Titlebook: Nucleosynthesis and Its Implications on Nuclear and Particle Physics; Jean Audouze,Nicole Mathieu Book 1986 D. Reidel Publishing Company,

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Primordial Nucleosynthesis with Generic Particlesduction of .He and D + .He is calculated as a function of the mass, spin degrees of freedom, and spin statistics of the generic particle for masses in the range 10. ≲ m/m. ≲ 10.. The particular case of the Gelmini and Roncadelli majoron model for massive neutrinos is discussed.

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Dark Matter and Cosmological Nucleosynthesis least two ad hoc assumptions. Of these more complex but complete solutions, the ability to produce large scale free structures where these dark baryons lie may be the best way to resolve the different proposed solutions to the several different dark matter problems.

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Reaction Rates in the RP-Process and Nucleosynthesis in Novaeve hydrogen burning. These rates were applied in a systematic analysis for a variety of temperature conditions, appropriate to nova explosions, to study nucleosynthesis for isotopes of Ne Na Mg Al Si. The results are discussed in comparison with recent observations of elemental abundances in nova ejecta.

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Type I Supernovaeat epochs near maximum light. 2) Dynamical calculations have been done exploring the range of possible outcomes of the evolution of binary white dwarfs. 3) Consideration is given to the need to eject iron from the Galaxy to avoid overproduction by Type I events. 4) The nature of the class of peculiar Type I supernovae is explored.

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