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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https://www.frontiersin.org/articles/10.3389/fphy.2021.741427/full

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