Organizing Committee:

Eric Adelberger, Univ. Washington
Heide Costantini, INFN-Genova
Wick Haxton, Univ. Washington
Peter Parker, Yale Univ.
R. G. Hamish Robertson, Univ. Washington
Kurt Snover, Univ. Washington
Frank Strieder, Ruhr-U. Bochum
Michael Wiescher, Notre Dame

Program Coordinator:
Inge Dolan
inge@phys.washington.edu
(206) 685-4286

Application form

Schedule

Participant List

Working Group Participation

Talks online

Reviews of Modern Physics -
Information for authors

Obtain an INT preprint number

INT homepage

Solar Fusion Cross Sections for the pp chain and CNO cycle

January 21-23 2009


Solar Fusion II paper

There is a mandatory registration fee of $75 to attend this workshop, payable in cash (preferred) or a check drawn on a U.S. bank.

The INT is grateful to the Joint Institute for Nuclear Astrophysics for its contributions in support of this workshop.

Introduction:

In February 1997, at the suggestion of John Bahcall, a group of investigators interested in the solar neutrino problem (and in hydrogen-burning stars generally) gathered at the Institute for Nuclear Theory to assess what is known about the nuclear physics of solar energy production. The group critically analyzed cross section data and theoretical analyses of that data to provide a set of "best values" and uncertainties for the needed S-factors. The results of this workshop were presented in a Reviews of Modern Physics article, RMP 70 (1998) 1265, that is now rated by Spires as a "famous paper."

The purpose of the 21-23 January 2009 workshop will be to reassess these cross section recommendations, in light of a variety of important new measurements and theory developments of the past decade. The workshop will be organized around twelve working groups:

Working Group Working Group Leaders
1. S11 and Related Theory
    Key Papers
Jiunn-Wei Chen, National Taiwan Univ.
Kuniharu Kubodera, Univ. South Carolina
2. 3He+3He S-factor
    Key Papers
Uwe Greife, Colorado School of Mines
Paolo Prati, INFN-Genova
3. p + 7Be and p+d S-factors
    Key Papers
Gianluca Imbriani, Univ. Napoli
Michael Hass, Weizmann Institute
4. Neutrino spectra
    Key Papers
Stuart Freedman, Univ. California Berkeley
Alejandro Garcia, Univ. Washington
5. 14N(p,γ) S-factor
    Key Papers
Heide Costantini, INFN-Genova
Hanns-Peter Trautvetter, Ruhr-U. Bochum
6. Other CNO S-factors
    Key Papers
Peter Parker, Yale Univ.
R. G. Hamish Robertson, Univ. Washington
7. 3He+4He S-factor
    Key Papers
Kurt Snover, Univ. Washington
Frank Strieder, Ruhr-U. Bochum
8. hep S-factor
   Key Papers
Laura Marcucci, Univ. of Pisa
Tae-Sun Park, Sungkyunkwan Univ.
9. 7Be, pep, CNO electron capture
    Key Papers
Andrei Gruzinov, New York Univ.
R. G. Hamish Robertson, Univ. Washington
10. Theoretical issues
       Key Papers
Wick Haxton, Univ. Washington
Stefan Typel, GSI
11. Validating new techniques:
           Trojan horse/Coulomb
           dissociation/asymptotic
           normalization
       Key Papers
Eric Adelberger, Univ. Washington
Barry Davids, TRIUMF
Filomena Nunes, Michigan State Univ.
12. Future facilities
        Key Papers
Daniela Leitner, Lawrence Berkeley Lab
Michael Wiescher, Notre Dame Univ.

While applications are welcome, the attendance will be capped (as in 1997) so that the working groups can function efficiently. The organizers and working group leaders will work together in making decisions on applications, if oversubscription occurs.

Working group leaders will also identify and post key papers on this page, prior to the start of the workshop. Please feel free to contact the working group leaders if you see important omissions. The emphasis will be on work done since the 1997 workshop.