Neutron star masses in R-2-gravity

We address the issue of the existence of inequivalent definitions of gravitational mass in R-2-gravity. We present several definitions of gravitational mass, and discuss the formal relations between them. We then consider the concrete case of a static and spherically symmetric neutron star, and solv...

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Bibliographic Details
Main Authors: Sbisá, Fulvio (Author) , Baqui, Pedro O. (Author) , Miranda, Tays (Author) , Piattella, Oliver F. (Author)
Format: Article (Journal)
Language:English
Published: 2020
In: Physics of the Dark Universe
Year: 2019, Volume: 27, Pages: 100411
ISSN:2212-6864
DOI:10.1016/j.dark.2019.100411
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1016/j.dark.2019.100411
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Author Notes:Fulvio Sbisa, Pedro O. Baqui, Tays Miranda, Sergio E. Joras and Oliver F. Piattella
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Summary:We address the issue of the existence of inequivalent definitions of gravitational mass in R-2-gravity. We present several definitions of gravitational mass, and discuss the formal relations between them. We then consider the concrete case of a static and spherically symmetric neutron star, and solve numerically the equations of motion for several values of the free parameter of the model. We compare the features of the mass-radius relations obtained for each definition of gravitational mass, and we comment on their dependence on the free parameter. We then argue that R-2-gravity is a valuable proxy to discuss the existence of inequivalent definitions of gravitational mass in a generic modified gravity theory, and present some comments on the general case. (C) 2019 Elsevier B.V. All rights reserved.
Item Description:14 Nov 2019
Gesehen am 14.04.2020
Physical Description:Online Resource
ISSN:2212-6864
DOI:10.1016/j.dark.2019.100411