Evidence map›Paper›PMID 36792638›Full record

ArticleScientific reports2023

Hydrodynamic Kelvin-Helmholtz instability on metallic surface.

Xi Wang, Xiao-Mian Hu, Sheng-Tao Wang, Hao Pan, Jian-Wei Yin

Abstract read
In one paragraph

Article in Scientific reports, 2023. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Not yet cited in PubMed.

0numbers the graph read from it
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0citing papers in PubMed
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1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

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3 · Its place in the literature

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0 citing papers in PubMed.

No citing paper in PubMed yet.

4 · The record

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PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

5 authors.

Xi WangInstitute of Applied Physics and Computational Mathematics, 100094, Beijing, People's Republic of China.
Xiao-Mian HuInstitute of Applied Physics and Computational Mathematics, 100094, Beijing, People's Republic of China.
Sheng-Tao WangInstitute of Applied Physics and Computational Mathematics, 100094, Beijing, People's Republic of China.
Hao PanInstitute of Applied Physics and Computational Mathematics, 100094, Beijing, People's Republic of China. pan_hao@iapcm.ac.cn.
Jian-Wei YinInstitute of Applied Physics and Computational Mathematics, 100094, Beijing, People's Republic of China. yin_jianwei@iapcm.ac.cn.

Funding

National Natural Science Foundation of China No. 11902039
6 · The paper itself

Abstract

Kelvin-Helmholtz instability on metallic surface is relevant to intense oblique impact in many physical processes such as explosive welding, Inertial Confinement Fusion and planetary impact events. Evolution of instability results in the formation of wavy morphology leading to material bonding or even mixing. However, mostly due to lack method to describe the dynamic behavior, instability mechanism controlled by elastoplastic properties of metal remains elusive. Here, we introduce a theory to reveal the evolution characteristics aroused by tangential velocity. Our simulations find that the unstable metallic surfaces exhibit amplitude growth and tangential motion by overcoming the depression of yield strength to generate wavy morphology. For diverse loading velocities, corrugated surfaces and material properties, an instability boundary distinguishes all unstable evolutions. Our analytical method with scale-independent variables reproducing numerical findings reveals plentiful characteristics of instability in strength materials. For designed loading velocities and material in oblique impact experiment in laboratory, the property of corrugated surfaces becomes an important factor to determine instability evolution.

Identifiers

PMID36792638
PMCPMC9931697

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Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.