Published May 2018 | Version v1
Journal article Metadata-only

On stability of a neutron star system in Palatini gravity

Creators

  • 1. Maria Curie-Sklodowska University, Institute of Physics, Lublin (Poland)

Description

We formulate the generalized Tolman-Oppenheimer-Volkoff equations for the f(R) Palatini gravity in the case of static and spherical symmetric geometry. We also show that a neutron star can be a stable system independently of the form of the functional f(R). (orig.)

Availability note (English)

Available from: http://dx.doi.org/10.1140/epjc/s10052-018-5900-3

Additional details

Identifiers

DOI
10.1140/epjc/s10052-018-5900-3;

Publishing Information

Journal Title
European Physical Journal. C, Particles and Fields (Online)
Journal Volume
78
Journal Issue
5
Journal Page Range
p. 1-8
ISSN
1434-6052

INIS

Country of Publication
Germany
Country of Input or Organization
Germany
INIS RN
49060332
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
FIELD EQUATIONS; FUNCTIONALS; GENERAL RELATIVITY THEORY; GRAVITATION; LAGRANGE EQUATIONS; LAGRANGIAN FIELD THEORY; NEUTRON STARS; SPHERICAL CONFIGURATION; STABILITY; STEADY-STATE CONDITIONS
Descriptors DEC
CONFIGURATION; DIFFERENTIAL EQUATIONS; EQUATIONS; FIELD THEORIES; FUNCTIONS; PARTIAL DIFFERENTIAL EQUATIONS; QUANTUM FIELD THEORY; RELATIVITY THEORY; STARS