We study charged and radially excited boson stars in both asymptotically flat as well as asymptotically Anti-de Sitter space-time. We demonstrate that two different types of radially excited solutions exist~: one that persists in the linear limit of small scalar fields, in which analytical arguments suggest the existence of these solutions, and one that appears only in the highly non-linear regime of the model. We also demonstrate that the formation of wavy scalar hair discussed previously for black holes and boson stars in asymptotically flat space-time persists for asymptotically Anti-de Sitter space-time
21 pages, 4 figuresInternational audienceStatic, charged black holes in the presence of a negative c...
In the realm of lower-dimensional accelerating spacetimes, it is well-established that the presence ...
In the large coupling regime of the 5-dimensional Einstein–Maxwell–Chern–Simons theory, charged and ...
We study axially symmetric solutions of the Einstein–Maxwell–Klein–Gordon equations describing spinn...
A scalar field non-minimally coupled to certain geometric [or matter] invariants which are sourced b...
We study charged boson stars in scalar-tensor (ST) gravitational theories. We analyze the weak field...
The existence of localized, approximately stationary, lumps of the classical gravitational and elect...
In this paper, we follow up on the discovery of a new type of solution in the Einstein-Maxwell syste...
Abstract: We study the interior of a recently constructed family of asymptotically flat, charged bla...
Boson stars are configurations of the gravitating complex scalar field in the Einstein’s GeneralTheo...
The Einstein-conformally coupled scalar field system is studied in the presence of a cosmological co...
AbstractWe present new spherically symmetric solutions of an SU(2) Einstein–Yang–Mills model coupled...
Sherpa Romeo green journal. Permission to archive final published version.We describe a class of asy...
In the standard asymptotic expansion of four dimensional static asymptotically flat spacetimes, the ...
We investigate the thermodynamics of spherically symmetric black hole solutions in a four-dimensiona...
21 pages, 4 figuresInternational audienceStatic, charged black holes in the presence of a negative c...
In the realm of lower-dimensional accelerating spacetimes, it is well-established that the presence ...
In the large coupling regime of the 5-dimensional Einstein–Maxwell–Chern–Simons theory, charged and ...
We study axially symmetric solutions of the Einstein–Maxwell–Klein–Gordon equations describing spinn...
A scalar field non-minimally coupled to certain geometric [or matter] invariants which are sourced b...
We study charged boson stars in scalar-tensor (ST) gravitational theories. We analyze the weak field...
The existence of localized, approximately stationary, lumps of the classical gravitational and elect...
In this paper, we follow up on the discovery of a new type of solution in the Einstein-Maxwell syste...
Abstract: We study the interior of a recently constructed family of asymptotically flat, charged bla...
Boson stars are configurations of the gravitating complex scalar field in the Einstein’s GeneralTheo...
The Einstein-conformally coupled scalar field system is studied in the presence of a cosmological co...
AbstractWe present new spherically symmetric solutions of an SU(2) Einstein–Yang–Mills model coupled...
Sherpa Romeo green journal. Permission to archive final published version.We describe a class of asy...
In the standard asymptotic expansion of four dimensional static asymptotically flat spacetimes, the ...
We investigate the thermodynamics of spherically symmetric black hole solutions in a four-dimensiona...
21 pages, 4 figuresInternational audienceStatic, charged black holes in the presence of a negative c...
In the realm of lower-dimensional accelerating spacetimes, it is well-established that the presence ...
In the large coupling regime of the 5-dimensional Einstein–Maxwell–Chern–Simons theory, charged and ...