Scalarized black holes in Einstein-scalar-Gauss-Bonnet-Ricci theory exhibit a continuous hierarchy of angular instabilities, starting in the eikonal regime and extending down to the quadrupole mode.
Kobayashi, Rept
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gr-qc 2years
2026 2verdicts
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Linearized Horndeski theory with a scalar potential yields Yukawa-type corrections to Solar-System observables that reduce to GR in heavy-scalar or large-coupling limits, with residual curvature terms from the potential minimum.
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Hierarchy of Angular Instabilities in Scalarized Black Holes
Scalarized black holes in Einstein-scalar-Gauss-Bonnet-Ricci theory exhibit a continuous hierarchy of angular instabilities, starting in the eikonal regime and extending down to the quadrupole mode.
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Linearized Horndeski Theory with a Potential in the Solar System Regime
Linearized Horndeski theory with a scalar potential yields Yukawa-type corrections to Solar-System observables that reduce to GR in heavy-scalar or large-coupling limits, with residual curvature terms from the potential minimum.