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Title: Non-Richtmyer–Meshkov instability ejecta production based on shallow bubble collapse

Abstract

The study of shock-driven ejecta production has focused on Richtmyer–Meshkov instability (RMI) growth from geometric features of the material surface. Extensive study of this mechanism under both single- and multiple-shock conditions has found that the ejected mass tends to be closely associated with the shocked surface phase, and its temperature is not dramatically greater than the hydrodynamic shock temperature of the bulk. In this work, we propose and demonstrate a new ejecta production mechanism that can occur under multiple-shock conditions based on the collapse of bubbles near the free surface of the material. This mechanism produces ejected mass that is much greater in quantity than observed in the RMI case. The particles are much hotter than predicted by the shock Hugoniot state, and the ejected mass does not appear to be strongly dependent upon initial surface finish. The ejecta source extends into the material with no clear remaining free surface. We name this mechanism Shallow Bubble Collapse (SBC) and discuss the conditions under which it activates. We demonstrate resolved modeling methods that enable the calculation, design, and study of SBC as a mechanism and perform a series of experiments to compare with the models. Under some multiple-shock conditions, SBC ejectionmore » produces ten times more ejected mass than RMI growth.« less

Authors:
ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [2]; ORCiD logo [2]; ORCiD logo [2]; ORCiD logo [1]; ORCiD logo [3]
+ Show Author Affiliations
  1. Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
  2. Nevada National Security Site (NNSS), Santa Barbara, CA (United States)
  3. Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Publication Date:
Research Org.:
Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States); Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Org.:
USDOE National Nuclear Security Administration (NNSA); USDOE Office of Science (SC)
OSTI Identifier:
1962478
Alternate Identifier(s):
OSTI ID: 1908834
Report Number(s):
LLNL-JRNL-841345
Journal ID: ISSN 0021-8979; 1062273; TRN: US2313079
Grant/Contract Number:  
AC52-07NA27344; NA0003624; 89233218CNA000001
Resource Type:
Accepted Manuscript
Journal Name:
Journal of Applied Physics
Additional Journal Information:
Journal Volume: 133; Journal Issue: 2; Journal ID: ISSN 0021-8979
Publisher:
American Institute of Physics (AIP)
Country of Publication:
United States
Language:
English
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; ballistic transport; thermal instruments; shock dynamics; temperature metrology; flow instabilities; shock wave; cavitation bubbles; spectrograms; heterodyne laser interferometry; surface states

Citation Formats

Maskaly, G. R., Stevens, G. D., La Lone, B. M., Turley, W. D., Staska, M. D., Najjar, F. M., and Hartsfield, T. M. Non-Richtmyer–Meshkov instability ejecta production based on shallow bubble collapse. United States: N. p., 2023. Web. doi:10.1063/5.0132256.
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Maskaly, G. R., Stevens, G. D., La Lone, B. M., Turley, W. D., Staska, M. D., Najjar, F. M., & Hartsfield, T. M. Non-Richtmyer–Meshkov instability ejecta production based on shallow bubble collapse. United States. https://doi.org/10.1063/5.0132256
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Maskaly, G. R., Stevens, G. D., La Lone, B. M., Turley, W. D., Staska, M. D., Najjar, F. M., and Hartsfield, T. M. Thu . "Non-Richtmyer–Meshkov instability ejecta production based on shallow bubble collapse". United States. https://doi.org/10.1063/5.0132256. https://www.osti.gov/servlets/purl/1962478.
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@article{osti_1962478,
title = {Non-Richtmyer–Meshkov instability ejecta production based on shallow bubble collapse},
author = {Maskaly, G. R. and Stevens, G. D. and La Lone, B. M. and Turley, W. D. and Staska, M. D. and Najjar, F. M. and Hartsfield, T. M.},
abstractNote = {The study of shock-driven ejecta production has focused on Richtmyer–Meshkov instability (RMI) growth from geometric features of the material surface. Extensive study of this mechanism under both single- and multiple-shock conditions has found that the ejected mass tends to be closely associated with the shocked surface phase, and its temperature is not dramatically greater than the hydrodynamic shock temperature of the bulk. In this work, we propose and demonstrate a new ejecta production mechanism that can occur under multiple-shock conditions based on the collapse of bubbles near the free surface of the material. This mechanism produces ejected mass that is much greater in quantity than observed in the RMI case. The particles are much hotter than predicted by the shock Hugoniot state, and the ejected mass does not appear to be strongly dependent upon initial surface finish. The ejecta source extends into the material with no clear remaining free surface. We name this mechanism Shallow Bubble Collapse (SBC) and discuss the conditions under which it activates. We demonstrate resolved modeling methods that enable the calculation, design, and study of SBC as a mechanism and perform a series of experiments to compare with the models. Under some multiple-shock conditions, SBC ejection produces ten times more ejected mass than RMI growth.},
doi = {10.1063/5.0132256},
journal = {Journal of Applied Physics},
number = 2,
volume = 133,
place = {United States},
year = {Thu Jan 12 00:00:00 EST 2023},
month = {Thu Jan 12 00:00:00 EST 2023}
}
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