Relativistic Dissipative Hydrodynamic Description of the Quark-Gluon Plasma

Relativistic Dissipative Hydrodynamic Description of the Quark-Gluon Plasma PDF

Author: Akihiko Monnai

Publisher: Springer Science & Business Media

Published: 2014-01-20

Total Pages: 138

ISBN-13: 4431547983

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This thesis presents theoretical and numerical studies on phenomenological description of the quark–gluon plasma (QGP), a many-body system of elementary particles. The author formulates a causal theory of hydrodynamics for systems with net charges from the law of increasing entropy and a momentum expansion method. The derived equation results can be applied not only to collider physics, but also to the early universe and ultra-cold atoms. The author also develops novel off-equilibrium hydrodynamic models for the longitudinal expansion of the QGP on the basis of these equations. Numerical estimations show that convection and entropy production during the hydrodynamic evolution are key to explaining excessive charged particle production, recently observed at the Large Hadron Collider. Furthermore, the analyses at finite baryon density indicate that the energy available for QGP production is larger than the amount conventionally assumed.

Quark--Gluon Plasma 3

Quark--Gluon Plasma 3 PDF

Author: Rudolph C. Hwa

Publisher: World Scientific

Published: 2004

Total Pages: 786

ISBN-13: 9812795537

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Annotation. Text reviews the major topics in Quark-Gluon Plasma, including: the QCD phase diagram, the transition temperature, equation of state, heavy quark free energies, and thermal modifications of hadron properties. Includes index, references, and appendix. For researchers and practitioners.

Non-equilibrium Hydrodynamics of the Quark-Gluon Plasma, from Theory to Phenomenology

Non-equilibrium Hydrodynamics of the Quark-Gluon Plasma, from Theory to Phenomenology PDF

Author: Dekrayat K. Almaalol

Publisher:

Published: 2021

Total Pages: 0

ISBN-13:

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The quark-gluon plasma (QGP) is a deconfined phase of strongly interacting matter which can be described by the theory of quantum chromodynamics (QCD). The QGP filled the entire universe in the early moments after the big bang and is believed to exist in the present time in the core of massive neutron stars. Understanding the physical properties of QGP and its non-equilibrium dynamics requires solving the full non-perturbative QCD equations of motion, which is an unsolved problem at this time. Ultra-relativistic heavy ion collisions (URHICs) can be used to reproduce the extreme conditions of the early universe and create a short-lived QGP in the laboratory; in what is called the ``little'' bang. The highly momentum-anisotropic far-from-equilibrium initial state created in these experiments evolves dynamically in three main stages: pre-equilibrium ([tau] 0.5 fm/c), thermalization/hydrodynamization ([tau] 0.5-2 fm/c), and finally freeze-out/hadronization ([tau]> 10 fm/c), where 1fm/c = 3x10^(-24) s. Each of these stages span a different regime of physics, with different relevant degrees of freedom and, therefore, are described by different theoretical models, such as QCD kinetic theory, dissipative hydrodynamics, and hadronic kinetic theory. This dissertation considers the impact of all three of these stages on our understanding of the QGP generated in URHICs, with the focus on better understanding the non-equilibrium dynamics of the QGP, its path to equilibrium and the effect such non-equilibrium dynamics have on our ability to extract fundamental information about the QGP. This dissertation also provides theoretical insights into how to improve URHIC simulations by examining the impact of non-equilibrium corrections present during different stages of QGP evolution.

Non-equilibrium Hydrodynamics of the Quark-gluon Plasma

Non-equilibrium Hydrodynamics of the Quark-gluon Plasma PDF

Author: Nopoush Mohammad

Publisher:

Published: 2019

Total Pages: 0

ISBN-13:

