Solar fusion cross sections. II. The<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi><mml:mi>p</mml:mi></mml:math>chain and CNO cycles
E. G. AdelbergerDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAA. Garcı́aDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAR. G. H. RobertsonDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAK. A. SnoverDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAA. B. BalantekinDepartment of Physics, University of Wisconsin, Madison, Wisconsin 53706, USAK. M. HeegerDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAMichael J. Ramsey-MusolfDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAD. BemmererDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAA. JunghansForschungszentrum Dresden-Rossendorf, D-01314 Dresden, GermanyC. A. BertulaniDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAJiunn-Wei ChenDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAH. CostantiniDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAP. PratiUniversità degli Studi di GenovaM. CouderDepartment of Physics and JINA, University of Notre Dame, Notre Dame, Indiana 46556, USAE. UbersederDepartment of Physics and JINA, University of Notre Dame, Notre Dame, Indiana 46556, USAM. WiescherDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USARichard H. CyburtJINA and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USAB. DavidsDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAS. J. FreedmanDepartment of Physics, University of California, Berkeley, California 94720, USA and Lawrence Berkeley National Laboratory, Berkeley, California 94720, USAM. GaiYale University ;Doron GazitDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAL. GialanellaUniversity of Naples-Federico IIG. ImbrianiUniversity of Naples-Federico IIU. GreifeDepartment of Physics, Colorado School of Mines, Golden, Colorado 80401, USAM. HassDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAW. C. HaxtonDepartment of Physics, University of California, Berkeley, California 94720, USA and Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA and Institute for Nuclear Theory, University of Washington, Seattle, Washington 98195, USAT. ItahashiDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAK. KuboderaDepartment of Physics and Astronomy, University of South Carolina, Columbia, South Carolina 29208, USAK. LangankeGSI Helmholtzzentrum für Schwerionenforschung, D-64291 Darmstadt, Germany, Institut für Kernphysik, Universität Darmstadt, D-64289 Darmstadt, Germany, and Frankfurt Institute for Advanced Studies, D-60438 Frankfurt, GermanyM. LeitnerLawrence Berkeley National Laboratory, Berkeley, California 94720, USAPaul VetterDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAL. A. WinslowLawrence Berkeley National Laboratory, Berkeley, California 94720, USAL. E. MarcucciDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAT. MotobayashiDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAA. M. MukhamedzhanovDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAR. E. TribbleCyclotron Institute, Texas A&M University, College Station, Texas 77843, USAKenneth M. NollettPhysics Division, Argonne National Laboratory, 9700 South Cass Avenue, Argonne, Illinois 60439, USAF. M. NunesMichigan State UniversityTaemin ParkDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAP. D. ParkerDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAR. SchiavillaDepartment of Physics, Old Dominion University, Norfolk, Virginia 23529, USA and Jefferson Laboratory, Newport News, Virginia 23606, USAE. C. SimpsonDepartment of Physics, University of Surrey, Guildford, Surrey GU2 7XH, United KingdomC. SpitaleriDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAF. StriederInstitut für Experimentalphysik III, Ruhr-Universität Bochum, D-44780 Bochum, GermanyH. P. TrautvetterDepartment of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USAK. SuemmererGSI Helmholtzzentrum für Schwerionenforschung GmbH, Planckstraße 1, D-64291 Darmstadt, GermanyS. TypelTechnical University of Munich
2011en
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Annotatsiya
The available data on nuclear fusion cross sections important to energy generation in the Sun and other hydrogen-burning stars and to solar neutrino production are summarized and critically evaluated. Recommended values and uncertainties are provided for key cross sections, and a recommended spectrum is given for $^{8}\mathrm{B}$ solar neutrinos. Opportunities for further increasing the precision of key rates are also discussed, including new facilities, new experimental techniques, and improvements in theory. This review, which summarizes the conclusions of a workshop held at the Institute for Nuclear Theory, Seattle, in January 2009, is intended as a 10-year update and supplement to 1998, Rev. Mod. Phys. 70, 1265.
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