Go back to Previous Lecture   Go to Next Lecture
Lecture 13: 4/1—Supernova Explosions, General Properties of Neutron Stars

Some possibly helpful links for this lecture:

Cool Simulations of Black Holes and Neutron Stars
More on Black Holes and Neutron Stars
Click on an image to enlarge it.

What happens to the Fe core when it contracts?

White dwarf -- mostly composed of degenerate electron gas and Fe nuclei

When density gets to 10E11 g/cm3, nuclei dissolve creating relativistic electron gas
General Properties of Neutron Stars

Most of neutron star is a superfluid composed of neutrons, protons and electrons with near-zero viscosity and is superconducting


Escape velocity is about one-third the speed of light ... star will accrete matter from gas or binary companion and some kinetic energy goes into radiation: X-Rays.
   

Return to lecture gallery