activity
20092026
most citedMagnetorotational instability in relativistic hypermassive neutron stars

171 citations · 1.1k across the 17 of their papers we have counts for

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Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2013★ 117 cited

On the universality of I-Love-Q relations in magnetized neutron stars

Brynmor Haskell, Riccardo Ciolfi, Francesco Pannarale +1

Recently, general relations among the quadrupole moment (Q), the moment of inertia (I), and the tidal deformability (Love number) of a neutron star were shown to exist. They are ne…

astro-ph.SR2013★ 157 cited

Twisted-torus configurations with large toroidal magnetic fields in relativistic stars

Riccardo Ciolfi, Luciano Rezzolla

Understanding the properties of the internal magnetic field of neutron stars remains a theoretical challenge. Over the last years, twisted-torus geometries have been considered bot…

astro-ph.SR2012★ 82 cited

Poloidal-Field Instability in Magnetized Relativistic Stars

Riccardo Ciolfi, Luciano Rezzolla

We investigate the instability of purely poloidal magnetic fields in nonrotating neutron stars by means of three-dimensional general-relativistic magnetohydrodynamics simulations,…

astro-ph.SR2010★ 24 cited

Structure, Deformations and Gravitational Wave Emission of Magnetars

L. Gualtieri, R. Ciolfi, V. Ferrari

Neutron stars can have, in some phases of their life, extremely strong magnetic fields, up to 10^15-10^16 G. These objects, named magnetars, could be powerful sources of gravitatio…

astro-ph.SR2010★ 142 cited

Structure and deformations of strongly magnetized neutron stars with twisted torus configurations

R. Ciolfi, V. Ferrari, L. Gualtieri

We construct general relativistic models of stationary, strongly magnetized neutron stars. The magnetic field configuration, obtained by solving the relativistic Grad-Shafranov equ…

astro-ph.SR2009★ 129 cited

Relativistic models of magnetars: the twisted-torus magnetic field configuration

R. Ciolfi, V. Ferrari, L. Gualtieri +1

We find general relativistic solutions of equilibrium magnetic field configurations in magnetars, extending previous results of Colaiuda et al. (2008). Our method is based on the s…