| Issue |
A&A
Volume 383, Number 1, FebruaryIII 2002
|
|
|---|---|---|
| Page(s) | 291 - 295 | |
| Section | Planets and planetary systems | |
| DOI | https://doi.org/10.1051/0004-6361:20011715 | |
| Published online | 15 February 2002 | |
The Salpeter plasma correction for solar fusion reactions
1
Institute for Advanced Study, Princeton, NJ 08540, USA e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
2
Department of Physics, University of Washington, Seattle, Washington 98195, USA e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
3
Institute for Advanced Study, Princeton, NJ 08540, USA e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
4
Department of Physics, University of California at Santa, Barbara, Santa Barbara, CA 93106, USA e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
Corresponding author: R. F. Sawyer, This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
1
August
2001
Accepted:
3
December
2001
Abstract
We describe five different ways of obtaining the Salpeter formula for the plasma corrections to fusion rates; this formula is valid at the center of the sun with insignificant errors (~percent). Several recent papers have obtained a variety of answers in conflict with this result. We analyse the arguments of these papers, identifying sources of the discrepancies in some cases, and pointing out internal inconsistencies in the arguments given in other cases.
Key words: nuclear reactions / plasmas / sun: interior
© ESO, 2002
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.