activity
20142026
most citedBlack holes, gravitational waves and fundamental physics: a roadmap

742 citations · 4.3k across the 89 of their papers we have counts for

collaborators

91 papers

astro-ph.CO2026

Scalar-Assisted Growth of Supermassive Black Holes: Boson-Mass Windows and Observational Constraints

Jorge Castelo Mourelle, Darío Núñez Zúñiga, Saeed Fakhry +1

We study a phenomenological cosmological model of black-hole growth in which a finite baryonic reservoir and a bosonic scalar cloud feed the black hole simultaneously. The baryonic…

astro-ph.CO2026

Dark-to-black super-accretion as a spin-imprinting mechanism for supermassive Kerr black holes

Saeed Fakhry, Nicolas Sanchis-Gual, Jorge Castelo Mourelle +2

The existence of supermassive black holes with masses and large dimensionless spins at high redshift remains a challenge to our understand…

gr-qc2026

Advanced Virgo during the LIGO-Virgo-KAGRA fourth observing run

Virgo Collaboration, F Acernese, A Agapito +546

From April 10, 2024 to November 18, 2025 Advanced Virgo participated in the fourth observing run of the network of gravitational-wave detectors, together with Advanced LIGO and KAG…

gr-qc2026

Rotating Fermion-Boson Stars in -squared Gravity

Saeed Fakhry, Jorge Castelo Mourelle, Nicolas Sanchis-Gual +3

Fermion-boson stars are compact equilibrium configurations composed of ordinary fermionic matter and a bosonic dark component interacting only through gravity. Such systems provide…

gr-qc2026

Intrinsic handedness in O1-O4a black-hole mergers: probing orbital precession, remnant retention in dense environments and cosmological mirror asymmetry

Juan Calderón Bustillo, Adrián del Rio, Nicolás Sanchis-Gual +1

Precessing binary black-holes generically produce an imbalance of right- and left- handed gravitational waves, reflecting the breaking of mirror symmetry by the merger dynamics. We…

gr-qc2026

Relativistic and Newtonian Proca Stars: A Tale of Two Limits

Alberto Diez-Tejedor, Carlos Herdeiro, Claudio Lazarte +4

We investigate a representative set of static solitonic solutions of the Einstein-Proca theory in the Newtonian regime, where the field frequency approaches the particle mass, $ω\t…

gr-qc2026

Constraint-satisfying binary boson star initial data via XCFC

Gabriele Palloni, Nicolas Sanchis-Gual, José A. Font +4

Numerical-relativity simulations with non-trivial matter configurations require initial data that satisfy the Hamiltonian and momentum constraints of the Einstein equations. We con…

gr-qc2026

Multipolar Proca stars: electric, magnetic and hybrid solitons

Carlos Herdeiro, Eugen Radu, Etevaldo dos Santos Costa Filho +1

We construct new families of everywhere regular, asymptotically flat solitons in the Einstein--Proca model, obtained as self-gravitating continuations of flat-spacetime (singular)…

astro-ph.IM2026

Advanced Virgo Plus for O5 -- Design Report Overview

F. Acernese, A. Agapito, D. Agarwal +578

This document presents an overview of the design, implementation, and expected performance of the Advanced Virgo Plus (AdV+) upgrades in view of the O5 observing run. Following the…

gr-qc2026

Gravitational confinement of ghost scalar fields in neutron stars

Argelia Bernal, Víctor Jaramillo, Néstor A. Montiel-Hernández +2

We investigate the effects, stability, and nonlinear dynamics of ghost scalar matter modeled as a field with a negative kinetic term confined within the cores of neutron stars. To…

gr-qc2025

Gravitational synchronization in bosonic dark matter admixed neutron stars

Claudio Lazarte, Nicolas Sanchis-Gual, José A. Font

While the search for dark matter remains a central focus of modern astrophysics and high-energy physics, neutron stars could provide natural laboratories in which the interaction b…

gr-qc2025

Improving the inference of the stellar quantities using the extended -Love-- relations

