443 citations · 2.3k across the 68 of their papers we have counts for
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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…
3D evolution of neutron star magnetic-fields from a realistic core-collapse turbulent topology
Clara Dehman, Daniele Viganò, Stefano Ascenzi +2
We present the first 3D fully coupled magneto-thermal simulations of neutron stars (including the most realistic background structure and microphysical ingredients so far) applied…
Vorticity and magnetic dynamo from subsonic expansion waves
Albert Elias-López, Fabio Del Sordo, Daniele Viganò
This work concentrates on the effect of an irrotational forcing on a magnetized flow in the presence of rotation, baroclinicity, shear, or a combination of them. By including magne…
Magnetic winding and turbulence in ultra-hot Jupiters
Clàudia Soriano-Guerrero, Daniele Viganò, Rosalba Perna +2
While magnetism in exoplanets remains largely unknown, Hot Jupiters have been considered as natural candidates to harbour intense magnetic fields, both due to their large masses an…
How bright can old magnetars be? Assessing the impact of magnetized envelopes and field topology on neutron star cooling
Clara Dehman, José A. Pons, Daniele Viganò +1
Neutron stars cool down during their lifetime through the combination of neutrino emission from the interior and photon cooling from the surface. Strongly magnetised neutron stars,…