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Neutron Star

A neutron star is the collapsed core of a large star which before collapse had a total of between 10 and 29 solar masses. Neutron stars are the smallest and densest stars, not counting hypothetical quark stars and strange stars.[1] Typically, neutron stars have a radius on the order of 10 kilometres (6.2 mi) and a mass between 1.4 and 3 solar masses.[2] They result from the supernova explosion of a massive star, combined with gravitational collapse, that compresses the core past the white dwarf star density to that of atomic nuclei. 671 more words

Bose-Einstein Condensate

When atoms become extremely cold and reach absolute zero on the Kelvin scale they enter what’s referred to as a “Bose-Einstein Condensate” which is a state of matter that causes individual atoms to lose their individual properties thus leading them to mash together and act strangely in their behavioral properties. 41 more words

Physics