activity
20122024
most citedPopulation synthesis of isolated Neutron Stars with magneto--rotational evolution

103 citations · 409 across the 13 of their papers we have counts for

collaborators

14 papers

astro-ph.HE20252 cited

Impact of magnetic field gradients on the development of the MRI: Applications to binary neutron star mergers and proto-planetary disks

T. Celora, C. Palenzuela, D. Viganò +1

The magneto-rotational instability (MRI) is widely believed to play a central role in generating large-scale, poloidal magnetic fields during binary neutron star mergers. However,…

astro-ph.HE20241 cited

Constraints on the dense matter equation of state from young and cold isolated neutron stars

Alessio Marino, Clara Dehman, Konstantinos Kovlakas +3

Neutron stars are the dense and highly magnetic relics of supernova explosions of massive stars. The quest to constrain the Equation of State (EoS) of ultra-dense matter and thereb…

astro-ph.EP202329 cited

The CARMENES search for exoplanets around M dwarfs. A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data

J. Blanco-Pozo, M. Perger, M. Damasso +37

Detecting a planetary companion in a short-period orbit through radio emission from the interaction with its host star is a new prospect in exoplanet science. Recently, a tantalisi…

astro-ph.HE202210 cited

Synchro-curvature emitting regions in high-energy pulsar models

Daniel Íñiguez-Pascual, Daniele Viganò, Diego F. Torres

The detected high-energy pulsars' population is growing in number, and thus, having agile and physically relevant codes to analyze it consistently is important. Here, we update our…

astro-ph.HE201439 cited

Compact formulae, dynamics and radiation of charged particles under synchro-curvature losses

Daniele Viganò, Diego F. Torres, Kouichi Hirotani +1

We consider the fundamental problem of charged particles moving along and around a curved magnetic field line, revising the synchro-curvature radiation formulae introduced by Cheng…

astro-ph.HE201425 cited

An assessment of the pulsar outer gap model. I: Assumptions, uncertainties, and implications for the gap size and the accelerating field

Daniele Viganò, Diego F. Torres, Kouichi Hirotani +1

The popular outer gap model of magnetospheric emission from pulsars has been widely applied to explain the properties observed in -rays. However, its quantitative predictions re…