Non-spherical core-collapse supernovae: Evolution towards homologous expansion

Nonlinearity

Volumn 22, Issue 11, 2009, Pages 2775-2797

  Guzman, J ^a   Plewa, T ^a  

^a FLORIDA STATE UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 70350639162     PISSN: 09517715     EISSN: 13616544     Source Type: Journal    
DOI: 10.1088/0951-7715/22/11/010     Document Type: Article

References (37)

1. Blondin J M, Mezzacappa A and DeMarino C 2003 Stability of standing accretion shocks, with an eye toward core-collapse supernovae Astrophys. J. 584 971-80
2. Brouillettee M 2002 The Richtmyer-Meshkov instability Annu. Rev. Fluid Mech. 34 445-68
3. Bruenn S W 1993 Numerical simulations of core collapse supernovae Nuclear Physics in the Universe ed M W Guidry and M R Strayer (Bristol: Institute of Physics Publishing) pp 31-50
4. Calzavara A J and Matzner C D 2004 Supernova properties from shock breakout x-rays Mon. Not. R. Astron. Soc. 351 694-706
5. Chandrasekhar S 1961 Hydrodynamic and Hydromagnetic Stability (Oxford: Clarendon) chapter X
6. Chevalier R A, Blondin J M and Emmering R T 1992 Hydrodynamics instabilities in supernova remnants: self-similar driven waves Astrophys. J. 392 118-30
7. Chevalier R A and Klein R I 1978 On the Rayleigh-Taylor instability in stellar explosions Astrophys. J. 219 994-1007
8. Colella P and Woodward P R 1984 The piecewise parabolic method (PPM) for gas-dynamical simulations J. Comput. Phys. 54 174-201
9. Couch S M, Wheeler J C and Milosavljević M 2009 Aspherical core-collapse supernovae in red supergiants powered by nonrelativistic jets Astrophys. J. 696 953-70
10. Foglizzo T 2009 A simple toy model of the advective-acoustic instability: I. Perturbative approach Astrophys. J. 694 820-32
11. Fryxell B et al 2000 FLASH: an adaptive mesh hydrodynamics code for modeling astrophysical thermonuclear flashes Astrophys. J. Suppl. Ser. 131 273-334
12. Godunov S K 1959 A difference method for numerical calculation of discontinuous solutions of the equations of hydrodynamics Mat. Sb. 47 271-306
13. Herant M and Benz W 1991 Hydrodynamical instabilities and mixing in SN 1987A-two-dimensional simulations of the first 3 months Astrophys. J. 370 L81-4
14. Herant M and Woosley S E 1994 Postexplosion hydrodynamics of supernovae in red supergiants Astrophys. J. 425 814-28 (Pubitemid 24973225)
15. Hungerford A L, Fryer C L and Rockefeller G 2005 Gamma rays from single-lone supernova explosions Astrophys. J. 635 487-501
16. Hungerford A L, Fryer C L and Warren M S 2003 Gamma-ray lines from asymmetric supernovae Astrophys. J. 594 390-403
17. Joggerst C C, Woosley S E and Heger A 2009 Mixing in zero- and solar-metallicity supernovae Astrophys. J. 693 1780-802
18. Khokhlov A M 1995 Propagation of turbulent flames in supernovae Astrophys. J. 449 695-713
19. Kifonidis K, Plewa T, Janka H-Th and Müller E 2003 Non-spherical core collapse supernovae: I. Neutrino-driven convection, Rayleigh-Taylor instabilities, and the formation and propagation of metal clumps Astron. Astrophys. 408 621-49
20. Kifonidis K, Plewa T, Scheck L, Janka H-Th and Müller E 2006 Non-spherical core collapse supernovae: II. The late-time evolution of globally anisotropic neutrino-driven explosions and their implications for SN 1987A Astron. Astrophys. 453 661-78
21. Lamb H 1932 Hydrodynamics (New York: Dover)
22. Laming J M 2007 Analytic approach to the stability of standing accretion shocks: application to core-collapse supernovae Astrophys. J. 659 1449-57
23. Meshkov E E 1969 Instability of the interface of two gases accelerated by a shock wave Fluid Dyn. 4 151-7
24. Müller E and Arnett W D 1986 Carbon combustion supernovae: Numerical studies of the final evolution of degenerate carbon-oxygen cores Astrophys. J. 307 619-43
25. Nomoto K, Sugimoto D and Neo S 1976 Carbon deflagration supernova, an alternative to carbon detonation Astrophys. Space Sci. 39 L37-42
26. Richtmyer R D 1960 Taylor instability in shock acceleration of compressible fluids Commun. Pure Appl. Math. 13 297-319
27. Sadot O et al 2005 Observation of self-similar behavior of the 3D, nonlinear Rayleigh-Taylor instability Phys. Rev. Lett. 95 265001
28. Scheck L, Plewa T, Janka H-Th, Kifonidis K and Müller E 2004 Pulsar recoil by large-scale anisotropies in supernova explosions Phys. Rev. Lett. 92 011103
29. Sedov L I 1959 Similarity and Dimensional Methods in Mechanics (New York: Academic)
30. Sharp D 1984 An overview of Rayleigh-Taylor instability Physica D 12 3-18
31. Sohn S-I and Hwang W 2005 Numerical simulations of vortex sheet evolution in stratified shear flow J. Phys. Soc. Japan 74 1472-8
32. Steffen M 1990 A simple method for monotonic interpolation in one dimension Astron. Astrophys. 239 443-50
33. Strang G 1968 On the construction and comparison of difference schemes SIAM J. Numer. Anal. 5 506-17
34. Timmes F X and Swesty F D 2000 The accuracy, consistency, and speed of an electron-positron equation of state based on table interpolation of the Helmholtz free energy Astrophys. J. Suppl. Ser. 126 501-16
35. Woosley S E, Pinto P A and Ensman L 1988 Supernova 1987A-six weeks later Astrophys. J. 324 466-89
36. Youngs D L 1984 Numerical simulations of turbulent mixing by Rayleigh-Taylor instability Physica D 12 32-44
37. Youngs D L and Williams R J R 2008 Turbulent mixing in spherical implosions Int. J. Numer. Meth. Fluids 56 1597-603