Nucleosynthesis and mixing: Unexamined assumptions

Details Nucleosynthesis and mixing: Unexamined assumptions Nucleosynthesis and mixing: Unexamined assumptions

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..402..307a&link_type=abstract

Astrophysical implications of the laboratory study of presolar materials. AIP Conference Proceedings, Volume 402, pp. 307-315 (

Astronomy and Astrophysics

Astrophysics

3

Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Interstellar Dust Grains, Diffuse Emission, Infrared Cirrus

Scientific paper

The investigation of rapidly evolving late stages of the lives of stars-by use of direct multidimensional hydrodynamic simulations-brings into question assumptions generally used in the theory of stellar evolution. A mathematical and a physical analysis of the origin of these differences is presented. Quantitative predictions of nucleosynthesis yields and presupernova characteristics will require attention to these new physical effects. Implications for interpreting the X grains are discussed as an example.

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