Truncated post-Newtonian neutron star model
نویسندگان
چکیده
منابع مشابه
Numerical Models of Newtonian and Post-Newtonian Binary Neutron Star Mergers
This article describes a comparison of two calculations of the merger of a binary neutron star (NS) system which is initially within the tidal instability as described by Rasio & Shapiro [1, 2]. The same initial data is used with one simulation involving a purely Newtonian evolution of the Euler equations for compressible fluids and another similarly evolved except there is an inclusion of a gr...
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ژورنال
عنوان ژورنال: Physical Review D
سال: 1999
ISSN: 0556-2821,1089-4918
DOI: 10.1103/physrevd.60.067504