0000000000264876
AUTHOR
Fabio D'antona
showing 9 related works from this author
Accretion and Magneto-Dipole Emission in Fast-Rotating Neutron Stars: New Spin-Equilibrium Lines
2005
Radio Ejection and Bump-related Orbital Period Gap of Millisecond Binary Pulsars
2006
UTILITA' DELL'ECOGRAFIA NELLA DIAGNOSI DI MALATTIA CELIACA
2004
Utilità dell’ecografia nella diagnosi di malattia celiaca
2004
Improved orbital parameters of accreting millisecond pulsar SAX J1808.4-3658
2006
To accrete or not to accrete: the dilemma of the recycling scenario
2004
We study the evolution of a low-mass X-ray binary by coupling a binary stellar evolution code with a general relativistic code that describes the behaviour of the neutron star. We find that non-conservative mass transfer scenarios are required to prevent the formation of submillisecond pulsars and/or the collapse to a black hole. We discuss the sweeping effects of an active magneto-dipole rotator on the transferred matter as a promising mechanism to obtain highly non-conservative evolutions.
Quale trattamento medico nell'esofago di Barrett
2004
Constraining the Equation of State of Neutron Stars with Genral Relativity
2005
When a radio pulsar breakes down by virtue of magnetodipole emission, its gravitational mass decreases accordingly. If the pulsar in hosted in a binary system, this mass loss will increase the orbital period of the system. We show that this relativistic effect can be indeed observable if the NS is fast and magnetized enough and that, if observed, it will help to put tight constraints on the equation of state of ultradense matter.