Neutron Stars in <i>f</i>(<i>R</i>)-Gravity and Its Extension with a Scalar Axion Field

We present a brief review of general results about non-rotating neutron stars in simple <inline-formula> <math display="inline"> <semantics> <msup> <mi>R</mi> <mn>2</mn> </msup> </semantics> </math> </inline-formula> g...

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Bibliographic Details
Main Authors: Artyom Astashenok, Sergey Odintsov
Format: Article
Language:English
Published: MDPI AG 2020-07-01
Series:Particles
Subjects:
Online Access:https://www.mdpi.com/2571-712X/3/3/36
Description
Summary:We present a brief review of general results about non-rotating neutron stars in simple <inline-formula> <math display="inline"> <semantics> <msup> <mi>R</mi> <mn>2</mn> </msup> </semantics> </math> </inline-formula> gravity and its extension with a scalar axion field. Modified Einstein equations are presented for metrics in isotropical coordinates. The mass–radius relation, mass profile and dependence of mass from central density on various equations of state are given in comparison to general relativity.
ISSN:2571-712X