activity
20112026
most citedThe Science of the Einstein Telescope

97 citations · 568 across the 26 of their papers we have counts for

collaborators

26 papers

gr-qc2026

Breakdown of Hydrodynamic Universality in Neutron Star Oscillations

Gabriel S. Denicol, Amanda Guerrieri, João V. M. Muniz +2

Hydrodynamic universality refers to the property that different formulations of relativistic dissipative hydrodynamics yield identical predictions in the asymptotic long-wavelength…

gr-qc2026

Radial Oscillations of Viscous Stars at Finite Temperature

Amanda Guerrieri, Gabriel S. Rocha, Gabriel S. Denicol +1

We study the radial oscillation spectrum of relativistic stars within Israel-Stewart and Navier-Stokes theories, extending previous analyses to include heat diffusion and a thermod…

gr-qc2026

Inspirals into bosonic dark matter stars and chirp mimickers

Caio F. B. Macedo, Haroldo C. D. Lima, Raissa F. P. Mendes +2

We investigate extreme--mass--ratio inspirals in which a stellar-mass compact object orbits a supermassive bosonic dark matter star, modeled as a boson star, using fully relativist…

gr-qc2025★ 3 cited

Radial Oscillations of Viscous Neutron Stars: Zero Diffusion Case

Raissa F. P. Mendes, Amanda Guerrieri, João V. M. Muniz +2

The spectrum of radial oscillations of neutron stars is systematically studied within two frameworks of viscous relativistic hydrodynamics: the relativistic Navier-Stokes and Israe…

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★ 7 cited

On the phase transition mechanism of spontaneous scalarization

João Vitor M. Muniz, Néstor Ortiz, Raissa F. P. Mendes

In certain modified gravity theories that include additional scalar degrees of freedom, compact objects such as black holes and neutron stars may undergo a process known as spontan…

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

Neutron stars in the symmetron model

Bernardo F. de Aguiar, Raissa F. P. Mendes, F. T. Falciano

Screening mechanisms are often deployed by dark energy models in order to conceal the effects of their new degrees of freedom from the scrutiny of terrestrial and solar system expe…

gr-qc2021★ 24 cited

Equation-of-state-insensitive measure of neutron star stiffness

Jayana A. Saes, Raissa F. P. Mendes

Universal relations (i.e., insensitive to the equation of state) between macroscopic properties of neutron stars have proven useful for a variety of applications -- from providing…

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★ 17 cited

Highly compact neutron stars and screening mechanisms. I. Equilibrium and stability

Bernardo F. de Aguiar, Raissa F. P. Mendes

Modified theories of gravity that offer viable models for dark energy often rely on mechanisms that screen their effects in high density environments. From this perspective, it wou…

gr-qc2019★ 10 cited

Scalar charges and pulsar-timing observables in the presence of nonminimally coupled scalar fields

Raissa F. P. Mendes, Tulio Ottoni

Pulsar-timing has become a celebrated tool for probing modifications to General Relativity in the strong-field surroundings of neutron stars. Here we investigate whether scalar-ten…

gr-qc2018★ 32 cited

Trace of the energy-momentum tensor and macroscopic properties of neutron stars

Dylan M. Podkowka, Raissa F. P. Mendes, Eric Poisson

A generic feature of scalar extensions of general relativity is the coupling of the scalar degrees of freedom to the trace of the energy-momentum tensor of matter fields. Inter…

gr-qc2018★ 45 cited

Evolution of Highly Eccentric Binary Neutron Stars Including Tidal Effects

Huan Yang, William E. East, Vasileios Paschalidis +2

This work is the first in a series of studies aimed at understanding the dynamics of highly eccentric binary neutron stars, and constructing an appropriate gravitational-waveform m…

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

Swimming in spacetime: the view from a Fermi observer

Raissa F. P. Mendes, Eric Poisson

An extended test body moving in a curved spacetime does not typically follow a geodesic, because of forces that arise from couplings between its multipole moments and the ambient c…

astro-ph.CO2016★ 47 cited

Tidal deformability of boson stars and dark matter clumps

Raissa F. P. Mendes, Huan Yang

In this work we consider minimally-coupled boson stars immersed in a tidal environment and compute their tidal deformability to leading order. We also describe an approximate corre…

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★ 2 cited

Instability of nonminimally coupled scalar fields in the spacetime of thin charged shells

Jessica Santiago, Andre G. S. Landulfo, William C. C. Lima +3

We investigate the stability of a free scalar field nonminimally coupled to gravity under linear perturbations in the spacetime of a charged spherical shell. Our analysis is perfor…

gr-qc2015★ 2 cited

Self-force and fluid resonances

Soichiro Isoyama, Raissa F. P. Mendes, Eric Poisson

The gravitational self-force acting on a particle orbiting a massive central body has thus far been computed for vacuum spacetimes involving a black hole. In this work we continue…

gr-qc2014★ 55 cited

On the possibility of setting a new constraint to scalar-tensor theories

Raissa F. P. Mendes

Scalar-tensor theories (STTs) are a widely studied alternative to General Relativity (GR) in which gravity is endowed with an additional scalar degree of freedom. Although severely…

gr-qc2014★ 21 cited

Instability of nonminimally coupled scalar fields in the spacetime of slowly rotating compact objects

Raissa F. P. Mendes, George E. A. Matsas, Daniel A. T. Vanzella

Nonminimally coupled free scalar fields may be unstable in the spacetime of compact objects. Such instability can be triggered by classical seeds or, more simply, by quantum fluctu…

gr-qc2013★ 1 cited

Reply to "Comment on `Quantum versus classical instability of scalar fields in curved backgrounds'"

George E. A. Matsas, Raissa F. P. Mendes, Daniel A. T. Vanzella

We show that the reasoning which led the author of arXiv:1310.6252 to reach his conclusions relies on an incorrect criterion for the existence of normalizable bound solutions. We r…

gr-qc2013★ 19 cited

Quantum versus classical instability of scalar fields in curved backgrounds

Raissa F. P. Mendes, George E. A. Matsas, Daniel A. T. Vanzella

General-relativistic stable spacetimes can be made unstable under the presence of certain nonminimally coupled free scalar fields. In this paper, we analyze the evolution of linear…