High-energy nuclear collisions produce a nonequilibrium plasma of quarks and gluons which thermalizes and exhibits hydrodynamic flow. There are currently no practical frameworks to connect the early particle production in classical field simulations to the subsequent hydrodynamic evolution. We build such a framework using nonequilibrium Green’s functions, calculated in QCD kinetic theory, to propagate the initial energy-momentum tensor to the hydrodynamic phase. We demonstrate that this approach can be easily incorporated into existing hydrodynamic simulations, leading to stronger constraints on the energy density at early times and the transport properties of the QCD medium. Based on (conformal) scaling properties of the Green’s functions,...
Relativistic hydrodynamics simulations of quark-gluon plasma play a pivotal role in our understandin...
Giacalone G, Mazeliauskas A, Schlichting S. Hydrodynamic attractors, initial state energy and partic...
We develop a macroscopic description of the space-time evolution of the energy-momentum tensor durin...
Kurkela A, Mazeliauskas A, Paquet J-F, Schlichting S, Teaney D. Matching the Nonequilibrium Initial ...
High-energy nuclear collisions produce a nonequilibrium plasma of quarks and gluons which thermalize...
The produced matter in the high energy nuclear collisions reinteracts and forms a plasma which ultim...
Kamata S, Martinez M, Plaschke P, Ochsenfeld S, Schlichting S. Hydrodynamization and nonequilibrium ...
Mazeliauskas A, Kurkela A, Paquet J-F, Schlichting S, Teaney D. Matching the non-equilibrium initial...
We use effective kinetic theory, accurate at weak coupling, to simulate the pre-equilibrium evolutio...
Mazeliauskas A, Kurkela A, Paquet J-F, Schlichting S, Teaney D. Initial conditions for heavy ion col...
Evolution of hot and dense nuclear matter produced in central Au+Au collisions at energies of NICA, ...
Relativistic hydrodynamics simulations of quark-gluon plasma play a pivotal role in our understandin...
International audienceWe exploit the concept of hydrodynamic attractors to establish a macroscopic d...
International audienceWe exploit the concept of hydrodynamic attractors to establish a macroscopic d...
International audienceWe exploit the concept of hydrodynamic attractors to establish a macroscopic d...
Relativistic hydrodynamics simulations of quark-gluon plasma play a pivotal role in our understandin...
Giacalone G, Mazeliauskas A, Schlichting S. Hydrodynamic attractors, initial state energy and partic...
We develop a macroscopic description of the space-time evolution of the energy-momentum tensor durin...
Kurkela A, Mazeliauskas A, Paquet J-F, Schlichting S, Teaney D. Matching the Nonequilibrium Initial ...
High-energy nuclear collisions produce a nonequilibrium plasma of quarks and gluons which thermalize...
The produced matter in the high energy nuclear collisions reinteracts and forms a plasma which ultim...
Kamata S, Martinez M, Plaschke P, Ochsenfeld S, Schlichting S. Hydrodynamization and nonequilibrium ...
Mazeliauskas A, Kurkela A, Paquet J-F, Schlichting S, Teaney D. Matching the non-equilibrium initial...
We use effective kinetic theory, accurate at weak coupling, to simulate the pre-equilibrium evolutio...
Mazeliauskas A, Kurkela A, Paquet J-F, Schlichting S, Teaney D. Initial conditions for heavy ion col...
Evolution of hot and dense nuclear matter produced in central Au+Au collisions at energies of NICA, ...
Relativistic hydrodynamics simulations of quark-gluon plasma play a pivotal role in our understandin...
International audienceWe exploit the concept of hydrodynamic attractors to establish a macroscopic d...
International audienceWe exploit the concept of hydrodynamic attractors to establish a macroscopic d...
International audienceWe exploit the concept of hydrodynamic attractors to establish a macroscopic d...
Relativistic hydrodynamics simulations of quark-gluon plasma play a pivotal role in our understandin...
Giacalone G, Mazeliauskas A, Schlichting S. Hydrodynamic attractors, initial state energy and partic...
We develop a macroscopic description of the space-time evolution of the energy-momentum tensor durin...