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相关论文: The Unstable Glasma

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We present first results for 3+1-D simulations of SU(2) Yang-Mills equations for matter expanding into the vacuum after a heavy ion collision. Violations of boost invariance cause a Weibel instability leading soft modes to grow with proper…

高能物理 - 唯象学 · 物理学 2010-04-06 Paul Romatschke , Raju Venugopalan

We extensively study the growing behavior of the energy and the pressure components depending on the space-time rapidity in the framework of the Glasma, which describes the early-time dynamics in the ultra-relativistic heavy-ion collisions.…

高能物理 - 唯象学 · 物理学 2015-05-28 Kenji Fukushima , Francois Gelis

Based on hep-ph/0510121, we discuss further the numerical study of classical SU(2) 3+1-D Yang-Mills equations for matter produced in a high energy heavy ion collision. The growth of the amplitude of fluctuations as $\exp{(\Gamma…

高能物理 - 唯象学 · 物理学 2009-11-11 Paul Romatschke , Raju Venugopalan

The quark gluon plasma as produced in heavy ion collisions is exposed to early anisotropies in momentum space due to its rapid expansion. Such anisotropies can lead to non-abelian plasma instabilities, driven by unstable gluonic modes that…

高能物理 - 唯象学 · 物理学 2015-06-11 Andreas Ipp

We study the evolution of quantum fluctuations in the Glasma created immediately after the collision of heavy nuclei. It is shown how the presence of instabilities leads to an enhancement of non-linear interactions among initially small…

高能物理 - 唯象学 · 物理学 2013-05-30 J. Berges , S. Schlichting

We study (3+1)D kinetic (Boltzmann-Vlasov) equations for relativistic plasma particles in a one-dimensionally expanding geometry motivated by ultrarelativistic heavy-ion collisions. We set up local equations in terms of Yang-Mills…

高能物理 - 唯象学 · 物理学 2008-11-26 Paul Romatschke , Anton Rebhan

We study the coupled Wong Yang-Mills equations for both U(1) and SU(2) gauge groups and anisotropic particle momentum distributions numerically on a lattice. For weak fields with initial energy density much smaller than that of the…

高能物理 - 唯象学 · 物理学 2008-11-26 Adrian Dumitru , Yasushi Nara

Non-Abelian plasma instabilities play a crucial role in the nonequilibrium dynamics of a weakly coupled quark-gluon plasma and they importantly modify the standard perturbative bottom-up thermalization scenario in heavy-ion collisions.…

高能物理 - 唯象学 · 物理学 2008-11-26 Anton Rebhan , Michael Strickland , Maximilian Attems

We study the dynamics of nonequilibrium instabilities in anisotropically expanding systems. The most prominent example of such a system is the 'Glasma' in the context of relativistic heavy-ion collision experiments, where the expansion is a…

高能物理 - 唯象学 · 物理学 2013-05-30 Jürgen Berges , Kirill Boguslavski , Sören Schlichting

We investigate the instability of classical Yang-Mills field in an expanding geometry under a color magnetic background field within the linear regime. We consider homogeneous, boost-invariant and time-dependent color magnetic fields…

高能物理 - 唯象学 · 物理学 2016-07-27 Shoichiro Tsutsui , Teiji Kunihiro , Akira Ohnishi

We consider the SU(2) Glasma with gaussian fluctuations and study its evolution by means of classical Yang-Mills equations solved numerically on a lattice. Neglecting in this first study the longitudinal expansion we follow the evolution of…

核理论 · 物理学 2018-04-18 M. Ruggieri , J. H. Liu , L. Oliva. G. X. Peng , V. Greco

We study the (3+1)-dimensional evolution of non-Abelian plasma instabilities in the presence of a longitudinally expanding background of hard particles using the discretized hard loop framework. The free streaming background dynamically…

高能物理 - 唯象学 · 物理学 2013-01-15 Maximilian Attems , Anton Rebhan , Michael Strickland

The non-equilibrium early time evolution of an ultra-relativistic heavy ion collision is often described by classical lattice Yang-Mills theory, starting from the colour glass condensate (CGC) effective theory with an anisotropic energy…

高能物理 - 格点 · 物理学 2019-05-01 Owe Philipsen , Björn Wagenbach , Savvas Zafeiropoulos

We numerically investigate gauge field instabilities in anisotropic SU(2) plasmas using weak field initial conditions. The growth of unstable modes is stopped by non-abelian effects for moderate anisotropy. If we increase the anisotropy the…

高能物理 - 唯象学 · 物理学 2008-11-26 D. Bodeker , K. Rummukainen

Under suitable non-equilibrium conditions QCD plasma can develop plasma instabilities, where some modes of the plasma grow exponentially. It has been argued that these instabilities can play a significant role in the thermalisation of the…

高能物理 - 格点 · 物理学 2008-11-26 Dietrich Bodeker , Kari Rummukainen

A system of gluon fields produced in the earliest phase of relativistic heavy-ion collisions, which is called `glasma', can be described in terms of classical fields. Initially there are chromoelectric and chromomagnetic fields along the…

高能物理 - 唯象学 · 物理学 2023-12-19 Sylwia Bazak , Stanislaw Mrowczynski

The gravitational instability of Yang-Mills cosmologies is numerically studied with the hamiltonian formulation of the spherically symmetric Einstein-Yang-Mills equations with SU(2) gauge group. On the short term, the expansion dilutes the…

广义相对论与量子宇宙学 · 物理学 2010-11-19 A. Fuzfa

Non-Abelian plasma instabilities may be responsible for the fast apparent quark-gluon thermalization in relativistic heavy-ion collisions if their exponential growth is not hindered by nonlinearities. We study the real-time evolution of…

高能物理 - 唯象学 · 物理学 2009-12-04 Anton Rebhan , Paul Romatschke , Michael Strickland

A homogeneous color magnetic field is known to be unstable for the fluctuations perpendicular to the field in the color space (the Nielsen-Olesen instability). We argue that these unstable modes, exponentially growing, generate an azimuthal…

高能物理 - 唯象学 · 物理学 2009-08-17 H. Fujii , K. Itakura , A. Iwazaki

We simulate the 3+1 D classical Yang-Mills dynamics of the collisions of longitudinally extended nuclei, described by eikonal color charges in the Color Glass Condensate framework. By varying the longitudinal thickness of the colliding…

高能物理 - 唯象学 · 物理学 2021-02-26 Soeren Schlichting , Pragya Singh
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