar as explicit particles, allow similar interaction types as for K+ & K-. Hadronization Several steps: K0 K+ K0-bar K- 1) Forbid final states that violate charge conservation: this is enough to conserve charge. 2) Update/determine cross sections of allowed final states including the branching ratios Hadron cascade (w/ full isospin) 3) Check detailed balance among related cross sections K0 K+ K0-bar KRequires checking essentially all hadron reactions in AMPT XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 24/31 Ongoing work: fix charge conservation in AMPT (6) Meson-Meson channels SU(2): With strangeness: XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 25/31 Ongoing work: fix charge conservation in AMPT (7) Meson-Baryon & Baryon-Baryon channels XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 26/31 Possible future directions 1 2 • Improve parton recombination by using local density as criteria • Coalescence in phase-space • Couple AMPT with viscous hydrodynamics • Gluons in parton recombination (energy-momentum conservation) • Fragmentation of high-Pt partons XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 27/31 Possible future direction 1: Coalescence Improve the quark coalescence model for hadronization Currently, a parton can coalesce after kinetic freeze-out (i.e. after it will not have further interactions) Average parton density at coalescence depends on parton scattering cross section σp; & typical value is too low (<< εc ~ 1 GeV/fm3) We need to start coalescence around energy density ~εc independent of σp Quark coalescence will work better due to the much higher density at the time of coalescence Zhang,Chen&Ko, JPG35 XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 28/31 Possible future direction 2: hybrid model A+B HIJING (parton dist. functions, nuclear shadowing): minijet partons, excited strings, spectators "Melt" to q & qbar via intermediate hadrons AMPT v2.xx (String Melting) ZPC (parton cascade) Partons freeze out Hadronization (Quark Coalescence) Extended ART Final particle spectra XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 29/31 Possible future direction 2: hybrid model HIJING (parton dist. functions, nuclear shadowing): minijet partons, excited strings, spectators A+B Direct link to QCD: (EoS, viscosity) Partons Distribution Self-contained initial condition, including fluctuations Other initial condition allowed, e.g. CGC Can compare with current AMPT: hydro vs parton cascade "Melt" to q & qbar via intermediate hadrons Hydrodynamics (viscous, 3+1d, event-by-event ) Distribution hadrons Extended ART Final particle spectra XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 30/31 Summary AMPT has been a self-contained phenomenological model (from initial condition to final observables event-by-event): includes fluctuations and non-equilibrium dynamics; can be a test-bed of different conceptual ideas; should incorporate essential stages of heavy ion collisions. The approach needs further developments (more direct link to QCD variables & properties): improving the parton recombination model for hadronization or couple with 3+1d viscous hydrodynamics. Comments, suggestions, collaborations are greatly welcome. XXXI Max Born Symposium and HIC for FAIR Workshop, Wrocław June 15, 2013 31/31