Shape of Nuclei in the Crust of Neutron Star : Nuclear Physics
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概要
- 論文の詳細を見る
The stable nuclear shape in very dense matter composed of protons, neutrons and electrons is investigated. It is shown that, as the density of the matter increases from 10^<13> to 10^<14.5> g cm^<-3>, the stable nuclear shape is likely to change successively from sphere to cylinder, board, cylindrical hole and spherical hole before uniform neutron-star matter is formed.
- 理論物理学刊行会の論文
- 1984-02-25
著者
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HASHIMOTO Masa-aki
Department of Physics, Kyushu University
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Hashimoto Masa-aki
Department Of Earth Science And Astronomy College Of Arts And Sciences University Of Tokyo
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Hashimoto Masa-aki
Department Of Physics And Applied Physics Waseda University
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YAMADA Masami
Science and Engineering Research Laboratory, Waseda University
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SEKI Hironori
Department of Physics and Applied Physics, Waseda University
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Seki Hironori
Department Of Physics And Applied Physics Waseda University
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Yamada Masami
Science And Engineering Research Laboratory Waseda University
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HASHIMOTO Masa-aki
Department of Physics and Applied Physics, Waseda University
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YAMADA Masami
Advancde Research Institute for Science and Engineering, Wasede University
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