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Relativistic heavy-ion collision experiments are currently the only controlled way to generate and study matter in the most extreme temperatures (T ~10e+12 K). At these temperatures matter undergoes a phase transition to an exotic phase of matter called the quark-gluon plasma (QGP). The QGP is an extremely hot and deconfined phase of matter where sub-nucleonic constituents (quarks and gluons) are asymptotically free. The QGP phase is important for different reasons. First of all, our universe existed in this phase up to approximately t ~10e-5 s after the Big Bang, before it cools down sufficiently to form any kind of quark bound states. In this regard, studying the QGP provides us with useful information about the dynamics and evolution of the early universe. Secondly, high-energy collisions serve as a microscope with a resolution on the order of 10e-15 m (several orders of magnitude more powerful than the best ever developed electron microscopes). With this fantastic probe, penetrating into the detailed structure of nucleons, and the discovery of new particles and fundamental phases are made possible. The dynamics of the QGP is based on quantum chromodynamics (which governs the interactions of quarks and gluons) and the associated force is "strong force". The strong collective behaviors observed experimentally inspired people to use dissipative fluid dynamics to model the dynamics of the medium. The QGP produced in heavy-ion collisions, experiences strong longitudinal expansion at early times which leads to a large momentum-space anisotropy in the local rest frame distribution function. The rapid longitudinal expansion casts doubt on the application of standard viscous hydrodynamics (vHydro) models, which lead to unphysical predictions such as negative pressure, negative one-particle distribution function, and so on. Anisotropic hydrodynamics (aHydro) takes into account the strong momentum-space anisotropy in the leading order distribution function in a consistent and systematic way. My dissertation is about the formulation and application of anisotropic hydrodynamics as a successful non-equilibrium hydrodynamics model for studying the QGP. For this purpose, I introduce the basic conformal anisotropic hydrodynamics formalism and then explain the ways we included realistic features (bulk degree of freedom, quasiparticle implementation of realistic equation of state, more realistic collisional kernel), to make it a suitable hydrodynamics model for studying the QGP generated in heavy-ion collisions. For verification of our model we have compared the evolution of model parameters predicted by aHydro and vHydro, with exact analytical solution of the Boltzmann equation. For this purpose, we have studied the evolution of the system under conformal Gubser flow using the aHydro model. By transforming to de Sitter spacetime (a non-trivial curved coordinate system) we simplified the dynamics to 0+1d spacetime. Comparisons with exact solutions show that aHydro better reproduces the exact solutions than the best available vHydro models. However, the system is not conformal and the aHydro needed to be improved to include a realistic prescription for the equation of state which takes care of non-ideal effect in the dynamics. In the framework of finite temperature eld theory the equation of state is provided by numerical calculation of QCD partition function using lattice QCD (LQCD), whereas, devising an equation of state for aHydro model is challenging because therein we deal with anisotropic pressures. In the next step of my research, we have designed a novel method for implementing the realistic equation of state (provided by lattice QCD) in the aHydro formalism. This model, called the quasiparticle aHydro model, integrates the non-conformal effects in the aHydro model. The non-conformal effects are due to strong interactions of plasma constituents which leads to temperature-dependence of the particles' effective mass in the system. Based on the quasiparticle picture, we have developed the quasiparticle aHydro (aHydroQP) model which has all necessary components for studying the phenomenology of the QGP created in heavy-ion collisions. We have then compared the phenomenological predictions of the aHydroQP model with experimental observations. Comparisons illustrate a high level of consistency between our model and the experimental data. The last two chapters are about two applications of the aHydro model to field-theoretical measurables in the QGP. In these chapters, we have calculated the quark self-energy in an anisotropic QGP. The quark self-energy is important because it encodes the way quarks gain interactional mass while in the hot QGP. I also have presented the calculation of gluon self-energy in hard loop approximation in an anisotropic QGP.The gluon self-energy is important since it is related to heavy-quark potential and heavy quarkonium suppression. Heavy quarkonia bound states, besides theoretical importance, serve as a thermometer for the QGP.

The XVIII International Conference on Strangeness in Quark Matter (SQM 2019)

The XVIII International Conference on Strangeness in Quark Matter (SQM 2019) PDF

Author: Domenico Elia

Publisher: Springer Nature

Published: 2020-10-03

Total Pages: 568

ISBN-13: 3030534480

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This book focuses on new experimental and theoretical advances concerning the role of strange and heavy-flavour quarks in high-energy heavy-ion collisions and in astrophysical phenomena. The topics covered include • Strangeness and heavy-quark production in nuclear collisions and hadronic interactions, • Hadron resonances in the strongly-coupled partonic and hadronic medium, • Bulk matter phenomena associated with strange and heavy quarks, • QCD phase structure, • Collectivity in small systems, • Strangeness in astrophysics,• Open questions and new developments.

