activity
20072026
most citedFirst M87 Event Horizon Telescope Results. III. Data Processing and Calibration

884 citations · 2.5k across the 34 of their papers we have counts for

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12 papers · 1 filter

gr-qc2026

Multi-messenger and multi-band signal from first-order phase transitions in proto-neutron stars

Christian Ecker, Mauro Giliberti, Luciano Rezzolla

A first-order phase transition (PT) alters a compact star on two scales: globally, via growth of a quark-matter core, and microscopically, via collision of quark bubbles, driving a…

gr-qc2026

Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures

Konrad Topolski, Samuel D. Tootle, Paramvir Singh +2

Compact binary systems consisting of a black hole (BH) and a neutron star (NS) are expected to provide detectable signals both in the gravitational wave and in the electromagnetic…

gr-qc2026

GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity

Carlo Musolino, Christian Ecker, Konrad Topolski +6

We present GRACE, a new GPU-accelerated numerical-relativity framework designed to run efficiently on heterogeneous high-performance computing platforms. Developed from scratch and…

gr-qc2026★ 1 cited

Dynamical response of twin stars to perturbations

Shamim Haque, Luciano Rezzolla, Ritam Mallick

If a strong first-order phase transition takes place at sufficiently high rest-mass densities in the equation of state (EOS) modelling compact stars, a new branch will appear in th…

gr-qc2026★ 1 cited

General gravitational properties of neutron stars: curvature invariants, binding energy, and trace anomaly

Iván Garibay, Christian Ecker, Luciano Rezzolla

We investigate the behavior of curvature invariants for a large ensemble of neutron stars built with equations of state (EOSs) that satisfy constraints from nuclear theory and pert…

gr-qc2025★ 8 cited

On the maximum compactness of neutron stars

Luciano Rezzolla, Christian Ecker

The stellar compactness, that is, the dimensionless ratio between the mass and radius of a compact star, , plays a fundamental role in characterising the gravit…

gr-qc2025★ 1 cited

Formation of gravastars

Daniel Jampolski, Luciano Rezzolla

Regular black holes and horizonless black hole mimickers offer mathematically consistent alternatives to address the challenges posed by standard black holes. However, the formatio…

gr-qc2025★ 60 cited

Towards a Non-singular Paradigm of Black Hole Physics

Raúl Carballo-Rubio, Francesco Di Filippo, Stefano Liberati +18

The study of regular black holes and black hole mimickers as alternatives to standard black holes has recently gained significant attention, driven both by the need to extend gener…

gr-qc2024

Black hole - neutron star binaries with high spins and large mass asymmetries: II. Properties of dynamical simulations

Konrad Topolski, Samuel Tootle, Luciano Rezzolla

Black hole (BH) - neutron star (NS) binary mergers are not only strong sources of gravitational waves (GWs), but they are also candidates for joint detections in the GW and electro…

gr-qc2024★ 1 cited

Black hole-neutron star binaries with high spins and large mass asymmetries: I. Properties of quasi-equilibrium sequences

Konrad Topolski, Samuel Tootle, Luciano Rezzolla

Black hole - neutron star (BHNS) mergers are a promising target of current gravitational-wave (GW) and electromagnetic (EM) searches, being the putative origin of ultra-relativisti…

gr-qc2024★ 9 cited

Can light-rings self-gravitate?

Francesco Di Filippo, Luciano Rezzolla

In a spherically symmetric and static spacetime of a compact object, such as that of a Schwarzschild black hole, the light-ring is a 2-sphere where photons experience the only poss…

gr-qc2007★ 332 cited

Phenomenological template family for black-hole coalescence waveforms

P. Ajith, S. Babak, Y. Chen +15

Recent progress in numerical relativity has enabled us to model the non-perturbative merger phase of the binary black-hole coalescence problem. Based on these results, we propose a…