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The technology of lined rock cavern (LRC) with great geographical flexibility is a promising, cost-effective solution to underground hydrogen storage. However, the air-tight steel tanks used in this technology are susceptible to material…

计算物理 · 物理学 2025-03-13 Chenxi Zhao , Haiyang Yu , Zixin Zhang , Qinghua Lei

A decrease of fracture toughness of irradiated materials is usually observed, as reported for austenitic stainless steels in Light Water Reactors (LWRs) or copper alloys for fusion applications. For a wide range of applications (e.g.…

材料科学 · 物理学 2018-03-13 P. O. Barrioz , J. Hure , B. Tanguy

(abridged) We use a one-dimensional hydrodynamical code to investigate the effects of preheating on gas accretion and cooling in cold dark matter halos. In the absence of radiative cooling, preheating reduces the amount of gas that can be…

天体物理学 · 物理学 2008-11-26 Yu Lu , H. J. Mo

A reactive fluid dissolving the surrounding rock matrix can trigger an instability in the dissolution front, leading to spontaneous formation of pronounced channels or wormholes. Theoretical investigations of this instability have typically…

地球物理 · 物理学 2011-03-22 Piotr Szymczak , Anthony J. C. Ladd

If a liquid is cooled rapidly to form a glass, its structural relaxation becomes retarded, producing a drastic increase in viscosity. In two dimensions, strong long-wavelength fluctuations persist, even at low temperature, making it…

软凝聚态物质 · 物理学 2019-12-25 Hayato Shiba , Takeshi Kawasaki , Kang Kim

Galactic spiral shocks are dominant morphological features and believed to be responsible for substructure formation within spiral arms in disk galaxies. They can also contribute a substantial amount of kinetic energy to the interstellar…

星系天体物理 · 物理学 2015-05-19 Chang-Goo Kim , Woong-Tae Kim , Eve C. Ostriker

Most massive galaxies host a supermassive black hole at their centre. Matter accretion creates an active galactic nucleus (AGN), forming a relativistic particle wind. The wind heats and pushes the interstellar medium, producing…

星系天体物理 · 物理学 2024-09-23 Martynas Laužikas , Kastytis Zubovas

The process of frictional rupture, i.e. the failure of frictional systems, abounds in the technological and natural world around us, ranging from squealing car brake pads to earthquakes along geological faults. A general framework for…

Condensed planets contract or expand as their temperature changes. With the exception of the effect of phase changes, this phenomenon is generally interpreted as being solely related to the thermal expansivity of the planet's components.…

地球与行星天体物理 · 物理学 2024-04-23 Yanick Ricard , Frédéric Chambat

Drying induced cracking of concrete surfaces and repair layers is a common problem. A principal cause for this type of cracking is the moisture and resulting contraction gradient that develops in the cement paste matrix upon drying. This…

材料科学 · 物理学 2015-09-17 Jan Bisschop , Falk K. Wittel

The relaxation of polymers around and below their glass transition temperature is governed by a range of correlated unit processes with a wide range of timescales. The fast deformation rates of shock loading can negate a significant…

材料科学 · 物理学 2022-07-27 Jalen Macatangay , Brenden W. Hamilton , Alejandro Strachan

Star formation generally proceeds inside-out, with overdense regions inside protostellar cores collapsing rapidly and progressively less dense regions following later. Consequently, a small protostar will form early in the evolution of a…

天体物理学 · 物理学 2009-11-11 Mark R. Krumholz

Theoretically, inflowing filaments of gas are one of the main causes of growth for a galaxy. Nonetheless, observationally, probing ongoing gas accretion is challenging. As part of the Gas Stripping Phenomena in galaxies with MUSE (GASP)…

星系天体物理 · 物理学 2018-02-22 B. Vulcani , B. M. Poggianti , A. Moretti , M. Mapelli , G. Fasano , J. Fritz , Y. Jaffe' , D. Bettoni , M. Gullieuszik , C. Bellhouse

Two puzzles associated with open clusters have attracted a lot of attention -- their formation, with densities and velocity dispersions that are not too different from those of the star forming regions in the Galaxy, given that the observed…

星系天体物理 · 物理学 2015-06-15 K. Indulekha

Erosion and deposition during flow through porous media can lead to large erosive bursts that manifest as jumps in permeability and pressure loss. Here we reveal that the cause of these bursts is the re-opening of clogged pores when the…

流体动力学 · 物理学 2017-09-26 Robin Jäger , Miller Mendoza , Hans J. Herrmann

The efficiency of thermal pressurisation as a dynamic weakening mechanism relies on the thermal and hydraulic properties of the rocks forming the fault core. Here, we assess the effectiveness of thermal pressurisation by comparing…

地球物理 · 物理学 2019-01-03 Nicolas Brantut , Thomas M. Mitchell

We report on the results of the first 3D SPH simulation of massive, gravitationally unstable protoplanetary disks with radiative transfer. We adopt a flux-limited diffusion scheme justified by the high opacity of most of the disk. The…

天体物理学 · 物理学 2009-11-11 Lucio Mayer , Graeme Lufkin , Thomas Quinn , James Wadsley

The drying of a colloidal dispersion can result in a gel phase defined as a porous matrix saturated in solvent. During the drying process, high mechanical stresses are generated. When these stresses exceed the strength of the material, they…

软凝聚态物质 · 物理学 2013-02-15 François Boulogne , Frédérique Giorgiutti-Dauphiné , Ludovic Pauchard

I calculate the action of a satellite, infalling through dynamical friction, on a coplanar gaseous disk of finite radial extent. The disk tides, raised by the infalling satellite, couple the satellite and disk. Dynamical friction acting on…

天体物理学 · 物理学 2009-11-13 P. Chang

Since it is difficult to apply the existing method of friction and heat flux decomposition on the complex surface, a combined decomposition method of friction and heat flux with clear physical interpretation is proposed, which is based on…

流体动力学 · 物理学 2023-03-16 Mingzhi Tang , Wenfeng Zhou , Yanchao Hu , Gang Wang , Ming Fang , Yan-guang Yang