Three approaches for the classification of protoneutron star oscillation modes
Sign Up to like & getrecommendations! Published in 2023 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stad1459
Abstract: The future detection of gravitational waves (GWs) from a galactic core-collapse supernova will provide information on the physics inside protoneutron stars (PNS). In this work, we apply three different classification methods for the PNS non-radial… read more here.
Keywords: approaches classification; protoneutron; three approaches; classification ... See more keywords
Magnetar formation through a convective dynamo in protoneutron stars
Sign Up to like & getrecommendations! Published in 2020 at "Science Advances"
DOI: 10.1126/sciadv.aay2732
Abstract: Strong field dynamos can explain magnetar formation consistently with the millisecond magnetar model for extreme explosions. The release of spin-down energy by a magnetar is a promising scenario to power several classes of extreme explosive… read more here.
Keywords: magnetar formation; protoneutron; formation convective; formation ... See more keywords