Formation of Nuclear "Pasta" in Cold Neutron Star Matter
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概要
- 論文の詳細を見る
Formation and decay of rod-like and slab-like nuclei, as may be encountered in the outer parts of neutron stars, are examined within a zero-temperature stability analysis with respect to perturbations inducing fission and proton clustering. The nonspherical nuclei are found to be stable against these perturbations, implying the possibility that the size of the stellar region containing such nuclei exceeds the equilibrium prediction.
- 理論物理学刊行会の論文
- 2001-09-25
著者
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SATO Katsuhiko
Department of Physics, Kyoto University
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Iida K
Inst. Physical And Chemical Res. (riken) Wako Jpn
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Iida Kei
Department Of Clinical Pharmacology And Therapeutics Hamamatsu University School Of Medicine
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WATANABE Gentaro
Department of Physics, School of Science, The University of Tokyo
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Sato Katsuhiko
Department Of Cardiovascular Medicine Hokkaido University School Of Medicine
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Watanabe Gentaro
Department Of Physics School Of Science The University Of Tokyo
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Koi SATO
Department of Physics, Nagoya University
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IIDA Kei
Department of Physics,University of Tokyo
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IIDA Kei
Department of Physics, University of Tokyo:Department of Physics, University of Illinois at Urbana-Champaign
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SATO Katsuhiko
Research Center for the Early Universe (RESCEU), School of Science, University of Tokyo:Departrment of Physics, Scool of Science, University of Tokyo
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WATANABE Gentaro
Department of Physics, University of Tokyo:Division of Computational Science, RIKEN
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WATANABE Gentaro
RIKEN:Department of Physics, University of Tokyo
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