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  • af J. Audouze & S. Vauclair
    880,95 kr.

  • af J. Audouze
    1.029,95 kr.

    I - PRIMORDIAL NUCLEOSYNTHESIS 1 --. -~-~----,---,-. --------- H. Reeves Primordial nucleosynthesis in 1985 3 The puzzle of lithium in evolved stars H. Reeves 13 High energy particles in dark molecular H. Reeves clouds 23 P. Delbourgo-Salvador, G. Malinie, J. Audouze Standard big bang nucleosynthesis and 3 chemical evolution of D and He 27 G. steigman, D. S. P. Dearborn, D. N. Schramm The survival of Helium,3 in stars 37 G. steigroan How degenerate can we be ? 45 J. Audouze, D. Lindley, J. Silk 3 Early-photoproduction of D and He and pregalactic nucleosynthesis of the light elements 57 R. Schaeffer, P. Delbourgo-Salvador, J. Audouze Influence of quark nuggets on primordial nucleosynthesis 65 T. P. Walker, E. W. Kolb, M. S. Turner Primordi. al nucleosynthesis with generic part. icles 71 D. N. Schramm Dark matter and cosmological nucleosynthesis 79 B. J. Carr Nucleosynthetic consequences of population [II stars W. Glatzel 87 vi CONTENTS 95 I I -EXPWSIVE OBJECTS J. W. Truran Nucleosynthesis accompanying classical nova outbursts 97 M. Wiescher, J. GOrres, P. -K. Thielemann, H. Ritter Reaction rates in the RP-process and nucleosynthesis in novae 105 Type I supernovae ll3 J. C. Wheeler R. canal, J. lsern, J. Labay, R. Lbpez Nucleosynthesis and type I supernovae 121 P. -K. Thielemann, K. Nomoto, K. Yokoi EXplosive nucleosynthesis in carbon deflagration models of type I supernovae 131 E. Mi. iller, Y. Eriquchi Differentially rotating equilibrium models and the collapse of rotating degenerate configurations 143 S. E. WOOsley, T. A.

  • af J. Audouze
    1.014,95 kr.

    This book is the third volume belonging to the series of proceedings of the Moriond Astrophysics meetings. I t follows "Cosmology and particles" publi shed in 1981 by les Editions Frontieres and "The birth of the Universe" whioh appeared in 1982 thanks to the same publisher. This workshop took plaoe on llBroh 1983 at La Plagne and as in 1981 and 1982 took advantage of the simultaneous presence of the particle physicists and the astrophysicists. As said in the title of the book the partioipa nts have presented their most recent views on the evolution of large structures and galaxies and the relevance of these questions on particle physics and cosmology. Among the llBny developments which are at the origin of the thirty five papers gathered here, three main themes have been touched on by several speakers during the workshop. They are (i) the influence of the mass of neutrinos and other "inos" predicted by the "Supersymmetry" theories, which are the more likely candidates for the hidden mass of the Universe, (ii) the dynamics of triaxial galaxies and (iii) the possible occurence of pregalactic stars with a debate on their hypothetioal nucleosynthetic role. Miny different views h3. ve been presented on these three topics (and many others) which prove the liveness of the physical cosmology. For the editor it has been quite difficult to find a reasonable and logical order to arrange the oontent of the book.

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