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Volumn 634, Issue 1-2, 1998, Pages 3-14

Can the equation of state of asymmetric nuclear matter be studied using unstable nuclei?

Author keywords

Asymmetric nuclear matter; EOS; Neutron skin; Nuclear density

Indexed keywords


EID: 0032481951     PISSN: 03759474     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0375-9474(98)00125-0     Document Type: Article
Times cited : (77)

References (24)
  • 20
    • 0010056892 scopus 로고
    • Nuclear shapes in the crust of the neutron stars and in the core of the supernovae
    • ed. S. Kubono, T. Kajino World Scientific, Singapore
    • [20] K. Oyamatsu, in Nuclear Shapes in the Crust of the Neutron Stars and in the Core of the supernovae, Proc. Conf. on Unstable Nuclei in Astrophysics, Hachiooji 1991, ed. S. Kubono, T. Kajino (World Scientific, Singapore, 1992), pp. 327-330.
    • (1992) Proc. Conf. on Unstable Nuclei in Astrophysics, Hachiooji 1991 , pp. 327-330
    • Oyamatsu, K.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.