Describing the Dynamics of the Quark-gluon Plasma Using Relativistic Viscous Hydrodynamics

Describing the Dynamics of the Quark-gluon Plasma Using Relativistic Viscous Hydrodynamics PDF

Author: Mohammad N. Yaseen

Publisher:

Published: 2016

Total Pages: 83

ISBN-13:

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When heavy nuclei collide at ultra-relativistic energies, their nuclear matter will melt producing what is known as the Quark-Gluon Plasma (QGP); a new state of matter that has been produced at the Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory (BNL) and Super Proton Synchrotron (LHC) in European Organization for Nuclear Research (CERN). Scientists now think that this matter filled the entire universe during the first micro second after the Big Bang. According to the experimental data, this matter acts like a nearly perfect liquid. This study requires a quantitatively precise theoretical framework to describe the dynamical evolution of the fireball produced by the collision. The equations that control the fireball expansion cannot be solved analytically. As a result, scientists must solve these equations numerically. The main goal of this thesis is to find precise numerical solutions for these equations. This is complicated by the fact that when using fluctuating initial conditions, discontinuities may be present which cause problems for standard centered differences schemes. To fix this problem, we will use the following two numerical methods: LAX and weighted LAX.

Hydrodynamic Description of the Baryon-charged Quark-gluon Plasma

Hydrodynamic Description of the Baryon-charged Quark-gluon Plasma PDF

Author: Lipei Du

Publisher:

Published: 2021

Total Pages: 0

ISBN-13:

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One of the primary goals of nuclear physics is studying the phase diagram of Quantum Chromodynamics, where a hypothetical critical point serves as a landmark. A systematic model-data comparison of heavy-ion collisions at center-of-mass energies between 1 and 100 GeV per nucleon is essential for locating the critical point and the phase boundary between the deconfined quark-gluon plasma and the confined hadron resonance gas. At these energies the net baryon density of the system can be high and critical fluctuations can become essential in the presence of the critical point. Simulating their dynamical evolution thus becomes an indispensable part of theoretical modeling. In this thesis we first present the (3+1)-dimensional relativistic hydrodynamic code BEShydro, which solves the equations of motion of second-order Denicol-Niemi-Molnar-Rischke theory, including bulk and shear viscous components as well as baryon diffusion current. We then study the effects caused by the baryon diffusion on the longitudinal dynamics and on the phase diagram trajectories of fluid cells at different space-time rapidities of the system, and how they are affected by critical dynamics near the critical point. We finally explore the evolution of non-hydrodynamic slow processes describing long wavelength critical fluctuations near the critical point, by extending the conventional hydrodynamic description by coupling it to additional explicitly evolving slow modes, and their back-reaction to the bulk matter properties.

Introduction to Particle and Astroparticle Physics

Introduction to Particle and Astroparticle Physics PDF

Author: Alessandro De Angelis

Publisher: Springer

Published: 2015-09-05

Total Pages: 680

ISBN-13: 8847026881

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This book, written by researchers who had been professionals in accelerator physics before becoming leaders of groups in astroparticle physics, introduces both fields in a balanced and elementary way, requiring only a basic knowledge of quantum mechanics on the part of the reader. The new profile of scientists in fundamental physics ideally involves the merging of knowledge in astroparticle and particle physics, but the duration of modern experiments is such that people cannot simultaneously be practitioners in both. Introduction to Particle and Astroparticle Physics is designed to bridge the gap between the fields. It can be used as a self-training book, a consultation book, or a textbook providing a “modern” approach to particles and fundamental interactions.

Understanding the Origin of Matter

Understanding the Origin of Matter PDF

Author: David Blaschke

Publisher: Springer Nature

Published: 2022-09-14

Total Pages: 397

ISBN-13: 3030954919

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This book aims at providing a solid basis for the education of the next generation of researchers in hot, dense QCD (Quantum ChromoDynamics) matter. This is a rapidly growing field at the interface of the smallest, i.e. subnuclear physics, and the largest scales, namely astrophysics and cosmology. The extensive lectures presented here are based on the material used at the training school of the European COST action THOR (Theory of hot matter in relativistic heavy-ion collisions). The book is divided in three parts covering ultrarelativistic heavy-ion collisions, several aspects related to QCD, and simulations of QCD and heavy-ion collisions. The scientific tools and methods discussed provide graduate students with the necessary skills to understand the structure of matter under extreme conditions of high densities, temperatures, and strong fields in the collapse of massive stars or a few microseconds after the big bang. In addition to the theory, the set of lectures presents hands-on material that includes an introduction to simulation programs for heavy-ion collisions, equations of state, and transport properties.

Phenomenology of Ultra-relativistic Heavy-ion Collisions

Phenomenology of Ultra-relativistic Heavy-ion Collisions PDF

Author:

Publisher: World Scientific

Published: 2010

Total Pages: 437

ISBN-13: 9814280682

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An introduction to the main ideas used in the physics of ultra-realistic heavy-ion collisions, this book covers topics such as hot and dense matter and the formation of the quark-gluon plasma in present and future heavy-ion experiments