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Mitigation and control of instabilities in DAFNE positron ring
Alessandro Drago, David Alesini, Theo Demma +5
The positron beam in the DAFNE e+/e- collider has always been suffering from strong e-cloud instabilities. In order to cope with them, several approaches have been adopted along th…
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…
The baryon number two system in the Chiral Soliton Model
Valentina Mantovani Sarti, Alessandro Drago, Vicente Vento +1
We study the interaction between two B = 1 states in a Chiral Soliton Model where baryons are described as non-topological solitons. By using the hedgehog solution for the B = 1 st…