Abstract
The classical electrostatic screening is revisited. We find major revisions already in the weak screening limit. Here we discuss the classical expression for the screening and show that the picture used to derive the screening is wrong. When corrected, all the screening factors are multiplied by a factor of 3/2 in the exponent.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Clayton, D.D., 1968, Stellar Structure and Evolution, Academic Press.
Graboske, H.C., De Witt, H.E., Grossman, A.S., Cooper, M.S., 1973, ApJ, 181, 457
Salpeter, E.E., 1954, Australian J. of Physics, 7, 373
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1997 Springer Science+Business Media Dordrecht
About this paper
Cite this paper
Shaviv, N.J., Shaviv, G. (1997). The Electrostatic Screening of Thermonuclear Reactions in Astrophysical Plasmas. In: Isern, J., Hernanz, M., GarcÃa-Berro, E. (eds) White Dwarfs. Astrophysics and Space Science Library, vol 214. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5542-7_6
Download citation
DOI: https://doi.org/10.1007/978-94-011-5542-7_6
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6334-0
Online ISBN: 978-94-011-5542-7
eBook Packages: Springer Book Archive