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Solar fusion cross sections. II. The pp chain and CNO cycles

E. G. Adelberger, A. García, R. G. Hamish Robertson, K. A. Snover, A. B. Balantekin, K. Heeger, M. J. Ramsey-Musolf, D. Bemmerer, A. Junghans et al.

E. G. Adelberger, A. García, R. G. Hamish Robertson, and K. A. Snover

  • Department of Physics and Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA

A. B. Balantekin, K. Heeger, and M. J. Ramsey-Musolf

  • Department of Physics, University of Wisconsin, Madison, Wisconsin 53706, USA

D. Bemmerer and A. Junghans

  • Forschungszentrum Dresden-Rossendorf, D-01314 Dresden, Germany

C. A. Bertulani

  • Department of Physics and Astronomy, Texas A&M University, Commerce, Texas 75429, USA

J.-W. Chen

  • Department of Physics, Center for Theoretical Sciences, and Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, Taipei 10617, Taiwan

H. Costantini and P. Prati

  • Università di Genova and INFN Sezione di Genova, I-16146 Genova, Italy

M. Couder, E. Uberseder, and M. Wiescher

  • Department of Physics and JINA, University of Notre Dame, Notre Dame, Indiana 46556, USA

R. Cyburt

  • JINA and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA

B. Davids

  • TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia, Canada V6T 2A3

S. J. Freedman

  • Department of Physics, University of California, Berkeley, California 94720, USA and Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA

M. Gai

  • Laboratory for Nuclear Sciences at Avery Point, University of Connecticut, Connecticut 06340-6097, USA and Department of Physics, Yale University, New Haven, Connecticut 06520-8124, USA

D. Gazit

  • Institute for Nuclear Theory, University of Washington, Seattle, Washington 98195, USA and Racah Institute of Physics, The Hebrew University, Jerusalem, 91904, Israel

L. Gialanella and G. Imbriani

  • Dipartimento di Scienze Fisiche, Università di Napoli, and INFN Sezione di Napoli, I-80126 Napoli, Italy

U. Greife

  • Department of Physics, Colorado School of Mines, Golden, Colorado 80401, USA

M. Hass

  • Department of Particle Physics and Astrophysics, The Weizmann Institute, Rehovot 76100, Israel

W. C. Haxton

  • Department 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, USA

T. Itahashi

  • Research Center for Nuclear Physics, Osaka University, Ibaraki, Osaka 567-0047 Japan

K. Kubodera

  • Department of Physics and Astronomy, University of South Carolina, Columbia, South Carolina 29208, USA

K. Langanke

  • GSI 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, Germany

D. Leitner, M. Leitner, P. Vetter, and L. Winslow

  • Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA

L. E. Marcucci

  • Department of Physics “E. Fermi,” University of Pisa, and INFN Sezione di Pisa, Largo Bruno Pontecorvo 3, I-56127, Pisa, Italy

T. Motobayashi

  • The Institute of Physical and Chemical Research (RIKEN), 2-1 Hirosawa, Wako, Saitama 351-0198, Japan

A. Mukhamedzhanov and R. E. Tribble

  • Cyclotron Institute, Texas A&M University, College Station, Texas 77843, USA

Kenneth M. Nollett

  • Physics Division, Argonne National Laboratory, 9700 South Cass Avenue, Argonne, Illinois 60439, USA

F. M. Nunes

  • National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA

T.-S. Park

  • Department of Physics and BAERI, Sungkyunkwan University, Suwon 440-746 Korea

P. D. Parker

  • Wright Nuclear Structure Laboratory, Yale University, New Haven, Connecticut 06520, USA

R. Schiavilla

  • Department of Physics, Old Dominion University, Norfolk, Virginia 23529, USA and Jefferson Laboratory, Newport News, Virginia 23606, USA

E. C. Simpson

  • Department of Physics, University of Surrey, Guildford, Surrey GU2 7XH, United Kingdom

C. Spitaleri

  • INFN Laboratori Nazionali del Sud and Dipartimento di Fisica ed Astronomia, Università di Catania, I-95123 Catania, Italy

F. Strieder and H.-P. Trautvetter

  • Institut für Experimentalphysik III, Ruhr-Universität Bochum, D-44780 Bochum, Germany

K. Suemmerer

  • GSI Helmholtzzentrum für Schwerionenforschung GmbH, Planckstraße 1, D-64291 Darmstadt, Germany

S. Typel

  • Excellence Cluster Universe, Technische Universität München, Boltzmannstraße 2, D-85748 Garching, Germany and GSI Helmholtzzentrum für Schwerionenforschung, Planckstraße 1, D-64291 Darmstadt, Germany

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Rev. Mod. Phys. 83, 195 – Published 12 April, 2011

DOI: https://doi.org/10.1103/RevModPhys.83.195

Abstract

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 B8 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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Rev. Mod. Phys. 83, 195– Published 12 April, 2011
  • Received 21 April 2010

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