SearcharxivSearch

arXiv · 2503.12263

The Science of the Einstein Telescope

Adrian Abac·Raul Abramo·Simone Albanesi·Angelica Albertini·Alessandro Agapito·Michalis Agathos·Conrado Albertus·Nils Andersson·Tomas Andrade·Igor Andreoni·Federico Angeloni·Marco Antonelli·John Antoniadis·Fabio Antonini·Manuel Arca Sedda·M. Celeste Artale·Stefano Ascenzi·Pierre Auclair·Matteo Bachetti·Charles Badger·Biswajit Banerjee·David Barba-Gonzalez·Daniel Barta·Nicola Bartolo·Andreas Bauswein·Andrea Begnoni·Freija Beirnaert·Michal Bejger·Enis Belgacem·Nicola Bellomo·Laura Bernard·Maria Grazia Bernardini·Sebastiano Bernuzzi·Christopher P. L. Berry·Emanuele Berti·Gianfranco Bertone·Dario Bettoni·Miguel Bezares·Swetha Bhagwat·Sofia Bisero·Marie Anne Bizouard·Jose J. Blanco-Pillado·Simone Blasi·Alice Bonino·Alice Borghese·Ssohrab Borhanian·Elisa Bortolas·Maria Teresa Botticella·Marica Branchesi·Matteo Breschi·Richard Brito·Enzo Brocato·Floor S. Broekgaarden·Tomasz Bulik·Alessandra Buonanno·Fiorella Burgio·Adam Burrows·Gianluca Calcagni·Sofia Canevarolo·Enrico Cappellaro·Giulia Capurri·Carmelita Carbone·Roberto Casadio·Ramiro Cayuso·Pablo Cerda-Duran·Prasanta Char·Sylvain Chaty·Tommaso Chiarusi·Martyna Chruslinska·Francesco Cireddu·Philippa Cole·Alberto Colombo·Monica Colpi·Geoffrey Compere·Carlo Contaldi·Maxence Corman·Francesco Crescimbeni·Sergio Cristallo·Elena Cuoco·Giulia Cusin·Tito Dal Canton·Gergely Dalya·Paolo D'Avanzo·Nazanin Davari·Valerio De Luca·Viola De Renzis·Massimo Della Valle·Walter Del Pozzo·Federico De Santi·Alessio Ludovico De Santis·Tim Dietrich·Ema Dimastrogiovanni·Guillem Domenech·Daniela Doneva·Marco Drago·Ulyana Dupletsa·Hannah Duval·Irina Dvorkin·Nancy Elias-Rosa·Stephen Fairhurst

Abstract

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 objectives, providing state-of-the-art predictions for the capabilities of ET in both geometries currently under consideration, a single-site triangular configuration or two L-shaped detectors. We discuss the impact that ET will have on domains as broad and diverse as fundamental physics, cosmology, early Universe, astrophysics of compact objects, physics of matter in extreme conditions, and dynamics of stellar collapse. We discuss how the study of extreme astrophysical events will be enhanced by multi-messenger observations. We highlight the ET synergies with ground-based and space-borne GW observatories, including multi-band investigations of the same sources, improved parameter estimation, and complementary information on astrophysical or cosmological mechanisms obtained combining observations from different frequency bands. We present advancements in waveform modeling dedicated to third-generation observatories, along with open tools developed within the ET Collaboration for assessing the scientific potentials of different detector configurations. We finally discuss the data analysis challenges posed by third-generation observatories, which will enable access to large populations of sources and provide unprecedented precision.

