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We investigate the properties of highly compressible turbulence, the compressibility arising from a small effective polytropic exponent $\gamma_e$ due to cooling. In the limit of small $\gamma_e$, the density jump at shocks is shown to be…

天体物理学 · 物理学 2009-10-28 E. Vazquez-Semadeni , T. Passot , A. Pouquet

Observational evidence in space and astrophysical plasmas with long collisional mean free path suggests that more massive charged particles may be preferentially heated. One possible mechanism for this is the turbulent cascade of energy…

等离子体物理 · 物理学 2018-01-15 M. Barnes , P. Abiuso , W. Dorland

Signs of turbulence have been observed at the relativistic heavy ion collision at high collision energies. We study the signatures of turbulence in this system and find that there are significant departures from isotropic turbulence in the…

核理论 · 物理学 2022-07-13 Abhisek Saha , Soma Sanyal

We address the formation of giant clumps in violently unstable gas-rich disc galaxies at cosmic noon. While these are commonly thought to originate from gravitational Toomre instability, cosmological simulations have indicated that clumps…

Massive galaxy clusters are filled with a hot, turbulent and magnetized intra-cluster medium. Still forming under the action of gravitational instability, they grow in mass by accretion of supersonic flows. These flows partially dissipate…

宇宙学与河外天体物理 · 物理学 2015-07-09 Francesco Miniati , Andrey Beresnyak

The continuity equation requires that energy released in nuclear fusion flows away from the point of interaction and is not immediately thermalised into the CMB. It is seen that consequently the bulk of thermo-nuclear energy released in BBN…

综合物理 · 物理学 2019-08-20 Charles Francis

When a planar shock wave interacts with a random pattern of pre-shock density non-uniformities, it generates an anisotropic turbulent velocity/vorticity field. This turbulence plays an important role at the early stages of the mixing…

流体动力学 · 物理学 2015-05-19 Cesar Huete Ruiz de Lira

The reheating of the universe after hybrid inflation proceeds through the nucleation and subsequent collision of large concentrations of energy density in the form of bubble-like structures moving at relativistic speeds. This generates a…

广义相对论与量子宇宙学 · 物理学 2008-01-29 Juan Garcia-Bellido , Daniel G. Figueroa

We show that rapidly-spinning black holes can display turbulent gravitational behavior which is mediated by a new type of parametric instability. This instability transfers energy from higher temporal and azimuthal spatial frequencies to…

广义相对论与量子宇宙学 · 物理学 2015-03-05 Huan Yang , Aaron Zimmerman , Luis Lehner

In the modern understanding of turbulence, a central concept is the existence of cascades of excitations from large to small lengthscales, or vice-versa. This concept was introduced in 1941 by Kolmogorov and Obukhov, and the phenomenon has…

量子气体 · 物理学 2016-11-04 Nir Navon , Alexander L. Gaunt , Robert P. Smith , Zoran Hadzibabic

Turbulence is ubiquitous in astrophysical fluids. Therefore it is necessary to study magnetic reconnection in turbulent environments. The model of fast turbulent reconnection proposed in Lazarian & Vishniac 1999 has been successfully tested…

星系天体物理 · 物理学 2011-12-16 A. Lazarian

The theory of gravitational structure formation in astrophysics and cosmology is revised based on real fluid behavior and turbulent mixing theory. Gibson's 1996-1998 theory balances fluid mechanical forces with gravitational forces and…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

The study of particle creation phenomena at the expense of the gravitational field is of great research interest. It might solve the cosmological puzzle single-handedly, without the need for either dark energy or the modified theory of…

广义相对论与量子宇宙学 · 物理学 2018-06-26 Abhik Kumar Sanyal , Subhra Debnath

The giant, star forming clumps in gas-rich, high redshift disks are commonly assumed to form due to gravitational instabilities, in which protoclumps have a Toomre-$Q$ parameter less than unity. However, some cosmological simulations show…

The transition from laminar to turbulent flow is an immensely important topic that is still being studied. Here we show that complex plasmas, i.e., microparticles immersed in a low temperature plasma, make it possible to study the…

等离子体物理 · 物理学 2024-01-30 Eshita Joshi , Markus H Thoma , Mierk Schwabe

The standard model for gravitational structure formation in astrophysics, astronomy, and cosmology is questioned. Cold dark matter (CDM) hierarchical clustering cosmology neglects particle collisions, viscosity, turbulence and diffusion and…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

Due to its ubiquitous presence, turbulence is often invoked to explain the origin of nonthermal particles in astrophysical sources of high-energy emission. With particle-in-cell simulations, we study decaying turbulence in…

高能天体物理现象 · 物理学 2018-12-21 Luca Comisso , Lorenzo Sironi

We investigate properties of turbulence and turbulent transport of non-inertial particles described in terms of turbulent thermal diffusion in strongly inhomogeneous and anisotropic convection forced by two similar turbulence generators…

流体动力学 · 物理学 2025-12-17 E. Zarbib , E. Elmakies , O. Shildkrot , N. Kleeorin , A. Levy , I. Rogachevskii

Since detonation is the only established theory that allows rapid burning producing a high pressure that can be sustained in open areas, the generally accepted opinion was that the mechanism explaining the high rate of combustion in dust…

化学物理 · 物理学 2019-01-01 Michael Liberman , Nathan Kleeorin , Igor Rogachevskii , Nils Haugen

Our Universe has multiple examples of unexplained gravitational losses in black holes and neutron stars. As all of the space is squeezed out, nucleons are not easily compressible further. Gravitational loss will allow galactic black holes…

天体物理学 · 物理学 2024-12-24 David E. Rosenberg