Slide 1Neutron Stars Slide 2 Gradual compression of a stellar iron core  trans. [g cm -3 ] CompositionDegen. pressure Remarks Iron nuclei; nonrel. free e - nonrel. e -…

Slide 1 Slide 2 Neutron Stars 3: Thermal evolution Andreas Reisenegger Depto. de Astronomía y Astrofísica Pontificia Universidad Católica de Chile Slide 3 Outline Cooling…

Slide 1 Constraining the symmetry energy of the EoS in relativistic heavy-ion reactions A. Krasznahorkay, ATOMKI, Debrecen Slide 2 2 neutrons protons Introduction The neutron-skin…

Neutron Stars 3: Thermal evolution Andreas Reisenegger ESO Visiting Scientist Associate Professor, Pontificia Universidad Católica de Chile Outline Cooling processes of…

Neutrino Cooling of Neutron Stars D.N. Voskresensky NRNU MEPhI, Moscow General information on NS “Standard” scenario. “Minimal” cooling. Neutrino reaction rates in…

Neutron Stars 3: Thermal evolution Andreas Reisenegger ESO Visiting Scientist Associate Professor, Pontificia Universidad Católica de Chile Outline Cooling processes of…

Dynamic stability of compact stars. Properties of the neutron star crust. G.S.Bisnovatyi-Kogan Space Research Institute RAN, Moscow Joint Institute of Nuclear Researches,…

Stability of compact stars (white dwarfs and neutron stars) . G.S.Bisnovatyi-Kogan Space Research Institute RAN, Moscow Joint Institute of Nuclear Researches, Dubna 1. History…

Dynamic stability of compact stars. Properties of the neutron star crust. G.S.Bisnovatyi-Kogan Space Research Institute RAN, Moscow Joint Institute of Nuclear Researches,…