Explore related subjects

Keep this discovery

BibTeXRIS

Adrian Abac, Raul Abramo, Simone Albanesi, Angelica Albertini, Alessandro Agapito, Michalis Agathos, Conrado Albertus, Nils Andersson, Tomas Andrade, Igor Andreoni, Federico Angeloni, Marco Antonelli, John Antoniadis, Fabio Antonini, Manuel Arca Sedda, M. Celeste Artale, Stefano Ascenzi, Pierre Auclair, Matteo Bachetti, Charles Badger, Biswajit Banerjee, David Barba-Gonzalez, Daniel Barta, Nicola Bartolo, Andreas Bauswein, Andrea Begnoni, Freija Beirnaert, Michal Bejger, Enis Belgacem, Nicola Bellomo, Laura Bernard, Maria Grazia Bernardini, Sebastiano Bernuzzi, Christopher P. L. Berry, Emanuele Berti, Gianfranco Bertone, Dario Bettoni, Miguel Bezares, Swetha Bhagwat, Sofia Bisero, Marie Anne Bizouard, Jose J. Blanco-Pillado, Simone Blasi, Alice Bonino, Alice Borghese, Ssohrab Borhanian, Elisa Bortolas, Maria Teresa Botticella, Marica Branchesi, Matteo Breschi, Richard Brito, Enzo Brocato, Floor S. Broekgaarden, Tomasz Bulik, Alessandra Buonanno, Fiorella Burgio, Adam Burrows, Gianluca Calcagni, Sofia Canevarolo, Enrico Cappellaro, Giulia Capurri, Carmelita Carbone, Roberto Casadio, Ramiro Cayuso, Pablo Cerda-Duran, Prasanta Char, Sylvain Chaty, Tommaso Chiarusi, Martyna Chruslinska, Francesco Cireddu, Philippa Cole, Alberto Colombo, Monica Colpi, Geoffrey Compere, Carlo Contaldi, Maxence Corman, Francesco Crescimbeni, Sergio Cristallo, Elena Cuoco, Giulia Cusin, Tito Dal Canton, Gergely Dalya, Paolo D'Avanzo, Nazanin Davari, Valerio De Luca, Viola De Renzis, Massimo Della Valle, Walter Del Pozzo, Federico De Santi, Alessio Ludovico De Santis, Tim Dietrich, Ema Dimastrogiovanni, Guillem Domenech, Daniela Doneva, Marco Drago, Ulyana Dupletsa, Hannah Duval, Irina Dvorkin, Nancy Elias-Rosa, Stephen Fairhurst. 2025-03-15. The Science of the Einstein Telescope. https://doi.org/10.1088/1475-7516/2026/03/081

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Electrovacuum Black Hole Uniqueness

We prove the black hole uniqueness conjecture in the axially symmetric, stationary, electrovacuum setting, subject to the refined asymptotic analysis of the associated singular harmonic maps, which includes an analyticity hypothesis at the axes. More precisely, it is shown that any asymptotically flat solution of the Einstein--Maxwell equations in this class, with more than one black hole horizon component is either: Majumdar--Papapetrou, up to a duality rotation, in which case all logarithmic angle defects vanish, or every finite axis rod logarithmic angle defect is strictly negative and hence every interaction force is strictly attractive. The proof extends the singular harmonic map method used for vacuum Kerr uniqueness in [18].

gr-qc

Constraining Modified Mass-to-Horizon Cosmology Through Primordial Inflationary Observables

We investigate slow-roll inflation in a modified cosmological framework inspired by a generalized mass-to-horizon relation (MHR), $M=\gamma {c^2 L^n}/{G}$, where $n$ is a real parameter and $\gamma$ a dimensional constant. Using Padmanabhan's emergence paradigm, we derive the modified Friedmann equations for a flat FRW universe and analyze the dynamics of a canonical scalar field (inflaton) under the slow-roll approximation. We study the resulting inflationary phenomenology for power-law and Starobinsky potentials. For power-law potentials, the MHR modification fails to reconcile these models with current CMB constraints on $r$ and $n_s$. In contrast, Starobinsky inflation exhibits significant sensitivity to deviations from $n=1$. A perturbative analysis ($n=1+\Delta$) yields corrections to inflationary observables. We observe that the scalar power-spectrum normalization, under a fixed-Starobinsky prescription, imposes the stringent constraint $0.960 \lesssim n \lesssim 1.040$ for $N=60$ efolds. This is considerably tighter than spectral-index bounds. Our results establish inflation, particularly Starobinsky-like models, as a sensitive probe of generalized horizon thermodynamics and departures from standard MHR scaling.

gr-qc

Improving the Sensitivity of Gravitational Wave Detection with Weighted Conformal Prediction

In the last decade, kilometre-scale interferometric gravitational-wave detectors have observed hundreds of compact binary mergers, the majority of which are binary black holes. However, the data are noise-dominated, and multiple independent search algorithms (pipelines) are used to enhance sensitivity and improve robustness. Rather than the standard approach of selecting the most significant pipeline output, we combine the outputs from all pipelines using a conformal prediction-based framework to provide statistically rigorous confidence estimates for candidate events. While combining pipelines improves sensitivity and ranking robustness, it requires a principled statistical framework that remains valid as data properties evolve across observing runs. A key challenge is distribution shifts between simulated datasets used for training and calibration and the real, unlabelled, observations used for testing, which can invalidate coverage guarantees and bias confidence estimates. In this work, we address this challenge by incorporating likelihood-ratio reweighting into our conformal prediction framework to account for covariate shift. Using mock datasets containing simulated signals, we demonstrate that weighted conformal prediction restores well-calibrated coverage under covariate shift and increases the confidence of events near the detection threshold, recovering true signals that would otherwise be missed.

gr-qc