We consider the status of black hole (BH) solutions with nontrivial scalar fields but no gauge
fields, in four-dimensional asymptotically flat spacetimes, reviewing both classical results …

Searching for violations of the no-hair theorem (NHT) is a powerful way to test gravity, and
more generally fundamental physics, particularly with regards to the existence of additional …

Bekenstein proved that in Einstein's gravity minimally coupled to one (or many) real,
Abelian, Proca field, stationary black holes (BHs) cannot have Proca hair. Dropping …

Symmetric teleparallel gravity is constructed with a nonzero nonmetricity tensor while both
torsion and curvature are vanishing. In this framework, we find exact scalarised spherically …

A bstract Spherical black hole (BH) solutions in Einstein-Maxwell-scalar (EMS) models
wherein the scalar field is non-minimally coupled to the Maxwell invariant by some coupling …

In this paper, we are interested in a model of exact asymptotically flat charged hairy black
holes in the background of a dilaton potential. We study the weak gravitational lensing in the …

In the framework of a simple gravitational theory that contains a scalar field minimally
coupled to gravity, we investigate the emergence of analytic black-hole solutions with …

We present and discuss new families of primary hair charged black hole solutions in
asymptotically anti–de Sitter space in three dimensions. The coupled Einstein-Maxwell …

A bstract Small black holes are a powerful tool to explore infinite distances in moduli spaces.
However, we show that in 4d theories with a scalar potential growing fast enough at infinity …

With the complexity of information tasks, the bipartite and tripartite entanglement can no
longer meet our needs, and we need more entangled particles to process relativistic …