Neutron and quark stars in f (R) gravity

被引：18

作者：

Astashenok, Artyom V. ^{[1
]}

机构：

[1] I Kant Baltic Fed Univ, Inst Phys & Technol, Nevskogo 14, Kaliningrad 236041, Russia

来源：

PROCEEDINGS OF THE 9TH ALEXANDER FRIEDMANN INTERNATIONAL SEMINAR ON GRAVITATION AND COSMOLOGY AND 3RD SATELLITE SYMPOSIUM ON THE CASIMIR EFFECT | 2016年 / 41卷

关键词：

Modified gravity; neutron stars; strange stars; STRONG MAGNETIC-FIELDS; LAMBDA; MATTER; STATE;

D O I：

10.1142/S2010194516601307

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The realistic compact star models are considered in f (R) gravity. The main result is that simple modified gravity can be consistent with current observational mass limit of neutron stars, with current data on their masses and radii; also, it simplifies solution of the hyperon problem. The effect of strong magnetic field in R-2-gravity is also investigated. The existence of more compact (in comparison with General Relativity) stars with large magnetic fields in central regions is possible. In fact the second branch of stability appears.

引用

页数：9

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