Matches in SemOpenAlex for { <https://semopenalex.org/work/W4381301097> ?p ?o ?g. }
- W4381301097 endingPage "56" @default.
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- W4381301097 abstract "This chapter will go through the important nuclear reactions in stellar evolution and explosions, going through the individual stellar burning stages and also explosive burning conditions. To follow the changes in the composition of nuclear abundances requires the knowledge of the relevant nuclear reaction rates. For light nuclei (entering in early stellar burning stages), the resonance density is generally quite low, and the reactions are determined by individual resonances, which are best obtained from experiments. For intermediate mass and heavy nuclei, the level density is typically sufficient to apply statistical model approaches. For this reason, while we discuss all burning stages and explosive burning, focusing on the reactions of importance, we will for light nuclei refer to the chapters by M. Wiescher, deBoer and Reifarth (Experimental Nuclear Astrophysics) and P. Descouvement (Theoretical Studies of Low-Energy Nuclear Reactions), which display many examples, experimental methods utilized, and theoretical approaches how to predict nuclear reaction rates for light nuclei. For nuclei with sufficiently high level densities, we discuss statistical model methods used in present predictions of nuclear reaction cross sections and thermonuclear rates across the nuclear chart, including also the application to nuclei far from stability and fission modes." @default.
- W4381301097 created "2023-06-21" @default.
- W4381301097 creator A5063882464 @default.
- W4381301097 creator A5080769390 @default.
- W4381301097 date "2023-01-01" @default.
- W4381301097 modified "2023-09-23" @default.
- W4381301097 title "Nuclear Reactions in Evolving Stars (and Their Theoretical Prediction)" @default.
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