Published October 1998
| Version Published
Journal Article
Open
Solar fusion cross sections
Creators
- Adelberger, Eric G.1
- Austin, Sam M.2
- Bahcall, John N.3
- Balantekin, A. B.4
- Bogaert, Gilles5
- Brown, Lowell S.1
- Buchmann, Lothar6
- Cecil, F. Edward7
- Champagne, Arthur E.8
- Braeckeleer, Ludwig de9
- Duba, Charles A.1
- Elliott, Steven R.1
- Freedman, Stuart J.10
- Gai, Moshe11
- Goldring, G.12
- Gould, Christopher R.13
- Gruzinov, Andrei3
- Haxton, Wick C.1
- Heeger, Karsten M.1
- Henley, Ernest1
- Johnson, Calvin W.14
-
Kamionkowski, Marc15
- Kavanagh, Ralph W.16
- Koonin, Steven E.16
- Kubodera, Kuniharu17
- Langanke, Karlheinz18
- Motobayashi, Tohru19
- Pandharipande, Vijay20
- Parker, Peter21
- Robertson, R. G. H.1
- Rolfs, Claus22
- Sawyer, R. F.23
- Shaviv, N.16
- Shoppa, T. D.6
- Snover, K. A.1
- Swanson, Erik1
- Tribble, Robert E.24
- Turck-Chièze, Sylvaine25
- Wilkerson, John F.1
-
1.
University of Washington
-
2.
Michigan State University
-
3.
Institute for Advanced Study
-
4.
University of Wisconsin–Madison
-
5.
Institut National de Physique Nucléaire et de Physique des Particules
-
6.
TRIUMF
-
7.
Colorado School of Mines
-
8.
University of North Carolina at Chapel Hill
-
9.
Duke University
-
10.
University of California, Berkeley
-
11.
University of Connecticut
-
12.
Weizmann Institute of Science
-
13.
North Carolina State University
-
14.
Louisiana State University
-
15.
Columbia University
-
16.
California Institute of Technology
-
17.
University of South Carolina
-
18.
Aarhus University
-
19.
Rikkyo University
-
20.
University of Illinois Urbana-Champaign
-
21.
Yale University
-
22.
Ruhr University Bochum
-
23.
University of California, Santa Barbara
-
24.
Texas A&M University
-
25.
CEA Saclay
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
Published - ADErmp98.pdf
Files
ADErmp98.pdf
Additional details
Identifiers
- Eprint ID
- 3597
- Resolver ID
- CaltechAUTHORS:ADErmp98
Funding
- NSF
- Department of Energy (DOE)
Dates
- Created
-
2006-06-22Created from EPrint's datestamp field
- Updated
-
2021-11-08Created from EPrint's last_modified field