CRACK
发表于 2025-3-28 17:17:26
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表示向前
发表于 2025-3-28 19:59:42
,Spezielle Dynamik der Atmosphäre, for fastest particles leading to unexpected non-extensive scaling exponents ; whereas in presence of gravity, the cluster bounces as a single inelastic body. All these results differ significantly from classical inelastic hard sphere kinetic theory and previous simulations, both based on a constant restitution coefficient.
稀释前
发表于 2025-3-29 02:39:40
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Emg827
发表于 2025-3-29 06:36:02
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农学
发表于 2025-3-29 09:01:56
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mitten
发表于 2025-3-29 15:18:00
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sleep-spindles
发表于 2025-3-29 15:46:22
Driven Granular Gases,if a driving inversely proportional to the velocity is used (. < 0). In the case of rotational driving, the system is well randomized and clusters are hindered. Even though rotational driving may be difficult to realize experimentally, this is an opportunity to avoid or delay the often unwanted effect of clustering.
绊住
发表于 2025-3-29 21:03:21
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white-matter
发表于 2025-3-30 01:10:26
Claudia von Aufschnaiter Prof. Dr.ibution function. We also discuss the possibility of a catastrophe whereby the number of particles diverges in a finite time. This phenomenon appears correlated to a “shattering” transition marked by a delta singularity at vanishingly small grains for the rescaled size distribution.
regale
发表于 2025-3-30 05:54:52
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