Phenomenology of axionic static neutron stars with masses in the mass-gap region
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Publication:6561037
DOI10.1088/1361-6382/AD33CDzbMATH Open1543.83041MaRDI QIDQ6561037
Publication date: 24 June 2024
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
polytropic equation of stateneutron starsscalar-tensor theoryTolman-Oppenheimer-Volkoff equationsaxions
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Cites Work
- Extended gravity description for the GW190814 supermassive neutron star
- Rectifying Einstein-Gauss-Bonnet inflation in view of GW170817
- Stellar structure models in modified theories of gravity: lessons and challenges
- Compact star in general \(F(R)\) gravity: inevitable degeneracy problem and non-integer power correction
- Neutron stars in scalar-tensor gravity with quartic order scalar potential
- Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
- Energy and the Criteria for Radiation in General Relativity
- Slowly rotating anisotropic neutron stars in general relativity and scalar–tensor theory
- Tensor-multi-scalar theories: relativistic stars and 3 + 1 decomposition
- Natural inflation with a nonminimal coupling to gravity
- Axion kinetic misalignment and parametric resonance from inflation
- Bottom-up reconstruction of viable GW170817 compatible Einstein–Gauss–Bonnet theories
- Universal inflationary attractors implications on static neutron stars
- A refined Einstein–Gauss–Bonnet inflationary theoretical framework
- Static neutron stars perspective of quadratic and induced inflationary attractor scalar-tensor theories
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