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Towards Fully 3-dimensional Simulations of Heavy Ion Collisions in the IP-Glasma Initial State Framework

Towards Fully 3-dimensional Simulations of Heavy Ion Collisions in the IP-Glasma Initial State Framework
Author: Scott McDonald
Publisher:
Total Pages:
Release: 2020
Genre:
ISBN:

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"Heavy ion collisions conducted at the Relativistic Heavy Ion Collider (RHIC) and the LargeHadron Collider (LHC) are sufficiently energetic to create a deconfined state of quarks andand gluons known as Quark Gluon Plasma (QGP). In the infinite momentum limit, thereis a longitudinal symmetry, known as boost invariance, that reduces the dynamics to 2+1-dimensions, simplifying simulations and allowing for detailed study of the transverse dy-namics of heavy ion collisions. Boost invariance is only an approximation, however, and acomplete understanding must come from the full 3+1D dynamics of heavy ion collisions. Inthis thesis, the phenomenologically successful IP-Glasma model [1, 2] for the initial state ofheavy ion collisions is generalized to 3+1D using JIMWLK rapidity evolution [3, 4] of thepre-collision Wilson lines. The initial gauge fields for the individual nuclei are modified to bepure gauge outside of the source terms in all three spatial directions in order to avoid energydeposition outside of the interaction region between the two nuclei. Additionally, Gauss’law is no longer trivially satisfied in 3+1D, and must be satisfied locally. An ansatz anditerative solution to Gauss’ law is introduced. The effect of these modifications is exploredon the evolution of the chromo-electric and chromo-magnetic fields, as well as the pressurein the IP-Glasma phase. Most importantly, these modifications allow for self-consistent tem-poral evolution of the Classical Yang Mills equation of motion on a 3D lattice and thusfor phenomenological application. The 3+1D IP-Glasma initial state is coupled to 3+1Drelativistic viscous hydrodynamics using the MUSIC numerical software [5], which is in turnmatched to the hadronic cascade model UrQMD [6]. This hybrid model is used to study theinitialization and evolution of Pb-Pb collisions at s =√2.76 TeV in 3+1D, providing thefirst opportunity to study the phenomenological consequences of the JIMWLK renormaliza-tion group equation on the longitudinal dynamics of heavy ion collisions and the resultingparticle spectra"--


Nuclear Matter and Heavy Ion Collisions

Nuclear Matter and Heavy Ion Collisions
Author: Madeleine Soyeur
Publisher: Springer Science & Business Media
Total Pages: 488
Release: 2012-12-06
Genre: Science
ISBN: 1468457152

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The Winter School "Nuclear Matter and Heavy Ion Collisions", a NATO Research Workshop held at Les Houches in February 89, has been devoted to recent developments in nuclear matter theory and to the study of central heavy ion collisions in which quasi macroscopic nuclear systems can be formed at various temperatures and densities. At in cident energies below 100 Me V per nucleon, the kinematic conditions are favourable for producing transient hot nuclei with temperatures of the order of a few MeV. At higher ener gies (100 MeV


Classical Models of Heavy-ion Collisions

Classical Models of Heavy-ion Collisions
Author: Thomas Jeffrey Schlagel
Publisher:
Total Pages: 272
Release: 1990
Genre:
ISBN:

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We study the effects of the nuclear equation of state (EOS) on intermediate energy heavy-ion collisions using classical microscopic models. The role of the EOS on the disassembly of expanding, hot nuclear matter, as well as the experimental data on multi-fragmentation and collective flow phenomena, are reviewed. Microscopic models used to describe heavy-ion collisions are also discussed. Collisions between cold drops, performed at various energies, are performed using classical molecular dynamics. These drops have an EOS which is similar to that of nuclear matter. Comparisons between collisions and disassemblies of hot, liquid drops indicate that equilibrated, hot matter is formed at 80% of the equilibrium density in central collisions between equal-sized drops. The yield of small clusters is given by the $Asbsp{c}{-tausb{rm eff}}$ power law; $tausb{rm eff}$ depends on the collision energy and has a minimum value of $tausb{rm eff} sim$ 1.7, which is also observed in nuclear fragmentation reactions. Two classical nucleon-nucleon interaction models are developed which have the saturation energy and density of nuclear matter, but have incompressibilities of 250 MeV and 535 MeV. Exact simulations of La+La and Au+Au collisions at 50 to 600 MeV/nucleon indicate that these models are sensitive to the interaction model at $Esb{rm lab} > 400$ MeV/nucleon. The results of Au+Au collisions are also compared to experimental data. The classical nuclear models are used to test the accuracy of the Vlasov-Nordheim approximation in the classical limit, called the Vlasov-Boltzmann (VB) equation, by comparing its results with the exact results at $Esb{rm lab} > 400$ MeV/nucleon. VB is found to be a reasonable approximation when the known EOS and scattering cross sections ($sigmasb{rm eff}$) are used. It is difficult to determine both the EOS and $sigmasb{rm eff}$ by fitting the exact results. A new treatment of scattering in VB simulations, which conserves angular momentum in two-body collisions, is also discussed. Using different n-n and n-p $sigmasb{rm eff}$, the VB simulations give very good agreement with the exact results.