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Surface and Core Detonations in Rotating White Dwarfs
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| Zeitschriftentitel: | The Astrophysical Journal |
|---|---|
| Personen und Körperschaften: | , , |
| In: | The Astrophysical Journal, 862, 2018, 1, S. 27 |
| Format: | E-Article |
| Sprache: | Unbestimmt |
| veröffentlicht: |
American Astronomical Society
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| Schlagwörter: |
| author_facet |
García-Senz, D. Cabezón, R. M. Domínguez, I. García-Senz, D. Cabezón, R. M. Domínguez, I. |
|---|---|
| author |
García-Senz, D. Cabezón, R. M. Domínguez, I. |
| spellingShingle |
García-Senz, D. Cabezón, R. M. Domínguez, I. The Astrophysical Journal Surface and Core Detonations in Rotating White Dwarfs Space and Planetary Science Astronomy and Astrophysics |
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garcía-senz, d. |
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García-Senz, D. Cabezón, R. M. Domínguez, I. 0004-637X 1538-4357 American Astronomical Society Space and Planetary Science Astronomy and Astrophysics http://dx.doi.org/10.3847/1538-4357/aacb7d <jats:title>Abstract</jats:title> <jats:p>The feasibility of the double detonation mechanism—surface helium detonation followed by complete carbon detonation of the core—in a rotating white dwarf with mass ≃1 <jats:italic>M</jats:italic> <jats:sub>⊙</jats:sub> is studied using three-dimensional hydrodynamic simulations. A rapid rigid rotation of the white dwarf was assumed, so that its initial spherical geometry is considerably distorted. Unlike spherically symmetric models, we found that when helium ignition is located far from the spinning axis, the detonation fronts converge asynchronically at the antipodes of the ignition point. Nevertheless, the detonation of the carbon core still remains as the most probable outcome. The detonation of the core gives rise to a strong explosion, matching many of the basic observational constraints of Type Ia supernovae (SNe Ia). We conclude that the double detonation mechanism also works when the white dwarf is rapidly rotating. These results provide further evidence for the viability of sub-Chandrasekhar-mass models as well as some double degenerate models (those having some helium fuel at the merging moment), making them appealing channels for the production of SN Ia events.</jats:p> Surface and Core Detonations in Rotating White Dwarfs The Astrophysical Journal |
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American Astronomical Society, 2018 |
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| title |
Surface and Core Detonations in Rotating White Dwarfs |
| title_unstemmed |
Surface and Core Detonations in Rotating White Dwarfs |
| title_full |
Surface and Core Detonations in Rotating White Dwarfs |
| title_fullStr |
Surface and Core Detonations in Rotating White Dwarfs |
| title_full_unstemmed |
Surface and Core Detonations in Rotating White Dwarfs |
| title_short |
Surface and Core Detonations in Rotating White Dwarfs |
| title_sort |
surface and core detonations in rotating white dwarfs |
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Space and Planetary Science Astronomy and Astrophysics |
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http://dx.doi.org/10.3847/1538-4357/aacb7d |
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2018 |
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27 |
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<jats:title>Abstract</jats:title>
<jats:p>The feasibility of the double detonation mechanism—surface helium detonation followed by complete carbon detonation of the core—in a rotating white dwarf with mass ≃1 <jats:italic>M</jats:italic>
<jats:sub>⊙</jats:sub> is studied using three-dimensional hydrodynamic simulations. A rapid rigid rotation of the white dwarf was assumed, so that its initial spherical geometry is considerably distorted. Unlike spherically symmetric models, we found that when helium ignition is located far from the spinning axis, the detonation fronts converge asynchronically at the antipodes of the ignition point. Nevertheless, the detonation of the carbon core still remains as the most probable outcome. The detonation of the core gives rise to a strong explosion, matching many of the basic observational constraints of Type Ia supernovae (SNe Ia). We conclude that the double detonation mechanism also works when the white dwarf is rapidly rotating. These results provide further evidence for the viability of sub-Chandrasekhar-mass models as well as some double degenerate models (those having some helium fuel at the merging moment), making them appealing channels for the production of SN Ia events.</jats:p> |
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| author | García-Senz, D., Cabezón, R. M., Domínguez, I. |
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| description | <jats:title>Abstract</jats:title> <jats:p>The feasibility of the double detonation mechanism—surface helium detonation followed by complete carbon detonation of the core—in a rotating white dwarf with mass ≃1 <jats:italic>M</jats:italic> <jats:sub>⊙</jats:sub> is studied using three-dimensional hydrodynamic simulations. A rapid rigid rotation of the white dwarf was assumed, so that its initial spherical geometry is considerably distorted. Unlike spherically symmetric models, we found that when helium ignition is located far from the spinning axis, the detonation fronts converge asynchronically at the antipodes of the ignition point. Nevertheless, the detonation of the carbon core still remains as the most probable outcome. The detonation of the core gives rise to a strong explosion, matching many of the basic observational constraints of Type Ia supernovae (SNe Ia). We conclude that the double detonation mechanism also works when the white dwarf is rapidly rotating. These results provide further evidence for the viability of sub-Chandrasekhar-mass models as well as some double degenerate models (those having some helium fuel at the merging moment), making them appealing channels for the production of SN Ia events.</jats:p> |
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| spelling | García-Senz, D. Cabezón, R. M. Domínguez, I. 0004-637X 1538-4357 American Astronomical Society Space and Planetary Science Astronomy and Astrophysics http://dx.doi.org/10.3847/1538-4357/aacb7d <jats:title>Abstract</jats:title> <jats:p>The feasibility of the double detonation mechanism—surface helium detonation followed by complete carbon detonation of the core—in a rotating white dwarf with mass ≃1 <jats:italic>M</jats:italic> <jats:sub>⊙</jats:sub> is studied using three-dimensional hydrodynamic simulations. A rapid rigid rotation of the white dwarf was assumed, so that its initial spherical geometry is considerably distorted. Unlike spherically symmetric models, we found that when helium ignition is located far from the spinning axis, the detonation fronts converge asynchronically at the antipodes of the ignition point. Nevertheless, the detonation of the carbon core still remains as the most probable outcome. The detonation of the core gives rise to a strong explosion, matching many of the basic observational constraints of Type Ia supernovae (SNe Ia). We conclude that the double detonation mechanism also works when the white dwarf is rapidly rotating. These results provide further evidence for the viability of sub-Chandrasekhar-mass models as well as some double degenerate models (those having some helium fuel at the merging moment), making them appealing channels for the production of SN Ia events.</jats:p> Surface and Core Detonations in Rotating White Dwarfs The Astrophysical Journal |
| spellingShingle | García-Senz, D., Cabezón, R. M., Domínguez, I., The Astrophysical Journal, Surface and Core Detonations in Rotating White Dwarfs, Space and Planetary Science, Astronomy and Astrophysics |
| title | Surface and Core Detonations in Rotating White Dwarfs |
| title_full | Surface and Core Detonations in Rotating White Dwarfs |
| title_fullStr | Surface and Core Detonations in Rotating White Dwarfs |
| title_full_unstemmed | Surface and Core Detonations in Rotating White Dwarfs |
| title_short | Surface and Core Detonations in Rotating White Dwarfs |
| title_sort | surface and core detonations in rotating white dwarfs |
| title_unstemmed | Surface and Core Detonations in Rotating White Dwarfs |
| topic | Space and Planetary Science, Astronomy and Astrophysics |
| url | http://dx.doi.org/10.3847/1538-4357/aacb7d |