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Nucleosynthesis in SNIa

  • Session 1 Stellar Structure and Evolution
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Abstract

The final products of a SNIa explosion critically depend on the degree of neutronization of the incinerated material and on the total amount of burned material. Here we study their dependence on the velocity of the burning front and on the density at which the thermonuclear runaway starts. The abundances of54Cr,54, 58Fe,58, 62Ni provide some constraints to the possible values of model parameters.

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Authors and Affiliations

  1. Departament de Física i Enginyería Nuclear, Universitat Politècnica de Catalunya, Barcelona, Spain

    E. Bravo

  2. Centre d'Estudis Avançats, C.S.I.C., Blanes, Spain

    J. Isern

  3. Departament de Física de l'Atmosfera, Astronomia i Astrofisica, Universitat de Barcelona, Spain

    R. Canal & J. Labay

  4. Grup d'Astrofisica, Institut d'Estudis Catalans, Barcelona, Spain

    E. Bravo, J. Isern, R. Canal & J. Labay

Authors
  1. E. Bravo
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  2. J. Isern
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  3. R. Canal
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  4. J. Labay
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Bravo, E., Isern, J., Canal, R. et al. Nucleosynthesis in SNIa. Astrophys Space Sci 169, 19–24 (1990). https://doi.org/10.1007/BF00640679

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  • DOI: https://doi.org/10.1007/BF00640679

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