Eneko Aranguren, José A. Font, Nicolas Sanchis-Gual +1

In relativistic Astrophysics the -Love- relations refer to approximately EoS-independent relations involving the moment of inertia, Love number, and quadrupole moment through…

astro-ph.HE2025

Testing bosonic dark matter through white dwarf mass measurements

Jorge Castelo Mourelle, Nicolas Sanchis-Gual, José A. Font +1

Mass estimates of white dwarfs via electromagnetic methods, often differ from those obtained through gravitational redshift measurements, in some cases with discrepancies ranging i…

astro-ph.CO2025

Dark-to-black super accretion as a mechanism for early supermassive black hole growth

Nicolas Sanchis-Gual, Juan Barranco, Juan Carlos Degollado +1

The discovery of supermassive black holes with masses at redshifts challenges conventional formation scenarios based on baryonic accretion and…

gr-qc2025

Non-linear stability analysis of -Proca stars

Claudio Lazarte, Nicolas Sanchis-Gual, José A. Font +1

Vector boson stars, also known as Proca stars, exhibit remarkable dynamical robustness, making them strong candidates for potential astrophysical exotic compact objects. In search…

gr-qc2025

Reducing the irreducible: the charged black hole bomb in a moving cavity

Nicolas Sanchis-Gual, Alejandro Belchí, Carlos Herdeiro +1

We revisit the charged black hole bomb by numerically solving the fully non-linear Einstein-Maxwell-(charged, complex) Klein-Gordon system with a moving mirror. By dynamically vary…

gr-qc2025★ 4 cited

Stability and collisions of excited spherical boson stars: glimpses of chains and rings

Marco Brito, Carlos Herdeiro, Eugen Radu +2

Scalar, spherically symmetric, radially excited boson stars were previously shown to be stabilized, against spherical dynamics, by sufficiently strong self-interactions. Here, we f…

gr-qc2025

Cosmological mirror symmetry and gravitational-wave helicity

Juan Calderón-Bustillo, Adrian del Rio, Samson H. W. Leong +1

Our current understanding of the Universe relies on the hypothesis that, when observed at sufficiently large scales, it looks statistically identical regardless of location or dire…

astro-ph.GA2025

Reproducing galactic rotation curves with a two-component bosonic dark matter model

Jorge Castelo Mourelle, Nicolas Sanchis-Gual, José A. Font

Bosonic stars,hypothetical astrophysical entities, are generally categorized into two primary classes based on the nature of their constituent particles: Einstein Klein Gordon star…

gr-qc2025★ 4 cited

Eccentric mergers of binary Proca stars

Gabriele Palloni, Nicolas Sanchis-Gual, José A. Font +2

We present a numerical relativity study of eccentric mergers of equal-mass rotating Proca stars, focusing on their gravitational-wave (GW) emission. By systematically va…

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★ 3 cited

Gravitational-wave signatures of mirror (a)symmetry in binary black hole mergers: measurability and correlation to gravitational-wave recoil

Samson H. W. Leong, Alejandro Florido Tomé, Juan Calderón Bustillo +2

Precessing binary black-hole mergers can produce a net flux of circularly-polarized gravitational waves. This imbalance between left- and right-handed circularly polarized waves, q…

gr-qc2024

-Love-, and too: The role of the mass in universal relations of compact stars

Eneko Aranguren, José A. Font, Nicolas Sanchis-Gual +1

In the study of rotating neutron stars the -Love- relations refer to the existence of various approximate, equation of state-independent relations involving the moment of ine…

gr-qc2024

Exotic compact objects: a recent numerical-relativity perspective

Miguel Bezares, Nicolas Sanchis-Gual

Beyond black holes and neutron stars, new hypothetical compact objects have been proposed as potential astrophysical entities. In general, their properties have not yet been fully…