activity
20182022
most citedVirgo Detector Characterization and Data Quality: results from the O3 run

60 citations · 178 across the 12 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2021

Detectability of continuous gravitational waves from magnetically deformed neutron stars

J. Soldateschi, N. Bucciantini

Extremely powerful magnetic fields are contained inside neutron stars. Their effect is to deform the shape of the star, leading to the emission of continuous gravitational waves. T…

astro-ph.HE2021★ 19 cited

Quasi-universality of the magnetic deformation of neutron stars in general relativity and beyond

J. Soldateschi, N. Bucciantini, L. Del Zanna

Neutron stars are known to host extremely powerful magnetic fields. Among other effects, one of the consequences of harbouring such fields is the deformation of the neutron star st…

astro-ph.HE2021

Axisymmetric equilibrium models of magnetised neutron stars in scalar-tensor theories

Jacopo Soldateschi, Niccolò Bucciantini, Luca Del Zanna

General relativity probably is not the definitive theory of gravity, due a number or issues, both from the theoretical and from the observational point of view. Alternative theorie…

astro-ph.HE2020★ 12 cited

Magnetic deformation of neutron stars in scalar-tensor theories

J. Soldateschi, N. Bucciantini, L. Del Zanna

Scalar-tensor theories are among the most promising alternatives to general relativity that have been developed to account for some long standing issues in our understanding of gra…

astro-ph.HE2020★ 15 cited

Axisymmetric equilibrium models for magnetised neutron stars in Scalar-Tensor Theories

J. Soldateschi, N. Bucciantini, L. Del Zanna

Among the possible extensions of General Relativity that have been put forward in order to address some long standing issues in our understanding of the Universe, Scalar-Tensor The…

astro-ph.HE2020★ 8 cited

Iron Line from Neutron Star Accretion Disks in Scalar Tensor Theories

N. Bucciantini, J. Soldateschi

The Fe K_αfluorescent line at 6.4 keV is a powerful probe of the space-time metric in the vicinity of accreting compact objects. We investigated here how some alternative theories…