Summary
The present status of our understanding of core-collapse and of thermonuclear supernovae is reviewed. It will be argued that the failure of numerical simulations of the collapse of massive stars to produce explosions is probably caused by our incomplete knowledge of the (micro-) physics involved. In contrast, for thermonuclear (type Ia) supernovae the basic physics seems to be well under control and, therefore, it is not surprising that model predictions and observations are in good agreement.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
P. Clavin: Ann. Rev. Fluid Mech. 26, 321 (1994)
R. Buras et al.: Phys. Rev. Lett. 90, 1101 (2003)
H. Dimmelmeier, J.A. Font, E. Müller: Astron. Astrophys. 388, 917 (2003)
H. Dimmelmeier, J.A. Font, E. Müller: Astron. Astrophys. 393, 523 (2003)
B.A. Fryxell, E. Müller, W.D. Arnett: MPA Preprint 449 (1989)
D. Garcia-Senz, S.E. Woosley: Astrophys. J. 454, 895 (1995)
W. Hillebrandt, J.C. Niemeyer: Ann. Rev. Astron. Astrophys. 38, 191 (2000)
H.-Th. Janka et al.: Core Collapse and Then? The Route to Massive Star Explosions. In: From Twilight to Highlight: The Physics of Supernovae, ed by W. Hillebrandt, B. Leibundgut (Springer, Berlin Heidelberg New York 2003) p. 39
M.Th. Keil, G.G. Raffelt, H.-Th. Janka: Astrophys. J. 590, 971 (2003)
K. Kifonidis et al.: Astron. Astrophys. 408, 621 (2003)
K. Langanke, G. Martinez-Pinedo: Rev. Mod. Phys. 75, 819 (2003)
K. Langanke et al.: Phys. Rev. Lett. 90, 1102 (2003)
M. Liebendörfer et al.: Nuc. Phys. A719, 144 (2003)
J.C. Niemeyer, W. Hillebrandt: Astrophys. J. 452, 769 (1995)
J.C. Niemeyer, S.E. Woosley: Astrophys. J. 475, 740 (1997)
M. Rampp, H.-Th. Janka: Astron. Astrophys. 396, 361 (2002)
M. Reinecke, W. Hillebrandt, J.C. Niemeyer: Astron. Astrophys. 347, 739 (1999)
M. Reinecke, W. Hillebrandt, J.C. Niemeyer: Astron. Astrophys. 386, 936 (2002)
M. Reinecke, W. Hillebrandt, J.C. Niemeyer: Astron. Astrophys. 391, 1167 (2002)
E. Sorokina, S. Blinnikov: Light Curves of Type Ia Supernovae as a Probe for an Explosion Model. In: From Twilight to Highlight: The Physics of Supernovae, ed by W. Hillebrandt, B. Leibundgut (Springer, Berlin Heidelberg New York 2003) p. 268
K. Sumiyoshi, H. Toki: Astrophys. J. 422, 700 1994
F.D. Swesty, J.M. Lattimer, E.S. Myra: Astrophys. J. 425, 195 (1994)
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2005 Springer-Verlag Berlin Heidelberg
About this paper
Cite this paper
Hillebrandt, W. (2005). Models of Supernova Explosions: Where Do We Stand?. In: Marcaide, JM., Weiler, K.W. (eds) Cosmic Explosions. Springer Proceedings in Physics, vol 99. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-26633-X_33
Download citation
DOI: https://doi.org/10.1007/3-540-26633-X_33
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-23039-7
Online ISBN: 978-3-540-26633-4
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)