activity
20122024
most citedTurbulent magnetic field amplification in binary neutron star mergers

81 citations · 636 across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.GA2024★ 7 cited

Imaging fermionic dark matter cores at the center of galaxies

Joaquin Pelle, Carlos R. Argüelles, Florencia L. Vieyro +5

Current images of the supermassive black hole (SMBH) candidates at the center of our Galaxy and M87 have opened an unprecedented era for studying strong gravity and the nature of r…

astro-ph.HE2024

Delayed jet launching in binary neutron star mergers with realistic initial magnetic fields

Ricard Aguilera-Miret, Carlos Palenzuela, Federico Carrasco +2

We analyze a long-lived hyper-massive neutron star merger remnant (post-merger lifetime ms) that has been obtained via large eddy simulations with a gradient subgrid-scale m…

astro-ph.HE2023★ 4 cited

The role of turbulence and winding in the development of large-scale, strong magnetic fields in long-lived remnants of binary neutron star mergers

Ricard Aguilera-Miret, Carlos Palenzuela, Federico Carrasco +1

We perform a long and accurate Large-Eddy Simulation of a binary neutron star merger, following the newly formed remnant up to 110 milliseconds. The combination of high-order schem…

astro-ph.HE2022★ 12 cited

Relativistic force-free models of the thermal X-ray emission in millisecond pulsars observed by NICER

Federico Carrasco, Joaquin Pelle, Oscar Reula +2

Several important properties of rotation-powered millisecond pulsars (MSPs), such as their mass-radius ratio, equation of state and magnetic field topology, can be inferred from pr…

astro-ph.HE2022★ 13 cited

Skylight: a new code for general-relativistic ray-tracing and radiative transfer in arbitrary spacetimes

Joaquín Pelle, Oscar Reula, Federico Carrasco +1

To reproduce the observed spectra and light curves originated in the neighborhood of compact objects requires accurate relativistic ray-tracing codes. In this work, we present Skyl…

gr-qc2021★ 81 cited

Turbulent magnetic field amplification in binary neutron star mergers

C. Palenzuela, R. Aguilera-Miret, F. Carrasco +5

Magnetic fields are expected to play a key role in the dynamics and the ejection mechanisms that accompany the merger of two neutron stars. General relativistic magnetohydrodynamic…

astro-ph.HE2021

Gamma-radiation sky maps from compact binaries

Néstor Ortiz, Federico Carrasco, Stephen R. Green +3

We study sky maps and light curves of gamma-ray emission from neutron stars in compact binaries, and in isolation. We briefly review some gamma-ray emission models, and reproduce s…

astro-ph.HE2021★ 25 cited

Magnetospheres of black hole-neutron star binaries

Federico Carrasco, Masaru Shibata, Oscar Reula

We perform force-free simulations for a neutron star orbiting a black hole, aiming at clarifying the main magnetosphere properties of such binaries towards their innermost stable c…

gr-qc2020★ 57 cited

Turbulent magnetic-field amplification in the first 10 milliseconds after a binary neutron star merger: comparing high-resolution and large eddy simulations

Ricard Aguilera-Miret, Daniele Viganò, Federico Carrasco +2

The detection of binary neutron star mergers represents one of the most important and complex astrophysical discoveries of the recent years. One of the unclear aspects of the probl…

gr-qc2020★ 43 cited

GRMHD large eddy simulations with gradient subgrid-scale model

Daniele Viganò, Ricard Aguilera-Miret, Federico Carrasco +2

The detection of binary neutron star mergers represents one of the most important astrophysical discoveries of the recent years. Due to the extreme matter and gravity conditions an…

astro-ph.HE2020★ 32 cited

Magnetosphere of an orbiting neutron star

Federico Carrasco, Masaru Shibata

We conduct force-free simulations of a single neutron star undergoing orbital motion in flat spacetime, mimicking the trajectory of the star about the center of mass on a compact b…

astro-ph.HE2019★ 37 cited

Gradient sub-grid-scale model for relativistic MHD Large Eddy Simulations

Federico Carrasco, Daniele Viganò, Carlos Palenzuela

MHD turbulence is likely to play an important role in several astrophysical scenarios where the magnetic Reynolds is very large. Numerically, these cases can be studied efficiently…

astro-ph.HE2019★ 15 cited

Astrophysical jets from boosted compact objects

Ramiro Cayuso, Federico Carrasco, Barbara Sbarato +1

We perform full 3D numerical simulations of compact objects, such as black holes or neutron stars, boosted through an ambient force-free plasma that posses a uniform magnetization.…

astro-ph.HE2019★ 61 cited

Triggering magnetar outbursts in 3D force-free simulations

Federico Carrasco, Daniele Viganò, Carlos Palenzuela +1

In this letter, we present the first 3D force-free general relativity simulations of the magnetosphere dynamics related to the magnetar outburst/flare phenomenology. Starting from…

astro-ph.IM2018★ 31 cited

A Simflowny-based high-performance 3D code for the generalized induction equation

Daniele Viganò, David Martínez-Gómez, José A. Pons +6

In the interior of neutron stars, the induction equation regulates the long-term evolution of the magnetic fields by means of resistivity, Hall dynamics and ambipolar diffusion. De…

astro-ph.HE2018★ 26 cited

Pulsar magnetospheres in General Relativity

Federico Carrasco, Carlos Palenzuela, Oscar Reula

The main contribution to the pulsar power can be calculated by assuming a rotating magnetically-dominated magnetosphere described by the force-free approximation. Although this sim…

gr-qc2017★ 23 cited

A novel scheme for simulating the force-free equations: boundary conditions and the evolution of solutions towards stationarity

Federico Carrasco, Oscar Reula

Force-Free Electrodynamics (FFE) describes a particular regime of magnetically dominated relativistic plasmas, which arises on several astrophysical scenarios of interest such as p…

gr-qc2016★ 25 cited

Covariant Hyperbolization of Force-free Electrodynamics

Federico Carrasco, Oscar Reula

Force-Free Flectrodynamics (FFE) is a non-linear system of equations modeling the evolution of the electromagnetic field, in the presence of a magnetically dominated relativistic p…

gr-qc2015★ 31 cited

Nonlinear electrodynamics as a symmetric hyperbolic system

Fernando Abalos, Federico Carrasco, Érico Goulart +1

Nonlinear theories generalizing Maxwell's electromagnetism and arising from a Lagrangian formalism have dispersion relations in which propagation planes factor into null planes cor…

hep-th2013★ 43 cited

A Holographic Path to the Turbulent Side of Gravity

Stephen R. Green, Federico Carrasco, Luis Lehner

We study the dynamics of a 2+1 dimensional relativistic viscous conformal fluid in Minkowski spacetime. Such fluid solutions arise as duals, under the "gravity/fluid correspondence…

hep-th2013

Multi-solitons with vector mesons on the two-sphere

Federico Carrasco, Oscar Reula

Recent studies have suggested a strong connection between the static solutions of the 3D Skyrme model and those corresponding to its low-dimensional analog (baby-Skyrme model) on a…

hep-th2012★ 70 cited

Turbulent flows for relativistic conformal fluids in 2+1 dimensions

Federico Carrasco, Luis Lehner, Robert C. Myers +2

We demonstrate that relativistic conformal hydrodynamics in 2+1 dimensions displays a turbulent behaviour which cascades energy to longer wavelengths on both flat and spherical man…