Abstract
Let L r = L r (r) be the function representing the net flow of integrated radiation (cf. [9], Chapter II, Section 2 and Chapter VII, Section 5) across a sphere (Σ r ) of radius r.
This is a preview of subscription content, log in via an institution to check access.
Preview
Unable to display preview. Download preview PDF.
Author information
Authors and Affiliations
Rights and permissions
Copyright information
© 1973 D. Reidel Publishing Company Dordrecht, Holland
About this chapter
Cite this chapter
Kourganoff, V. (1973). Energy Equilibrium and Nuclear Reactions. In: Introduction to the Physics of Stellar Interiors. Astrophysics and Space Science Library, vol 34. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2539-3_4
Download citation
DOI: https://doi.org/10.1007/978-94-010-2539-3_4
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-2541-6
Online ISBN: 978-94-010-2539-3
eBook Packages: Springer Book Archive