In U(1) gauge-invariant scalar–vector–tensor theories with second-order equations of motion, we study the properties of black holes (BH) on a static and spherically symmetric background. In shift-symmetric theories invariant under the shift of scalar ϕ→ϕ+c, we show the existence of new hairy BH solutions where a cubic-order scalar–vector interaction gives rise to a scalar hair manifesting itself around the event horizon. In the presence of a quartic-order interaction besides the cubic coupling, there are also regular BH solutions endowed with scalar and vector hairs
Scalar hair of black holes in theories with a shift symmetry are constrained by the no-hair theorem ...
In the presence of a complex scalar field scalar–tensor theory allows for scalarized rotating hairy ...
Scalar-tensor theories of gravity where a new scalar degree of freedom couples to the Gauss-Bonnet i...
A linear coupling between a scalar field and the Gauss–Bonnet invariant is the only known interactio...
A linear coupling between a scalar field and the Gauss–Bonnet invariant is the only known interactio...
The most general action for a scalar field coupled to gravity that leads to second-order field equat...
International audienceScalar-tensor theories are a natural alternative to general relativity, as the...
International audienceScalar-tensor theories are a natural alternative to general relativity, as the...
International audienceScalar-tensor theories are a natural alternative to general relativity, as the...
International audienceScalar-tensor theories are a natural alternative to general relativity, as the...
A linear coupling between a scalar field and the Gauss–Bonnet invariant is the only known interactio...
In the presence of a complex scalar field scalar–tensor theory allows for scalarized rotating hairy ...
In the presence of a complex scalar field scalar–tensor theory allows for scalarized rotating hairy ...
AbstractIn the presence of a complex scalar field scalar–tensor theory allows for scalarized rotatin...
Scalar-tensor theories of gravity where a new scalar degree of freedom couples to the Gauss-Bonnet i...
Scalar hair of black holes in theories with a shift symmetry are constrained by the no-hair theorem ...
In the presence of a complex scalar field scalar–tensor theory allows for scalarized rotating hairy ...
Scalar-tensor theories of gravity where a new scalar degree of freedom couples to the Gauss-Bonnet i...
A linear coupling between a scalar field and the Gauss–Bonnet invariant is the only known interactio...
A linear coupling between a scalar field and the Gauss–Bonnet invariant is the only known interactio...
The most general action for a scalar field coupled to gravity that leads to second-order field equat...
International audienceScalar-tensor theories are a natural alternative to general relativity, as the...
International audienceScalar-tensor theories are a natural alternative to general relativity, as the...
International audienceScalar-tensor theories are a natural alternative to general relativity, as the...
International audienceScalar-tensor theories are a natural alternative to general relativity, as the...
A linear coupling between a scalar field and the Gauss–Bonnet invariant is the only known interactio...
In the presence of a complex scalar field scalar–tensor theory allows for scalarized rotating hairy ...
In the presence of a complex scalar field scalar–tensor theory allows for scalarized rotating hairy ...
AbstractIn the presence of a complex scalar field scalar–tensor theory allows for scalarized rotatin...
Scalar-tensor theories of gravity where a new scalar degree of freedom couples to the Gauss-Bonnet i...
Scalar hair of black holes in theories with a shift symmetry are constrained by the no-hair theorem ...
In the presence of a complex scalar field scalar–tensor theory allows for scalarized rotating hairy ...
Scalar-tensor theories of gravity where a new scalar degree of freedom couples to the Gauss-Bonnet i...