Published October 1998
| Published
Journal Article
Open
Solar fusion cross sections
- Creators
- Adelberger, Eric G.
- Austin, Sam M.
- Bahcall, John N.
- Balantekin, A. B.
- Bogaert, Gilles
- Brown, Lowell S.
- Buchmann, Lothar
- Cecil, F. Edward
- Champagne, Arthur E.
- Braeckeleer, Ludwig de
- Duba, Charles A.
- Elliott, Steven R.
- Freedman, Stuart J.
- Gai, Moshe
- Goldring, G.
- Gould, Christopher R.
- Gruzinov, Andrei
- Haxton, Wick C.
- Heeger, Karsten M.
- Henley, Ernest
- Johnson, Calvin W.
-
Kamionkowski, Marc
- Kavanagh, Ralph W.
- Koonin, Steven E.
- Kubodera, Kuniharu
- Langanke, Karlheinz
- Motobayashi, Tohru
- Pandharipande, Vijay
- Parker, Peter
- Robertson, R. G. H.
- Rolfs, Claus
- Sawyer, R. F.
- Shaviv, N.
- Shoppa, T. D.
- Snover, K. A.
- Swanson, Erik
- Tribble, Robert E.
- Turck-Chièze, Sylvaine
- Wilkerson, John F.
Abstract
We review and analyze the available information on the nuclear-fusion cross sections that are most important for solar energy generation and solar neutrino production. We provide best values for the low-energy cross-section factors and, wherever possible, estimates of the uncertainties. We also describe the most important experiments and calculations that are required in order to improve our knowledge of solar fusion rates.
Additional Information
© 1998 The American Physical Society. This research was funded in part by the U.S. National Science Foundation and Department of Energy.Attached Files
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Additional details
- Eprint ID
- 3597
- Resolver ID
- CaltechAUTHORS:ADErmp98
- NSF
- Department of Energy (DOE)
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2006-06-22Created from EPrint's datestamp field
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2021-11-08Created from EPrint's last_modified field