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20112023
most citedAccretion-induced prompt black hole formation in asymmetric neutron star mergers, dynamical ejecta and kilonova signals

122 citations · 874 across the 24 of their papers we have counts for

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19 papers · 1 filter

gr-qc2023

Analytically improved and numerical-relativity informed effective-one-body model for coalescing binary neutron stars

Rossella Gamba, Matteo Breschi, Sebastiano Bernuzzi +9

Gravitational wave astronomy pipelines rely on template waveform models for searches and parameter estimation purposes. For coalescing binary neutron stars (BNS), such models need…

gr-qc2022★ 18 cited

Effective-action model for dynamical scalarization beyond the adiabatic approximation

Mohammed Khalil, Raissa F. P. Mendes, Néstor Ortiz +1

In certain scalar-field extensions to general relativity, scalar charges can develop on compact objects in an inspiraling binary -- an effect known as dynamical scalarization. This…

gr-qc2021★ 14 cited

Nonlinear dynamics of oscillating neutron stars in scalar-tensor gravity

Raissa F. P. Mendes, Néstor Ortiz, Nikolaos Stergioulas

The spectrum of oscillating compact objects can be considerably altered in alternative theories of gravity. In particular, it may be enriched by modes with no counterpart in genera…

gr-qc2020★ 50 cited

Nonlinear curvature effects in gravitational waves from inspiralling black hole binaries

Banafsheh Shiralilou, Tanja Hinderer, Samaya Nissanke +2

Gravitational waves (GWs) from merging black holes allow for unprecedented probes of strong-field gravity. Testing gravity in this regime requires accurate predictions of gravitati…

gr-qc2018★ 94 cited

Effective-one-body multipolar waveform for tidally interacting binary neutron stars up to merger

Sarp Akcay, Sebastiano Bernuzzi, Francesco Messina +3

Gravitational-wave astronomy with coalescing binary neutron star sources requires the availability of gravitational waveforms with tidal effects accurate up to merger. This article…

gr-qc2018★ 55 cited

New class of quasinormal modes of neutron stars in scalar-tensor gravity

Raissa F. P. Mendes, Néstor Ortiz

Detection of the characteristic spectrum of pulsating neutron stars can be a powerful tool not only to probe the nuclear equation of state, but also to test modifications to genera…

gr-qc2017★ 27 cited

Extended I-Love relations for slowly rotating neutron stars

Jérémie Gagnon-Bischoff, Stephen R. Green, Philippe Landry +1

Observations of gravitational waves from inspiralling neutron star binaries---such as GW170817---can be used to constrain the nuclear equation of state by placing bounds on stellar…

gr-qc2017★ 84 cited

Fixing extensions to General Relativity in the non-linear regime

Juan Cayuso, Néstor Ortiz, Luis Lehner

The question of what gravitational theory could supersede General Relativity has been central in theoretical physics for decades. Many disparate alternatives have been proposed mot…

gr-qc2017★ 1 cited

Cauchy horizon stability in a collapsing spherical dust cloud. II: Energy bounds for test fields and odd-parity gravitational perturbations

Néstor Ortiz, Olivier Sarbach

We analyze the stability of the Cauchy horizon associated with a globally naked, shell-focussing singularity arising from the complete gravitational collapse of a spherical dust cl…

gr-qc2016★ 83 cited

Highly compact neutron stars in scalar-tensor theories of gravity: Spontaneous scalarization versus gravitational collapse

Raissa F. P. Mendes, Néstor Ortiz

Scalar-tensor theories of gravity are extensions of General Relativity (GR) including an extra, nonminimally coupled scalar degree of freedom. A wide class of these theories, albei…

gr-qc2015★ 46 cited

Shadow of a naked singularity

Néstor Ortiz, Olivier Sarbach, Thomas Zannias

We analyze the redshift suffered by photons originating from an external source, traversing a collapsing dust cloud and finally being received by an asymptotic observer. In additio…

gr-qc2015★ 1 cited

On the behaviour of non-radial null geodesics in self-similar Tolman-Bondi collapse

Néstor Ortiz, Olivier Sarbach, Thomas Zannias

Motivated by recent work on the structure of the singularity in inhomogeneous Tolman-Bondi collapse models, we investigate the behaviour of null geodesics in the particular case wh…

gr-qc2014★ 17 cited

Observational distinction between black holes and naked singularities: the role of the redshift function

Néstor Ortiz, Olivier Sarbach, Thomas Zannias

We suggest that the redshift of photons traveling from past to future null infinity through a collapsing object could provide an observational signature capable of differentiating…

gr-qc2013★ 11 cited

The gravitational redshift of photons traversing a collapsing dust cloud and observable consequences

Néstor Ortiz, Olivier Sarbach

We analyze the frequency shift of photons propagating on an asymptotically flat spacetime describing a collapsing, spherical dust cloud. We focus on the case where the interaction…

gr-qc2013★ 4 cited

Cauchy horizon stability in a collapsing spherical dust cloud I: geometric optic approximation and spherically symmetric test fields

Néstor Ortiz, Olivier Sarbach

A spherical dust cloud which is initially at rest and which has a monotonously decaying density profile collapses and forms a shell-focussing singularity. Provided the density prof…

gr-qc2012★ 28 cited

Linear perturbations of self-gravitating spherically symmetric configurations

Eliana Chaverra, Néstor Ortiz, Olivier Sarbach

We present a new covariant, gauge-invariant formalism describing linear metric perturbation fields on any spherically symmetric background in general relativity. The advantage of t…

gr-qc2012★ 2 cited

Conformal diagrams for the gravitational collapse of a spherically symmetric dust cloud

Néstor Ortiz, Olivier Sarbach

We present an algorithm for the construction of conformal coordinates in the interior of a spherically symmetric, collapsing matter cloud in general relativity. This algorithm is b…

gr-qc2012★ 4 cited

Initial data giving rise to naked singularities in spherically symmetric dust collapse

Néstor Ortiz

The phase space corresponding to a particular four-parameter family of initial data for the gravitational collapse of a spherically symmetric dust cloud is investigated. In a certa…

gr-qc2011★ 20 cited

Conformal diagrams for the gravitational collapse of a spherical dust cloud

Néstor Ortiz, Olivier Sarbach

We present an algorithm for the construction of conformal coordinates in the interior of a spherically symmetric, collapsing matter cloud in general relativity. This algorithm is b…