- Abstract:
-
We introduce two simplified nuclear networks that can be used in hydrostatic carbon burning reactions occurring in white dwarf interiors. They model the relevant nuclear reactions in carbon-oxygen white dwarfs (COWDs) approaching ignition in Type Ia supernova (SN Ia) progenitors, including the effects of the main e-captures and \beta-decays that drive the convective Urca process. They are based on studies of a detailed nuclear network compiled by the authors and are defined by approximate set...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1088/0067-0049/190/2/334
-
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- Journal:
- ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
- Volume:
- 190
- Issue:
- 2
- Pages:
- 334-347
- Publication date:
- 2010-09-08
- DOI:
- EISSN:
-
1538-4365
- ISSN:
-
0067-0049
- URN:
-
uuid:517dea09-1186-449f-8107-18e521ccca04
- Source identifiers:
-
103694
- Local pid:
- pubs:103694
- Keywords:
- Copyright date:
- 2010
- Notes:
-
52 pages, 16 figures, accepted for publication in the Astrophysical
Journal
Journal article
Simplified Hydrostatic Carbon Burning in White Dwarf Interiors
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