Constraining Dense Matter Physics Using <i>f</i>-Mode Oscillations in Neutron Stars
In this paper, an investigation of the role of nuclear saturation parameters on <i>f</i>-mode oscillations in neutron stars is performed within the Cowling approximation. It is found that the uncertainty in the effective nucleon mass plays a dominant role in controlling the <i>f</i>-mode frequencies...
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| Médium: | Artigo |
| Jazyk: | Inglês |
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MDPI AG
2021-05-01
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| Edice: | Physics |
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| On-line přístup: | https://www.mdpi.com/2624-8174/3/2/22 |
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