activity
20242026
most citedThe Science of the Einstein Telescope

97 citations · 193 across the 15 of their papers we have counts for

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Showing astro-ph.COShow all

13 papers · 1 filter

astro-ph.CO2026

Memoirs of the curvaton: non-perturbative non-Gaussianity and supermassive primordial black holes

S. Allegrini, A. J. Iovino, G. Perna +1

The curvaton provides a simple mechanism for generating strongly non-Gaussian curvature perturbations after inflation, with potentially important consequences on small scales. We s…

astro-ph.CO2026

Exploring Gravitational Wave Signatures Due to Primordial Non-gaussianity and Large Scale Structure Using SKAO

H. V. Ragavendra, Giulia Capurri, Alina Mierna +8

This chapter explores theoretical and observational strategies to use the stochastic gravitational-wave background detectable by Square Kilometre Array Observatory (SKAO) as a prob…

astro-ph.CO2026

Probing non-Gaussianity during reheating with SIGW in the LISA band

Gabriele Perna, Guillem Domènech

We analyse the effects of a non-standard evolution of the Universe during the reheating epoch on the spectrum of scalar-induced gravitational waves (SIGWs) accounting for the prese…

astro-ph.CO2026

Probing Cosmic Expansion and Early Universe with Einstein Telescope

Angelo Ricciardone, Mairi Sakellariadou, Archisman Ghosh +52

Over the next two decades, gravitational-wave (GW) observations are expected to evolve from a discovery-driven endeavour into a precision tool for astrophysics, cosmology, and fund…

astro-ph.CO2026★ 15 cited

Primordial black holes: constraints, potential evidence and prospects

Bernard Carr, Antonio J. Iovino, Gabriele Perna +2

Primordial black holes (PBHs) may have formed in the early Universe and may account for all or part of the dark matter. In this review, we summarize the current observational const…

astro-ph.CO2025

From the Solar System to cosmological distances: a complete formalism for gravitational wave astrometry

Gabriele Perna, Nicola Bellomo, Vincenzo Roatti +1

The presence of a gravitational wave background (GWB) can be established not only via exquisitely precise pulsar timing array (PTA) measurements, but also via astrometric observati…

astro-ph.CO2025

The impact of non-Gaussianity when searching for Primordial Black Holes with LISA

Antonio Junior Iovino, Gabriele Perna, Hardi Veermäe

LISA can observe cosmological millihertz (mHz) gravitational wave (GW) backgrounds that may offer a decisive test for asteroid-mass primordial black hole (PBH) dark matter (DM). In…

astro-ph.CO2025★ 13 cited

The Irrelevance of Primordial Black Hole Clustering in the LVK mass range

F. Crescimbeni, V. Desjacques, G. Franciolini +6

We show that in realistic models where primordial black holes are formed due to the collapse of sizeable inflationary perturbations, their initial spatial clustering beyond Poisson…

astro-ph.CO2025

Reconstructing Primordial Curvature Perturbations via Scalar-Induced Gravitational Waves with LISA

Jonas El Gammal, Aya Ghaleb, Gabriele Franciolini +17

Many early universe scenarios predict an enhancement of scalar perturbations at scales currently unconstrained by cosmological probes. These perturbations source gravitational wave…

astro-ph.CO2024★ 6 cited

How Well Do We Know the Scalar-Induced Gravitational Waves?

A. J. Iovino, S. Matarrese, G. Perna +2

Gravitational waves sourced by amplified scalar perturbations are a common prediction across a wide range of cosmological models. These scalar curvature fluctuations are inherently…

astro-ph.CO2024★ 49 cited

Curbing PBHs with PTAs

A. J. Iovino, G. Perna, A. Riotto +1

Sizeable primordial curvature perturbations needed to seed a population of primordial black holes (PBHs) will be accompanied by a scalar-induced gravitational wave signal that can…

astro-ph.CO2024★ 13 cited

Investigating the impact of galaxies' compact binary hosting probability for gravitational-wave cosmology

Gabriele Perna, Simone Mastrogiovanni, Angelo Ricciardone

With the advent of future-generation interferometers a huge number of Gravitational Wave (GW) signals is expected to be measured without an electromagnetic counterpart. Although th…

astro-ph.CO2024

Fully non-Gaussian Scalar-Induced Gravitational Waves

Gabriele Perna, Chiara Testini, Angelo Ricciardone +1

Scalar-induced Gravitational Waves (SIGWs) represent a particular class of primordial signals which are sourced at second-order in perturbation theory whenever a scalar fluctuation…