Speaker
Hovik Grigorian
(JINR)
Description
The influence of environmental effects and proton superconductivity in the matter of neutron stars on the evolution of stellar cooling is studied. It is shown that using cooling models and observational data on the temperature and age of pulsars, it is possible to extract the masses of the observed objects and the mass spectrum of neutron stars.
Author
Hovik Grigorian
(JINR)
