Stabilization of spherically symmetric static boson stars by Coleman-Weinberg self-interaction potential
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Publication:6670841
DOI10.1016/J.NUCLPHYSB.2024.116764MaRDI QIDQ6670841
Hossein Ghaffarnejad, F. Eidizadeh
Publication date: 24 January 2025
Published in: Nuclear Physics B (Search for Journal in Brave)
Cites Work
- Title not available (Why is that?)
- Title not available (Why is that?)
- Boson and neutron stars with increased density
- Dynamical system approach to scalar-vector-tensor cosmology
- Lorentzian causality theory
- Physical Foundations of Cosmology
- Gravastars must have anisotropic pressures
- On the stability of electrostatics stars with modified non-gauge invariant Einstein-Maxwell gravity
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