2020
DOI: 10.1021/acs.jpcc.0c05241
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Effects of the Growth Kinetics on Solute Diffusion in Porous Films

Abstract: For the development of porous materials with improved transport properties, a key ingredient is to determine the relations between growth kinetics, structure, and transport parameters. Here, we address these relations by studying solute diffusion through three-dimensional porous films produced by deposition models with controlled thickness and porosity. A competition between pore formation by lateral particle aggregation and surface relaxation that favors compaction is simulated by the lattice models of ballis… Show more

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Cited by 4 publications
(3 citation statements)
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“…It is also interesting to note that Draco was considered as a challenging case for SIDM [61,62] as it has the highest dark matter content among the Milky Way satellites, but both dark matter self-interactions and tidal interactions are commonly expected to produce a shallow density core for a satellite galaxy. Recent works show the interplay of the two effects could actually lead to an opposite consequence, resulting in a high central density, due to the onset of SIDM core collapse [33,34,[63][64][65]. Ref.…”
Section: Applications To Dracomentioning
confidence: 99%
“…It is also interesting to note that Draco was considered as a challenging case for SIDM [61,62] as it has the highest dark matter content among the Milky Way satellites, but both dark matter self-interactions and tidal interactions are commonly expected to produce a shallow density core for a satellite galaxy. Recent works show the interplay of the two effects could actually lead to an opposite consequence, resulting in a high central density, due to the onset of SIDM core collapse [33,34,[63][64][65]. Ref.…”
Section: Applications To Dracomentioning
confidence: 99%
“…Thus SIDM has a natural mechanism in triggering gravitational stabilities, a necessary condition to form a black hole. Recent studies also show that SIDM is favored for explaining diverse dark matter distributions over a wide range of galactic systems [25,[35][36][37][38][39][40][41][42][43][44][45]. It is intriguing to explore an SIDM scenario that may explain the origin of the high-z SMBHs and observations of galaxies at z ∼ 0.…”
Section: Introductionmentioning
confidence: 99%
“…Without stars, the collapse would not occur within 6 Gyr unless c 200 is 6σ higher than the median, and a subhalo with median c 200 would be nearly destroyed [43]. In the cluster environment, tidal stripping could also speed up the onset of gravothermal collapse [70][71][72][73][74]. Strong lensing observables.…”
mentioning
confidence: 99%