Spin polarization phenomena in dense nuclear matter Alexander Isayev Kharkov Institute of Physics and Technology Ukraine.
Neutron Stars 3: Thermal evolution Andreas Reisenegger Depto. de Astronomía y Astrofísica Pontificia Universidad Católica de Chile.
Neutron Stars 3: Thermal evolution Andreas Reisenegger ESO Visiting Scientist Associate Professor, Pontificia Universidad Católica de Chile.
COOLING OF N EUTRON ST A R S
COOLING OF NEUTRON STARS D.G. Yakovlev Ioffe Physical Technical Institute, St.-Petersburg, Russia Ladek Zdroj, February 2008, 1. Formulation of the Cooling.
Spin polarization phenomena in dense nuclear matter
Neutron Stars 3: Thermal evolution
