Polar Quasinormal Modes of Neutron Stars in Massive Scalar-Tensor Theories

Polar Quasinormal Modes of Neutron Stars in Massive Scalar-Tensor Theories

We study polar quasinormal modes of relativistic stars in scalar-tensor theories, where we include a massive gravitational scalar field and employ the standard Brans-Dicke coupling function. For the potential of the scalar field we consider a simple mass term as well as a potential associated with R...

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Bibliographic Details
Main Authors:	Jose Luis Blázquez-Salcedo , Fech Scen Khoo , Jutta Kunz , Vincent Preut
Format:	Article
Language:	English
Published:	Frontiers Media S.A. 2021-09-01
Series:	Frontiers in Physics
Subjects:	relativistic stars - structure and stability modified theories of gravity gravitational waves neutron star quasinormal modes
Online Access:	https://www.frontiersin.org/articles/10.3389/fphy.2021.741427/full

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