Self-interactions can (also) destabilize bosonic stars

DOI10.1088/1361-6382/AD7188zbMATH Open1547.83051MaRDI QIDQ6603944

Marco Brito, Nicolas Sanchis-Gual, Carlos Herdeiro, Miguel Zilhão, Etevaldo dos Santos Costa Filho

Publication date: 12 September 2024

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

zbMATH Keywords

spherical symmetryHiggs fieldminimal couplingnumerical relativityvector bosonsboson starProca star

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Cites Work

• Formulations of the \(3+1\) evolution equations in curvilinear coordinates
• Efficient vectorizable PDE solvers
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• Asymptotically flat spinning scalar, Dirac and Proca stars
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• Numerical integration of Einstein’s field equations
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• General relativistic boson stars
• Comparing timelike geodesics around a Kerr black hole and a boson star
• The imitation game: Proca stars that can mimic the Schwarzschild shadow
• Soliton boson stars, Q-balls and the causal Buchdahl bound
• A stabilization mechanism for excited fermion–boson stars
• Boson stars in Palatini f(R) gravity
• Self-interactions can stabilize excited boson stars
• The well-posedness of the Cauchy problem for self-interacting vector fields
• Kerr black holes with synchronised Proca hair: lensing, shadows and EHT constraints
• Gauss-Bonnet boson stars
• Proca-Higgs balls and stars in a UV completion for Proca self-interactions
• Proca stars with dark photons from spontaneous symmetry breaking of the scalar field dark matter

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