Scaling supernova hydrodynamics to the laboratory
dc.contributor.author | Kane, J. O. | en_US |
dc.contributor.author | Arnett, David | en_US |
dc.contributor.author | Remington, Bruce A. | en_US |
dc.contributor.author | Glendinning, S. Gail | en_US |
dc.contributor.author | Bazan, G. | en_US |
dc.contributor.author | Drake, R. Paul | en_US |
dc.contributor.author | Fryxell, B. A. | en_US |
dc.contributor.author | Teyssier, R. | en_US |
dc.contributor.author | Moore, K. | en_US |
dc.date.accessioned | 2010-05-06T20:57:44Z | |
dc.date.available | 2010-05-06T20:57:44Z | |
dc.date.issued | 1999-05 | en_US |
dc.identifier.citation | Kane, J.; Arnett, D.; Remington, B. A.; Glendinning, S. G.; Bazan, G.; Drake, R. P.; Fryxell, B. A.; Teyssier, R.; Moore, K. (1999). "Scaling supernova hydrodynamics to the laboratory." Physics of Plasmas 6(5): 2065-2071. <http://hdl.handle.net/2027.42/69672> | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/69672 | |
dc.description.abstract | Supernova (SN) 1987A focused attention on the critical role of hydrodynamic instabilities in the evolution of supernovae. To test the modeling of these instabilities, we are developing laboratory experiments of hydrodynamic mixing under conditions relevant to supernovae. Initial results were reported in J. Kane et al. [Astrophys. J. 478, L75 (1997) and B. A. Remington et al., Phys. Plasmas 4, 1994 (1997)]. The Nova laser is used to generate a 10–15 Mbar shock at the interface of a two-layer planar target, which triggers perturbation growth due to the Richtmyer–Meshkov instability, and to the Rayleigh–Taylor 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 ×103 s.×103s. The scaling of hydrodynamics on microscopic laser scales to the SN-size scales is presented. The experiment is modeled using the hydrodynamics codes HYADES [J. T. Larson and S. M. Lane, J. Quant. Spect. Rad. Trans. 51, 179 (1994)] and CALE [R. T. Barton, Numerical Astrophysics (Jones and Bartlett, Boston, 1985), pp. 482–497], and the supernova code PROMETHEUS [P. R. Woodward and P. Collela, J. Comp. Phys. 54, 115 (1984)]. Results of the experiments and simulations are presented. Analysis of the spike-and-bubble velocities using potential flow theory and Ott thin-shell theory is presented, as well as a study of 2D versus 3D differences in perturbation growth at the He-H interface of SN 1987A. | en_US |
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dc.format.extent | 346209 bytes | |
dc.format.mimetype | text/plain | |
dc.format.mimetype | application/pdf | |
dc.publisher | The American Institute of Physics | en_US |
dc.rights | © The American Institute of Physics | en_US |
dc.title | Scaling supernova hydrodynamics to the laboratory | en_US |
dc.type | Article | en_US |
dc.subject.hlbsecondlevel | Physics | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | University of Michigan, Ann Arbor, Michigan 48109-2143 | en_US |
dc.contributor.affiliationother | University of Arizona, Tucson, Arizona 85721 | en_US |
dc.contributor.affiliationother | Lawrence Livermore National Laboratory, Livermore, California 94550 | en_US |
dc.contributor.affiliationother | ASCI Flash Center, University of Chicago, Chicago, Illinois 60637 | en_US |
dc.contributor.affiliationother | CEA/DSM/DAPNIA/Service d’Astrophysique, Bat. 709 Centre d’Etudes de Saclay L’Orme des Merisiers F-91191 Gif-sur-Yvette Cedex, France | en_US |
dc.contributor.affiliationother | Harvey Mudd College, Claremont, California 91711 | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/69672/2/PHPAEN-6-5-2065-1.pdf | |
dc.identifier.doi | 10.1063/1.873497 | en_US |
dc.identifier.source | Physics of Plasmas | en_US |
dc.identifier.citedreference | R. D. Richtmyer, Commun. Pure Appl. Math. CPAMAT13, 297 (1960). | en_US |
dc.identifier.citedreference | E. E. Meshkov, Izv. Akad. Nauk SSSR, Mekh. Zhidk. Gaza IMZGAB4, 151 (1969); Izv., Acad. Sci., USSR Fluid Dyn. ZZZZZZ4, 101 (1969). | en_US |
dc.identifier.citedreference | Lord Rayleigh, Scientific Papers II, Cambridge, England, 1900. | en_US |
dc.identifier.citedreference | G. Taylor, Proc. R. Soc. London, Ser. A PRLAAZ201, 192 (1950). | en_US |
dc.identifier.citedreference | D. Arnett, J. N. Bahcall, R. A. Kirshner, and S. E. Woosley, Annu. Rev. Astron. Astrophys. ARAAAJ27, 629 (1989). | en_US |
