中文
相关论文

相关论文: Turbulence in the Ocean, Atmosphere, Galaxy, and U…

200 篇论文

Turbulence is defined as an eddy-like state of fluid motion where the inertial-vortex forces of the eddies are larger than all the other forces that tend to damp the eddies out. Fossil turbulence is a perturbation produced by turbulence…

流体动力学 · 物理学 2012-04-30 Carl H. Gibson

Turbulence is defined as an eddy-like state of fluid motion where the inertial-vortex forces of the eddies are larger than any of the other forces that tend to damp the eddies out. Energy cascades of irrotational flows from large scales to…

天体物理学 · 物理学 2009-11-10 Pak Tao Leung , Carl H. Gibson

Turbulence and turbulent mixing in natural fluids begins with big bang turbulence powered by spinning combustible combinations of Planck particles and Planck antiparticles. Particle prograde accretions on a spinning pair releases 42% of the…

宇宙学与河外天体物理 · 物理学 2015-05-19 Carl H. Gibson

Turbulence is defined as an eddy-like state of fluid motion where the inertial-vortex forces of the eddies are larger than any other forces that tend to damp the eddies out. By this definition, turbulence always cascades from small scales…

流体动力学 · 物理学 2012-03-28 Carl H. Gibson

Fossil turbulence processes are central to turbulence, turbulent mixing, and turbulent diffusion in the ocean and atmosphere, in astrophysics and cosmology, and in most other natural flows. George Gamov suggested in 1954 that galaxies might…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

Turbulence is defined as an eddy-like state of fluid motion where the inertial-vortex forces of the eddies are larger than any other forces that tend to damp the eddies out. By this definition, turbulence always cascades from small scales…

综合物理 · 物理学 2012-12-21 Carl H Gibson

Chaotic, eddy-like motions dominated by inertial-vortex forces begin immediately at Planck scales in a hot big-bang cosmological model. This quantum-gravitational-dynamics epoch produced not only the first space-time-energy of the universe…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

Turbulence and turbulent mixing of temperature powered the big bang formation of the universe at Planck length, time, and temperature scales. Planck-Kerr inertial-vortex forces balanced Planck gravitational forces to produce Planck…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

The gravitational hydrodynamics of the primordial plasma with neutrino hot dark matter is considered as a challenge to the bottom-up cold dark matter paradigm. Viscosity and turbulence induce a top-down fragmentation scenario before and at…

宇宙学与河外天体物理 · 物理学 2009-12-08 Theo M. Nieuwenhuizen , Carl H. Gibson , Rudy E. Schild

Turbulence is ever produced in the low-viscosity/large-scale fluid flows by the velocity shears and, in unstable stratification, by buoyancy forces. It is commonly believed that both mechanisms produce the same type of chaotic motions,…

大气与海洋物理 · 物理学 2022-01-12 Sergej S Zilitinkevich , Evgeny Kadantsev , Irina Repina , Evgeny Mortikov , Andrey Glazunov

Was the primordial universe turbulent or non-turbulent soon after the Big Bang? How did the hydrodynamic state of the early universe affect the formation of structure from gravitational forces, and how did the formation of structure by…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

Extreme conditions in natural flows are examined, starting with a turbulent big bang. A hydro-gravitational-dynamics cosmology model is adopted. Planck-Kerr turbulence instability causes Planck-particle turbulent combustion. Inertial-vortex…

宇宙学与河外天体物理 · 物理学 2010-12-13 R. Norris Keeler , Carl H. Gibson

The formation of astrophysical structures, such as stars, compact objects but also galaxies, entail an,enhancement of densities by many orders of magnitude which occurs through gravitational collapse. The role played by turbulence during…

星系天体物理 · 物理学 2021-11-03 Patrick Hennebelle

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 first structures were proto-voids formed in the primordial plasma. Viscous and weak turbulence forces balanced gravitational forces when the scale of causal connection at time 30,000 years matched the viscous and turbulent Schwarz…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

The equilibrium state of a turbulent clumpy gas disk is analytically investigated. The disk consists of distinct self-gravitating clouds. Gravitational cloud-cloud interactions transfer energy over spatial scales and produce a viscosity,…

天体物理学 · 物理学 2009-11-07 B. Vollmer , T. Beckert

There is a clear distinction between simple laminar and complex turbulent fluids. But in some cases, as for the nocturnal planetary boundary layer, a stable and well-ordered flow can develop intense and sporadic bursts of turbulent activity…

流体动力学 · 物理学 2015-06-17 C. Rorai , P. D. Mininni , A. Pouquet

The first turbulent combustion arises in a hot big bang cosmological model Gibson (2004) where nonlinear exothermic turbulence permitted by quantum mechanics, general relativity, multidimensional superstring theory, and fluid mechanics…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

The role of turbulence and turbulent mixing in the formation and evolution of the early universe is examined. A new quantum-gravitational-dynamics model suggests that the mechanism of the hot big bang is functionally equivalent to the…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

In recent works, we proposed a hypothesis, according to which turbulence in gases is created by the mean field effect of an intermolecular potential. We discovered that, in a numerically simulated inertial flow, turbulent solutions indeed…

流体动力学 · 物理学 2023-10-18 Rafail V. Abramov
‹ 上一页 1 2 3 10 下一页 ›