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	Three-body forces and neutron star structure
	Zhou, X. R. ; Burgio, G. F. ; Lombardo, U. ; Schulze, H. J. ; Zuo, W. ; Zhou XR(周先荣)
	2004
关键词	MONTE-CARLO CALCULATIONS NUCLEAR-MATTER TRANSITION EQUATION EOS
英文摘要	We calculate the nucleonic equation of state within the Brueckner-Bethe-Goldstone formalism using the Argonne v(18) two-body interaction and a three-body interaction. We adopt two different three-body forces: the phenomenological Urbana IX model and a microscopic meson-exchange force including nucleon virtual excitations and nucleon-antinucleon excitations. We compare their respective predictions regarding the structure of neutron stars, in particular the mass-radius relation.
语种	英语
内容类型	期刊论文
源URL	[http://dspace.xmu.edu.cn/handle/2288/68876]
专题	物理技术－已发表论文
推荐引用方式 GB/T 7714	Zhou, X. R.,Burgio, G. F.,Lombardo, U.,et al. Three-body forces and neutron star structure[J],2004.
APA	Zhou, X. R.,Burgio, G. F.,Lombardo, U.,Schulze, H. J.,Zuo, W.,&周先荣.(2004).Three-body forces and neutron star structure..
MLA	Zhou, X. R.,et al."Three-body forces and neutron star structure".(2004).

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