dc.identifier.citedreference | T. Shigeyama and K. Nomoto, Astrophys. J. ASJOAB360, 242 (1990). | en_US |
dc.identifier.citedreference | R. W. Hanuschik and J. Dachs, Astron. Astrophys. AAEJAF192, L29 (1987). | en_US |
dc.identifier.citedreference | V. M. Blanco et al., Astrophys. J. ASJOAB320, 589 (1987). | en_US |
dc.identifier.citedreference | F. C. Witteborn, J. D. Bregman, D. H. Wooden, P. A. Pinto, D. M. Rank, S. E. Woosley, and M. Cohen, Astrophys. J. ASJOAB338, L9 (1989). | en_US |
dc.identifier.citedreference | J. Tueller, S. Barthelmy, N. Gehrels, B. J. Teegarden, M. Leventhal, and C. J. MacCallum, Astrophys. J. ASJOAB351, L41 (1990). | en_US |
dc.identifier.citedreference | R. McCray, Annu. Rev. Astron. Astrophys. ARAAAJ31, 175 (1993). | en_US |
dc.identifier.citedreference | J. Kane, D. Arnett, B. A. Remington, S. G. Glendinning, J. Castor, R. Wallace, A. Rubenchik, and B. A. Fryxell, Astrophys. J. ASJOAB478, L75 (1997). | en_US |
dc.identifier.citedreference | B. A. Remington et al., Phys. Plasmas PHPAEN4, 1994 (1997). | en_US |
dc.identifier.citedreference | R. P. Drake et al., Phys. Rev. Lett. PRLTAO81, 2068 (1998). | en_US |
dc.identifier.citedreference | R. P. Drake, J. P. Carroll, K. Estabrook, S. G. Glendinning, B. A. Remington, R. Wallace, and R. McCray, Astrophys. J., ASJOAB500, L157 (1998). | en_US |
dc.identifier.citedreference | J. T. Larsen and S. M. Lane, J. Quant. Spectrosc. Radiat. Transf. JQSRAE51, 179 (1994). | en_US |
dc.identifier.citedreference | R. T. Barton, in Numerical Astrophysics, edited by J. M. Centrella, J. M. LeBlanc, and R. L. Bowers (Jones and Bartlett, Boston, 1985), pp. 482–497. | en_US |
dc.identifier.citedreference | P. R. Woodward and P. Colella, J. Comput. Phys. JCTPAH54, 115 (1984). | en_US |
dc.identifier.citedreference | D. Arnett, Supernovae and Nucleosynthesis (Princeton University Press, Princeton, 1996). | en_US |
dc.identifier.citedreference | D. Arnett, B. A. Fryxell, and E. Müller, Astrophys. J. ASJOAB341, L63 (1989). | en_US |
dc.identifier.citedreference | B. A. Fryxell, E. Müller, and D. Arnett, Astrophys. J. ASJOAB367, 619 (1991). | en_US |
dc.identifier.citedreference | E. Müller, B. A. Fryxell, and D. Arnett, Astron. Astrophys. AAEJAF251, 505 (1991). | en_US |
dc.identifier.citedreference | S. G. Glendinning, Rev. Sci. Instrum. RSINAK63, 5108 (1992). | en_US |
dc.identifier.citedreference | G. M. Dimonte, C. E. Frerking, M. Schneider, and B. A. Remington, Phys. Plasmas PHPAEN3, 614 (1996). | en_US |
dc.identifier.citedreference | K. S. Budil, B. A. Remington, T. A. Peyser, K. O. Mikaelian, P. L. Miller, N. C. Woolsey, W. M. Wood-Vasey, and A. M. Rubenchik, Phys. Rev. Lett. PRLTAO76, 4536 (1996). | en_US |
dc.identifier.citedreference | T. A. Peyser, P. L. Miller, P. E. Stry, K. S. Budil, E. W. Burke, D. A. Wojtowicz, D. L. Griswold, B. A. Hammel, and D. W. Phillion, Phys. Rev. Lett. PRLTAO75, 2332 (1995). | en_US |
dc.identifier.citedreference | U. Alon, J. Hecht, D. Mukamel, and D. Shvarts, Phys. Rev. Lett. PRLTAO72, 2867 (1994). | en_US |
dc.identifier.citedreference | U. Alon, J. Hecht, D. Ofer, and D. Shvarts, Phys. Rev. Lett. PRLTAO74, 534 (1995). | en_US |
dc.identifier.citedreference | J. Hecht, U. Alon, and D. Shvarts, Phys. Fluids PHFLE66, 4019 (1994). | en_US |
dc.identifier.citedreference | E. Ott, Phys. Rev. Lett. PRLTAO29, 1429 (1995). | en_US |
dc.identifier.citedreference | M. M. Basko, Phys. Plasmas PHPAEN1, 1270 (1994). | en_US |
dc.identifier.citedreference | K. A. Mayer and P. J. Blewett, Phys. Fluids PFLDAS15, 753 (1972). | en_US |
dc.identifier.citedreference | D. Ryutov, R. P. Drake, J. Kane, E. Liang, B. A. Remington, and W. M. Wood-Vasey, “Similarity criteria for the laboratory simulation of supernova hydrodynamics,” Astrophys. J., June 1999 (in press). | en_US |
dc.identifier.citedreference | E. M. Campbell et al., Laser Part. Beams LPBEDA15, 607 (1997). | en_US |
dc.identifier.citedreference | L. Landau and E. Lifshitz, Fluid Dynamics (Pergammon, Princeton, 1960). | en_US |
dc.identifier.citedreference | J. P. Dahlburg, J. H. Gardner, G. D. Doolen, and S. W. Haan, Phys. Fluids B PFBPEI5, 571 (1993). | en_US |
dc.identifier.citedreference | M. M. Marinak et al., Phys. Rev. Lett. PRLTAO75, 3677 (1995). | en_US |
dc.owningcollname | Physics, Department of |
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