We present a comparative study of spherically symmetric, localized, particle-like solutions for spin s=0,1/2 and 1 gravitating fields in a D-dimensional, asymptotically flat spacetime. These fields are massive, possessing a harmonic time dependence and no self-interaction. Special attention is paid to the mathematical similarities and physical differences between the bosonic and fermionic cases. We find that the generic pattern of solutions is similar for any value of the spin s, depending only on the dimensionality of spacetime, the cases D=4,5 being special.publishe
International audienceWe have developed a highly accurate numerical code capable of solving the coup...
AbstractWe establish that massive complex Abelian vector fields (mass μ) can form gravitating solito...
To describe a massive particle with fixed, but arbitrary, spin on d=4 anti-de Sitter space M^4, we p...
Einstein's gravity minimally coupled to free, massive, classical fundamental fields admits particle-...
The existence of localized, approximately stationary, lumps of the classical gravitational and elect...
We present a comparative analysis of the self-gravitating solitons that arise in the Einstein–Klein–...
AbstractWe establish that massive complex Abelian vector fields (mass μ) can form gravitating solito...
The existence of localized, approximately stationary, lumps of the classical gravitational and elect...
We establish that massive complex Abelian vector fields (mass μ) can form gravitating solitons, when...
We establish that massive complex Abelian vector fields (mass mu) can form gravitating solitons, whe...
We present an approximate solution to the minimally coupled Einstein-Dirac equations. We interpret t...
Scalar boson stars and Dirac stars are solitonic solutions of the Einstein{Klein-Gordon and Einstei...
International audienceWe have developed a highly accurate numerical code capable of solving the coup...
International audienceWe have developed a highly accurate numerical code capable of solving the coup...
In this paper, we construct \textit{Dirac-boson stars} (DBSs) model composed of a scalar field and t...
International audienceWe have developed a highly accurate numerical code capable of solving the coup...
AbstractWe establish that massive complex Abelian vector fields (mass μ) can form gravitating solito...
To describe a massive particle with fixed, but arbitrary, spin on d=4 anti-de Sitter space M^4, we p...
Einstein's gravity minimally coupled to free, massive, classical fundamental fields admits particle-...
The existence of localized, approximately stationary, lumps of the classical gravitational and elect...
We present a comparative analysis of the self-gravitating solitons that arise in the Einstein–Klein–...
AbstractWe establish that massive complex Abelian vector fields (mass μ) can form gravitating solito...
The existence of localized, approximately stationary, lumps of the classical gravitational and elect...
We establish that massive complex Abelian vector fields (mass μ) can form gravitating solitons, when...
We establish that massive complex Abelian vector fields (mass mu) can form gravitating solitons, whe...
We present an approximate solution to the minimally coupled Einstein-Dirac equations. We interpret t...
Scalar boson stars and Dirac stars are solitonic solutions of the Einstein{Klein-Gordon and Einstei...
International audienceWe have developed a highly accurate numerical code capable of solving the coup...
International audienceWe have developed a highly accurate numerical code capable of solving the coup...
In this paper, we construct \textit{Dirac-boson stars} (DBSs) model composed of a scalar field and t...
International audienceWe have developed a highly accurate numerical code capable of solving the coup...
AbstractWe establish that massive complex Abelian vector fields (mass μ) can form gravitating solito...
To describe a massive particle with fixed, but arbitrary, spin on d=4 anti-de Sitter space M^4, we p...