Neutron stars in the bimetric scalar—tensor theory of gravitation. II. solutions with a variable scalar field

被引：0
作者：
L. Sh Grigorian
P. F. Kazarian
H. F. Khachatrian
机构：
[1] Institute of Applied Physics Problems,
[2] Erevan State University,undefined
来源：
Astrophysics | 1998年 / 41卷 / 1期
关键词：
Scalar Field; Neutron Star; Gravitational Field; Celestial Body; Central Pressure;
D O I：
10.1007/BF03036056
中图分类号：
学科分类号：
摘要：
Solutions of the equations of the bimetric scalar—tensor theory of gravitation with a variable scalar field are found for configurations of superdense matter with different versions of the equation of state. The possible existence of static superdense and supermassive configurations is established for all of the versions of the equation of state of superdense matter used.
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页码：85 / 88
页数：3
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