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| 4. This is a simplified version of the relativistic calculation that we performed for a white dwarf. Here we immediately take the electrons to be highly relativistic. As before, assume that the inward gravitational pressure | |||
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Summary: 4. This is a simplified version of the relativistic calculation that we performed for a white dwarf. Here we |
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Source: Allen, Roland E. - Department of Physics and Astronomy, Texas A&M University |
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Collections: Physics |
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