activity
20122026
most citedScience Case for the Einstein Telescope

1.2k citations · 6k across the 77 of their papers we have counts for

collaborators

85 papers

eess.SP2026

To Stack or Not to Stack? Jacobian Conditioning and the Benefits of Depth in Metasurface-Based Linear Transformation Synthesis

Andrea Abrardo, Andrea Garulli

This paper investigates when and why stacking programmable metasurfaces into Stacked Intelligent Metasurfaces (SIMs) improves linear transformation synthesis at a fixed phase-contr…

gr-qc2026

Architecture Acceleration of Machine Learning Gravitational Waveform Surrogate Models

Adriano Frattale Mascioli, Lorenzo Piccari, Saulo Albuquerque +9

Accurate and computationally efficient waveform models of compact binary coalescences are a fundamental requirement for gravitational wave data analysis. This work presents differe…

astro-ph.CO2026

Constraining primordial non-Gaussianity and parity-violation through Scalar-Induced Gravitational Waves with next-generation ground-based interferometers

Ilaria Caporali, H. V. Ragavendra, Angelo Ricciardone +1

In this work, we investigate the prospects for probing primordial non-Gaussianity and associated symmetry of parity through scalar-induced gravitational waves (SIGWs), with third-g…

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

Tracing Primordial Gravitational Waves via non-Gaussian Signatures of Halo Bias

Mariam Abdelaziz, Pritha Bari, Sabino Matarrese +1

Primordial gravitational waves (PGWs) generate scalar density perturbations at second order. Since the induced density contrast is quadratic in the tensor field, it is intrinsicall…

astro-ph.CO2026

Probing scalar-tensor-induced gravitational waves in the nHz band: NANOGrav and SKA

William Iania, Angelo Ricciardone

Scalar-induced gravitational waves (SIGWs) have recently attracted considerable interest, both as a possible explanation for the nanohertz signal reported by the Pulsar Timing Arra…

astro-ph.CO2026

Inflation without an Inflaton III: non-Gaussian signatures

Mariam Abdelaziz, Marisol Traforetti, Daniele Bertacca +3

We investigate primordial non-Gaussianity in the Inflation without an Inflaton (IWI) framework, where scalar perturbations are generated at second order by primordial gravitational…

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…

gr-qc2026

The Sequential Monte Carlo goes NUTS: Boosting Gravitational-Wave Inference

Gabriele Demasi, Giulia Capurri, Massimo Lenti +9

Sequential Monte Carlo (SMC) methods have recently been applied to gravitational-wave inference as a powerful alternative to standard sampling techniques, such as Nested Sampling.…

astro-ph.CO2025

Updated and Projected Cosmic Microwave Background Bounds on WIMP Annihilation

Charlotte Myers, Dominic Agius, Daniele Gaggero +1

We derive updated Cosmic Microwave Background (CMB) constraints on annihilating dark matter, and present forecasts for upcoming CMB surveys. We show that the addition of recent tem…

astro-ph.CO2025

Inflation without an Inflaton II: observational predictions

Marisol Traforetti, Mariam Abdelaziz, Daniele Bertacca +3

We present a complete computation of the scalar power spectrum in the \emph{inflation without inflaton} (IWI) framework, where the inflationary expansion is driven solely by a de~S…

gr-qc2025

Tests of General Relativity with Einstein Telescope

Andrea Begnoni, Walter Del Pozzo, Matteo Pegorin +2

Gravitational wave signals from compact binary coalescences provide powerful and reliable probes of General Relativity. To date, the LIGO-Virgo-KAGRA collaboration has provided str…

stat.CO2025

samsara: A Continuous-Time Markov Chain Monte Carlo Sampler for Trans-Dimensional Bayesian Analysis

Gabriele Astorino, Lorenzo Valbusa Dall'Armi, Riccardo Buscicchio +3

Bayesian inference requires determining the posterior distribution, a task that becomes particularly challenging when the dimension of the parameter space is large and unknown. Thi…

astro-ph.IM2025

\texttt{GWBird}: a toolkit for the characterization of the Stochastic Gravitational Wave Background for Ground, Space, and Pulsar Timing Array detectors

Ilaria Caporali, Angelo Ricciardone

The detection of the Stochastic Gravitational Wave Background (SGWB) is one of the most challenging tasks for both current and next-generation detectors. Successfully distinguishin…

gr-qc2025

Quantum production of gravitational waves after inflation

Alina Mierna, Gabriele Perna, Sabino Matarrese +2

A variety of mechanisms in the early Universe lead to the generation of gravitational waves (GWs). We introduce here a novel source of GWs generated by vacuum fluctuations after in…

astro-ph.CO2025★ 1 cited

Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia

Andrea Begnoni, Stefano Anselmi, Mauro Pieroni +2

Future gravitational-wave (GW) detectors are expected to detect tens of thousands of compact binary coalescences (CBC) per year, depending also on the final detectors layout. For t…

gr-qc2025

Likelihoods for Stochastic Gravitational Wave Background Data Analysis

Gabriele Franciolini, Mauro Pieroni, Angelo Ricciardone +1

We present a systematic study of likelihood functions used for Stochastic Gravitational Wave Background (SGWB) searches. By dividing the data into many short segments, one customar…

astro-ph.CO2025★ 2 cited

Non-Gaussianity of Tensor Induced Density Perturbations

Mariam Abdelaziz, Pritha Bari, Sabino Matarrese +1

We investigate the non-Gaussianity of second-order matter density perturbations induced by primordial gravitational waves (GWs). These tensor-induced scalar modes arise from local…

gr-qc2025★ 97 cited

The Science of the Einstein Telescope

Adrian Abac, Raul Abramo, Simone Albanesi +485

Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science ob…

gr-qc2025★ 6 cited

Scalar-Induced Gravitational Waves in Modified Gravity

Anjali Abirami Kugarajh, Marisol Traforetti, Andrea Maselli +2

Scalar-Induced Gravitational Waves (SIGWs), second-order tensor modes sourced by first-order scalar fluctuations in General Relativity (GR), are expected to contribute to the Stoch…

gr-qc2025

Impact of correlated noise on the reconstruction of the stochastic gravitational wave background with Einstein Telescope

Ilaria Caporali, Giulia Capurri, Walter Del Pozzo +2

Einstein Telescope (ET) is a proposed next-generation Gravitational Wave (GW) interferometer designed to detect a large number of astrophysical and cosmological sources with unprec…

gr-qc2025★ 34 cited

Challenges and Opportunities of Gravitational Wave Searches above 10 kHz

Nancy Aggarwal, Odylio D. Aguiar, Diego Blas +34

The first direct measurement of gravitational waves by the LIGO and Virgo collaborations has opened up new avenues to explore our Universe. This white paper outlines the challenges…

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

Inflation without an Inflaton

Daniele Bertacca, Raul Jimenez, Sabino Matarrese +1

We propose a novel scenario in which scalar perturbations, that seed the large scale structure of the Universe, are generated without relying on a scalar field (the inflaton). In t…