13 citations · 14 across the 2 of their papers we have counts for
4 papers
Growth of magnetic fields in accreting millisecond pulsars
Carmine Cuofano, Alessandro Drago, Giuseppe Pagliara
R-modes can generate strong magnetic fields in the core of accreting millisecond neutron stars (NSs). The diffusion of these fields outside the core causes the growth of the extern…
Generation of strong magnetic fields by r-modes in millisecond accreting neutron stars: induced deformations and gravitational wave emission
Carmine Cuofano, Simone Dall'Osso, Alessandro Drago +1
Differential rotation induced by the r-mode instability can generate very strong toroidal fields in the core of accreting, millisecond spinning neutron stars. We introduce explicit…
Magnetic fields generated by r-modes in accreting millisecond pulsars
Carmine Cuofano, Alessandro Drago
In rotating neutron stars the existence of the Coriolis force allows the presence of the so-called Rossby oscillations (r-modes) which are know to be unstable to emission of gravit…
Magnetic fields generated by r-modes in accreting millisecond pulsars
Carmine Cuofano, Alessandro Drago
In millisecond pulsars the existence of the Coriolis force allows the development of the so-called Rossby oscillations (r-modes) which are know to be unstable to emission of gravit…