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Equation of state of hot, dense stellar matter

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Date

1981

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Abstract

The properties of hot, dense stellar matter are investigated with a finite temperature nuclear Thomas-Fermi model. NUCLEAR STRUCTURE Hot stellar matter, equation of state, finite temperature nuclear Thomas-Fermi model.

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Citation

URI

https://dspace-test.anu.edu.au/handle/1885/733741076

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DevOps Pure Testing

Source

Physical Review C - Nuclear Physics

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Article

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License Rights

DOI

10.1103/PhysRevC.24.1191

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