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Future Evolution of Neutron Star Binaries by phamdinhhoa1235 is a document available to read on EtoBox.

This study models the future evolution of 21 Gaia neutron star-main sequence binaries, focusing on their transition to neutron star-white dwarf binaries. Different mass-transfer modes yield varying outcomes, with eccentric mass transfer leading to higher eccentricities and longer orbital periods, while circularized mass transfer results in fully recycled millisecond pulsars. The findings highlight the need for different initial conditions to match the observed Galactic millisecond pulsar-white dwarf populat

Author

phamdinhhoa1235

Language

EN