Speaker
Dr
Michał Bejger
(N. Copernicus Astronomical Center, PAS)
Description
Using a recent equation of state (Benic et al., 2015, A&A 577, A40) I will discuss
the stability of rotating neutron stars with strong phase
transitions (so-called twin family of neutron stars). The existence of an instability
region separating the twin families - a direct outcome of the strong phase transition
- creates several astrophysical implications that are interesting from the point
of view of observational and microphysical aspects of the equation of state.
Primary author
Dr
Michał Bejger
(N. Copernicus Astronomical Center, PAS)
