Vogt-Russell theorem

The Vogt–Russell theorem states that the structure of a star, in hydrostatic and thermal equilibrium with all energy derived from nuclear reactions, is uniquely determined by its mass and the distribution of chemical elements throughout its interior.[1] Although referred to as a theorem, the Vogt–Russell theorem has never been formally proved. The theorem is named after astronomers Heinrich Vogt and Henry Norris Russell, who devised it independently.

References

  1. ↑ Carroll, Bradley W. & Ostlie, Dale A. (28 July 2006). An Introduction to Modern Astrophysics (Second ed.). Addison-Wesley. p. 333. ISBN 978-0805304022.


This article is issued from Wikipedia - version of the Thursday, December 31, 2015. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.