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: Blázquez-Salcedo, J.L (Author), Khoo, F.S (Author), Kunz, J. (Author), Preut, V. (Author)
Format: Article
Language:English
Published: Frontiers Media S.A. 2021
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Online Access:View Fulltext in Publisher

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