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Neutron degeneracy - PowerPoint PPT Presentation

Problem Set 5

Problem Set 5.

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Stars and their Physical Properties

Stars and their Physical Properties. Background Information. Name: Isabel Baransky School: Fu Foundation of Engineering and Applied Science Major: Applied Physics Minor: Music. OVERVIEW OF FORCE. THE BIG BANG. Big Bang. Occurred 13.7 billion years ago.

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Lecture 21

Lecture 21. Neutron stars. Neutron stars. If a degenerate core (or white dwarf) exceeds the Chandrasekhar mass limit (1.4M Sun ) it must collapse until neutron degeneracy pressure takes over. Neutron stars. The force of gravity at the surface is very strong:.

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14.9 SUPERDENSE MATTER

14.9 SUPERDENSE MATTER.

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ASTRONOMY

ASTRONOMY. Chapter 31 Black Holes. Relativity. Einstein published his General Theory of Relativity in 1916 His Special Theory of Relativity, published in 1905, predicted that the speed of light did not change for any observer despite their motion.

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Neutron degeneracy - PowerPoint PPT Presentation

Problem Set 5

Stars and their Physical Properties

Lecture 21

14.9 SUPERDENSE MATTER

ASTRONOMY