Book contents
- Frontmatter
- Contents
- Part I Introduction
- Part II Supernovae: Observations Today
- Part III Theory of Thermonuclear Supernovae
- 10 Semi-Steady burning evolutionary sequences for CAL 83 and CAL 87: Super Soft X-ray binaries are supernova Ia progenitors
- 11 Type Ia progenitors: effects of spin-up of white dwarfs
- 12 Terrestrial combustion: feedback to the stars
- 13 Non-spherical delayed detonations
- 14 Numerical simulations of Type Ia supernovae: deflagrations and detonations
- 15 Type Ia supernovae: spectroscopic surprises
- 16 Aspherity effects in supernovae
- 17 Broad lightcurve SNe Ia: asymmetry or something else?
- 18 Synthetic spectrum methods for three-dimensional supernova models
- 19 A hole in Ia? Spectroscopic and polarimetric signatures of SN Ia asymmetry due to a companion star
- 20 Hunting for the signatures of 3-D explosions with 1-D synthetic spectra
- 21 On variations in the peak luminosities of Type Ia supernovae
- Part IV Theory of Core Collapse Supernovae
- Part V Magnetars, N-Stars, Pulsars
- Part VI Gamma-ray Bursts
- Part VII Conference Summary
- References
16 - Aspherity effects in supernovae
Published online by Cambridge University Press: 11 August 2009
- Frontmatter
- Contents
- Part I Introduction
- Part II Supernovae: Observations Today
- Part III Theory of Thermonuclear Supernovae
- 10 Semi-Steady burning evolutionary sequences for CAL 83 and CAL 87: Super Soft X-ray binaries are supernova Ia progenitors
- 11 Type Ia progenitors: effects of spin-up of white dwarfs
- 12 Terrestrial combustion: feedback to the stars
- 13 Non-spherical delayed detonations
- 14 Numerical simulations of Type Ia supernovae: deflagrations and detonations
- 15 Type Ia supernovae: spectroscopic surprises
- 16 Aspherity effects in supernovae
- 17 Broad lightcurve SNe Ia: asymmetry or something else?
- 18 Synthetic spectrum methods for three-dimensional supernova models
- 19 A hole in Ia? Spectroscopic and polarimetric signatures of SN Ia asymmetry due to a companion star
- 20 Hunting for the signatures of 3-D explosions with 1-D synthetic spectra
- 21 On variations in the peak luminosities of Type Ia supernovae
- Part IV Theory of Core Collapse Supernovae
- Part V Magnetars, N-Stars, Pulsars
- Part VI Gamma-ray Bursts
- Part VII Conference Summary
- References
Summary
Abstract
We present a brief summary of asphericity effects in thermonuclear and core collapse supernovae (SN), and how to distinguish the underlying physics by their observable signatures. Electron scattering is the dominant process to produce polarization which is one of the main diagnostical tools. Asphericities result in a directional dependence of the luminosity which has direct implications for the use of SNe in cosmology. For core collapse SNe, the current observations and their interpretations suggest that the explosion mechanism itself is highly aspherical with a well defined axis and, typically, axis ratios of 2 to 3. Asymmetric density/chemical distributions and off-center energy depositions have been identified as crucial for the interpretation of the polarization P. For thermonuclear SNe, polarization turned out to be an order of magnitude smaller strongly supporting rather spherical, radially stratified envelopes. Nevertheless, asymmetries have been recognized as important signatures to probe A) for the signatures of the progenitor system, B) the global asymmetry with well defined axis, likely to be caused by rotation of an accreting white dwarf or merging WDs, and C) possible remains of the deflagration pattern.
Introduction
During the last decade, advances in observational, theoretical and computational astronomy have provided new insights into the nature and physics of SNe and gamma-ray bursts. Due to the extreme brightness of these events, they are expected to continue to play important role in cosmology. SNe Ia allowed good measurements of the Hubble constant both by statistical methods and theoretical models.
- Type
- Chapter
- Information
- Cosmic Explosions in Three DimensionsAsymmetries in Supernovae and Gamma-Ray Bursts, pp. 142 - 150Publisher: Cambridge University PressPrint publication year: 2004