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...
| Main Authors: | , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Frontiers Media S.A.
2021
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| Subjects: | |
| Online Access: | View Fulltext in Publisher |