Self-interactions can (also) destabilize bosonic stars
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Publication:6603944
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)
Cites Work
- Formulations of the \(3+1\) evolution equations in curvilinear coordinates
- Efficient vectorizable PDE solvers
- Hairy black holes, boson stars and non-minimal coupling to curvature invariants
- Asymptotically flat spinning scalar, Dirac and Proca stars
- Evolution of three-dimensional gravitational waves: Harmonic slicing case
- Numerical integration of Einstein’s field equations
- SUPERMASSIVE BLACK HOLES OR BOSON STARS? HAIR COUNTING WITH GRAVITATIONAL WAVE DETECTORS
- 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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