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Cosmology with subdominant Horndeski scalar field
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We study the cosmological evolution of a scalar field in Horndeski gravity, assuming that the scalar field is subdominant with respect to the cosmic fluid. We first analyse the most general shift-symmetric action that respects local Lorentz symmetry. We show that the bound on the speed of gravitational waves set by GW170817+GRB170817A imposes a constraint only on the linear coupling between the scalar and the Gauss-Bonnet invariant and this constraint is rather mild. Then, we consider some interesting examples of theories that break shift-symmetry, such as the Damour-Esposito-Far\`ese model of spontaneous scalarization and a theory with a quadratic coupling to the Gauss-Bonnet invariant that can lead to black hole scalarization. In both cases, tuning of cosmological initial conditions is necessary to keep the scalar field dormant during cosmic evolution.
Forward citations
Cited by 3 Pith papers
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Spontaneous scalarization of charged black holes in the Scalar-Vector-Tensor theory
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A kinetic cubic Horndeski coupling creates an ultra-slow-roll phase that amplifies curvature perturbations enough to produce asteroid-mass primordial black holes, potentially 90% of dark matter.
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Compact Objects in Einstein-scalar-Gauss-Bonnet Theory and beyond
A review of compact-object solutions in Einstein-scalar-Gauss-Bonnet and Horndeski theories, emphasizing scalarized black holes, traversable wormholes, and bubble-like particle solutions.
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