Supernova-relevant hydrodynamic instability experiments on the Nova laser
Abstract
Observations of Supernova 1987A suggest that hydrodynamic instabilities play a critical role in the evolution of supernovae. To test the modeling of these instabilities, and to study instability issues which are difficult to model, we are developing laboratory experiments of hydrodynamic mixing under conditions relevant to supernovae. We use the Nova laser to generate a 10{endash}15 Mbar shock at the interface between an 85 {mu}m thick layer of Cu and a 500 {mu}m layer of CH{sub 2}; our first target is planar. We impose a single mode sinusoidal material perturbation at the interface with {lambda}=200{mu}m, {eta}{sub 0}=20{mu}m, causing perturbation growth by the RM instability as the shock accelerates the interface, and by RT instability as the interface decelerates. This resembles the hydrodynamics of the He-H interface of a Type II supernova at intermediate times, up to a few {times}10{sup 3}s. We use the supernova code PROMETHEUS and the hydrodynamics codes HYADES and CALE to model the experiment. We are designing further experiments to compare results for 2D vs. 3D single mode perturbations; high resolution 3D modeling requires prohibitive time and computing resources, but we can perform and study 3D experiments as easily as 2D experiments. Low resolution simulations suggest thatmore »
- Authors:
-
- University of Arizona, Tucson, Arizona85721 (United States)
- Publication Date:
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 678784
- Report Number(s):
- CONF-970407-
Journal ID: APCPCS; ISSN 0094-243X; TRN: 99:009233
- Resource Type:
- Journal Article
- Journal Name:
- AIP Conference Proceedings
- Additional Journal Information:
- Journal Volume: 406; Journal Issue: 1; Conference: 13. international conference on laser interaction and related plasma phenomena, Monterey, CA (United States), 13-18 Apr 1997; Other Information: PBD: Apr 1997
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 70 PLASMA PHYSICS AND FUSION; NOVA FACILITY; PLASMA INSTABILITY; LASER-PRODUCED PLASMA; HYDRODYNAMICS; SUPERNOVAE; RAYLEIGH-TAYLOR INSTABILITY
Citation Formats
Kane, J, Arnett, D, Remington, B A, Glendinning, S G, Wallace, R, Managan, R, and Rubenchik, A. Supernova-relevant hydrodynamic instability experiments on the Nova laser. United States: N. p., 1997.
Web. doi:10.1063/1.53577.
Kane, J, Arnett, D, Remington, B A, Glendinning, S G, Wallace, R, Managan, R, & Rubenchik, A. Supernova-relevant hydrodynamic instability experiments on the Nova laser. United States. https://doi.org/10.1063/1.53577
Kane, J, Arnett, D, Remington, B A, Glendinning, S G, Wallace, R, Managan, R, and Rubenchik, A. 1997.
"Supernova-relevant hydrodynamic instability experiments on the Nova laser". United States. https://doi.org/10.1063/1.53577.
@article{osti_678784,
title = {Supernova-relevant hydrodynamic instability experiments on the Nova laser},
author = {Kane, J and Arnett, D and Remington, B A and Glendinning, S G and Wallace, R and Managan, R and Rubenchik, A.},
abstractNote = {Observations of Supernova 1987A suggest that hydrodynamic instabilities play a critical role in the evolution of supernovae. To test the modeling of these instabilities, and to study instability issues which are difficult to model, we are developing laboratory experiments of hydrodynamic mixing under conditions relevant to supernovae. We use the Nova laser to generate a 10{endash}15 Mbar shock at the interface between an 85 {mu}m thick layer of Cu and a 500 {mu}m layer of CH{sub 2}; our first target is planar. We impose a single mode sinusoidal material perturbation at the interface with {lambda}=200{mu}m, {eta}{sub 0}=20{mu}m, causing perturbation growth by the RM instability as the shock accelerates the interface, and by RT instability as the interface decelerates. This resembles the hydrodynamics of the He-H interface of a Type II supernova at intermediate times, up to a few {times}10{sup 3}s. We use the supernova code PROMETHEUS and the hydrodynamics codes HYADES and CALE to model the experiment. We are designing further experiments to compare results for 2D vs. 3D single mode perturbations; high resolution 3D modeling requires prohibitive time and computing resources, but we can perform and study 3D experiments as easily as 2D experiments. Low resolution simulations suggest that the perturbations grow 50{percent} faster in 3D than in 2D; such a difference may help explain the high observed velocities of radioactive core material in SN1987A. We present the results of the experiments and simulations. {copyright} {ital 1997 American Institute of Physics.}},
doi = {10.1063/1.53577},
url = {https://www.osti.gov/biblio/678784},
journal = {AIP Conference Proceedings},
number = 1,
volume = 406,
place = {United States},
year = {Tue Apr 01 00:00:00 EST 1997},
month = {Tue Apr 01 00:00:00 EST 1997}
}