We use the latest constraints on the population of stellar origin binary black holes (SOBBH)
from LIGO/Virgo/KAGRA (LVK) observations, to estimate the stochastic gravitational wave …

Gravitational-wave observations by the laser interferometer gravitational-wave observatory
(LIGO) and Virgo have provided us a new tool to explore the Universe on all scales from …

It has been recently proposed that Hawking evaporation might slow down after a black hole
has lost about half of its mass. Such an effect, called" memory burden", is parameterized as …

The next generation of ground-based gravitational-wave detectors, the Einstein Telescope
and Cosmic Explorer, present a unique opportunity to put constraints on dense matter …

The detection of a subsolar object in a compact binary merger is regarded as one of the
smoking gun signatures of a population of primordial black holes (PBHs). We critically …

We revise primordial black holes (PBHs) production in the axion-curvaton model, in light of
recent developments in the computation of their abundance accounting for non …

In this study, we use simple performance metrics to assess the science capabilities of future
ground-based gravitational-wave detector networks composed of A+ or Voyager upgrades …

Gravitational-wave signals from binaries that contain spinning black holes in general include
an asymmetry between the+ m and-m multipoles that is not included in most signal models …

The current generation of very-high-energy gamma-ray (VHE; E> 30 GeV) detectors (MAGIC
and HESS) have recently demonstrated the ability to detect the afterglow emission of …

We show that—in the framework of general relativity (GR)—if black holes (BHs) are
singularity-free objects, they couple to the large-scale cosmological dynamics. We find that …