Speaker
Sergey kolevatov
(SPbSU)
Description
There is no precise theory describing the structure of neutron stars. However, inside such objects the baryon density is very high and a pion condensation may occur. This condensate, if it exist, might give a significant effect on a spectrum of neutron stars. We investigate this influence with a help of simplified model to give qualitative picture of the effect.
Author
Sergey kolevatov
(SPbSU)
Co-author
Prof.
Alexander Andrianov
(Saint Petersburg State University)
