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Particle-resolved direct numerical simulation (PR-DNS) is performed for turbulent open channel flow over a smooth horizontal wall with a vertical cylinder and a dilute set of mobile, heavy, spherical particles. At the chosen parameter point…

流体动力学 · 物理学 2026-04-20 Leo Bürk , Artjom Hermann , Markus Weyrauch , Markus Uhlmann

The magnetization of superconducting samples is influenced by their porosity. In addition to structural modifications and improved cooling, the presence of pores also plays a role in trapping magnetic flux. Pores have an impact on the…

超导电性 · 物理学 2024-03-19 Denis Gokhfeld

After the initial stage of fast expanding of the hot Universe comes epoch of temperature fall and subsequent formation of dense clouds of hydrogen. Due to process of accretion some of this clouds became compact objects. Initially accretion…

等离子体物理 · 物理学 2016-11-14 Zlatan Dimitrov Dimitrov

Space-filling assemblies of athermal hydrophobic particles floating at an air-water interface, called particle rafts, are shown to undergo an unusual phase transition between two i.e., a low density `less-rigid and a high density…

无序系统与神经网络 · 物理学 2015-06-11 Atul Varshney , A. Sane , Shankar Ghosh , S. Bhattacharya

The large-scale structures in the ocean and the atmosphere are in geostrophic balance, and a conduit must be found to channel the energy to the small scales where it can be dissipated. In turbulence this takes the form of an energy cascade,…

流体动力学 · 物理学 2018-02-20 N. E. Sujovolsky , P. D. Mininni , A. Pouquet

From a new anti-parallel initial condition using long vortices, three-dimensional turbulence forms after two reconnection steps and the formation of at least one vortex ring. The long domain is needed in order to accommodate the multiple…

流体动力学 · 物理学 2013-01-21 Robert M. Kerr

Tidal interaction between a gaseous disk and a massive orbiting perturber is known to result in angular momentum exchange between them. Understanding astrophysical manifestations of this coupling such as gap opening by planets in…

地球与行星天体物理 · 物理学 2015-06-03 Roman R. Rafikov , Cristobal Petrovich

A dynamical phase transition from reversible to irreversible behavior occurs when particle suspensions are subjected to uniform oscillatory shear, even in the Stokes flow limit. We consider a more general situation with non-uniform strain…

流体动力学 · 物理学 2015-05-18 Jeffrey S. Guasto , Andrew S. Ross , J. P. Gollub

A colloidal particle driven by externally actuated rotation can self-propel parallel to a rigid boundary by exploiting the hydrodynamic coupling that surfaces induce between translation and rotation. As such a roller moves along the…

流体动力学 · 物理学 2020-02-20 Alexander Chamolly , Eric Lauga , Soichiro Tottori

Turbo-generators shafts are manufactured through the extrusion process. This results in the formation of weak planes along the extrusion process. It has been observed that large longitudinal cracks often form in these shafts before any…

材料科学 · 物理学 2018-10-05 Mohsen Nabian , Hamid Nayeb Hashemi

An extended gravitational object embedded in a parent system comprised of gas and collisionless particles may undergo both dynamical friction (DF) and mass loss by tidal forces. If the object is compact enough, it can increase its mass…

星系天体物理 · 物理学 2018-10-17 F. J. Sanchez-Salcedo , R. O. Chametla

Traveling waves describe diverse natural phenomena from crystal growth in physics to range expansions in biology. Two classes of waves exist with very different properties: pulled and pushed. Pulled waves are driven by high growth rates at…

种群与进化 · 定量生物学 2018-02-27 Gabriel Birzu , Oskar Hallatschek , Kirill S. Korolev

The mechanism for flow generation in dense degenerate stellar atmospheres is suggested when the electron gas is degenerate and ions are assumed to be classical. It is shown, that there is a catastrophe in such system -- fast flows are…

太阳与恒星天体物理 · 物理学 2017-08-15 A. A. Barnaveli , N. L. Shatashvili

Feedback from active galactic nuclei (AGN) has often been invoked both in simulations and in interpreting observations for regulating star formation and quenching cooling flows in massive galaxies. AGN activity can, however, also…

星系天体物理 · 物理学 2015-12-16 Rebekka Bieri , Yohan Dubois , Joseph Silk , Gary Mamon , Volker Gaibler

We perform a detailed analytical and numerical study of the dynamics of perturbations (vortex/aperiodic mode, Rossby and spiral-density waves) in 2D compressible disks with a Keplerian law of rotation. We draw attention to the process of…

天体物理学 · 物理学 2009-11-10 G. Bodo , G. Chagelishvili , G. Murante , A. Tevzadze , P. Rossi , A. Ferrari

The forced motion of superfluid vortices in shear oscillations of rotating solid neutron star matter produces damping of the mode. A simple model of the unpinning and repinning processes is described, with numerical calculations of the…

天体物理学 · 物理学 2009-11-07 P. B. Jones

Direct numerical simulation of open channel flow over a geometrically rough wall has been performed at a bulk Reynolds number of approximately 2900. The wall consisted of a layer of spheres in a square arrangement. Two cases have been…

流体动力学 · 物理学 2013-01-28 Clemens Chan-Braun , Manuel García-Villalba , Markus Uhlmann

Jellyfish galaxies are an intriguing snapshot of galaxies undergoing ram-pressure stripping (RPS) in dense environments, showing spectacular star-forming knots in their disks and tails. We study the ionized gas properties of five jellyfish…

星系天体物理 · 物理学 2022-11-30 Jeong Hwan Lee , Myung Gyoon Lee , Jae Yeon Mun , Brian S. Cho , Jisu Kang

Galaxy evolution can be dramatically affected by the environment, especially by the dense environment of a galaxy cluster. Recent observational studies show that massive galaxies undergoing strong ram pressure stripping (RPS) also show an…

星系天体物理 · 物理学 2023-05-03 Nina Akerman , Stephanie Tonnesen , Bianca M. Poggianti , Rory Smith , Antonino Marasco

Turbulent water motions are important for the exchange of momentum, heat, nutrients, and suspended matter including sediments in the deep-sea that is generally stably stratified in density. To maintain ocean-density stratification, an…

大气与海洋物理 · 物理学 2024-08-14 Hans van Haren , Henk de Haas