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Titlebook: Nuclear Astrophysics; Proceedings of a Wor Wolfgang Hillebrandt,Rudolf Kuhfu?,James W. Truran Conference proceedings 1987 Springer-Verlag B

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書目名稱Nuclear Astrophysics
副標(biāo)題Proceedings of a Wor
編輯Wolfgang Hillebrandt,Rudolf Kuhfu?,James W. Truran
視頻videohttp://file.papertrans.cn/669/668505/668505.mp4
叢書名稱Lecture Notes in Physics
圖書封面Titlebook: Nuclear Astrophysics; Proceedings of a Wor Wolfgang Hillebrandt,Rudolf Kuhfu?,James W. Truran Conference proceedings 1987 Springer-Verlag B
描述The recent discovery of a type II supernova in the Large Magellanic Cloud provides a rare chance to compare models of stellar evolution and nucleosynthesis directly with observations. This workshop covers thermonuclear reaction rates in chaos (experimental and theoretical), stellar evolution, nucleosynthesis and isotopic anomalies in meteorites and, in a final section, the supernovae, in particular SN 1987A. It brings the most interesting news in the rapidly developing field of nuclear astrophysics to researchers and also to graduate students. Recent and future developments are discussed. Special emphasis is placed on experimental and theoretical approaches to obtaining nuclear reaction rates, models of stellar evolution and explosions, and theories of nucleosynthesis. Various aspects of stellar evolution, nucleosynthesis, and thermonuclear reactions of astrophysical interest are reviewed. Several contributions deal with supernova explosions of massive stars, and in particular with Supernova 1987A and its impact on current models of the evolution of massive stars, the gravitational collapse of stellar cores, and neutrino physics and astronomy.
出版日期Conference proceedings 1987
關(guān)鍵詞Anomalie; Supernova; astronomy; astrophysics; gravitation; gravity; nuclear reaction; stellar evolution
版次1
doihttps://doi.org/10.1007/BFb0016562
isbn_softcover978-3-662-13627-0
isbn_ebook978-3-540-47869-0Series ISSN 0075-8450 Series E-ISSN 1616-6361
issn_series 0075-8450
copyrightSpringer-Verlag Berlin Heidelberg 1987
The information of publication is updating

書目名稱Nuclear Astrophysics影響因子(影響力)




書目名稱Nuclear Astrophysics影響因子(影響力)學(xué)科排名




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書目名稱Nuclear Astrophysics網(wǎng)絡(luò)公開度學(xué)科排名




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書目名稱Nuclear Astrophysics被引頻次學(xué)科排名




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沙發(fā)
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地板
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Chemodynamical models of galactic evolution,ses in the ISM and the interaction between stars and the ISM in more detail..As a first step towards a consistent galactic evolution model we consider in this study the temporal evolution of an isolated galactic region applying an advanced model of the ISM based on the three-component picture of McKee and Ostriker.
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Thermonuclear reactions at high temperatures and densities,odisintegration reactions and reactions involving charged particles in both the incoming and outgoing channels. These results provide a unified and consistent procedure for the determination of thermonuclear reaction rates as a function of both temperature and density.
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The ETFSI approach to the nuclear mass formula,o unknown nuclei far from the stability line it is essentially as accurate as the Hartree-Fock method for a given form of force, but is so much faster that the construction of a complete mass table is feasible. Results of preliminary fits are presented.
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