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With all reserve we advance the view that a supernova represents the transition of an ordinary star into a neutron star consisting mainly of neutrons. Such a star may possess a very small radius and an extremely high density. As neutrons can be packed much more closely than ordinary nuclei and electrons, the gravitational packing energy in a cold neutron star may become very large, and under certain conditions may far exceed the ordinary nuclear packing fractions.

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Chris Sharma

Climbing is an amazing, unique sport, and I want to share that with as many people as possible. I want to be an ambassador for the sport and raise the profile. I try to take advantage of any opportunity to share climbing with the world.

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