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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
  • , C. A. Bertulani
  • , J. W. Chen
  • , H. Costantini
  • , P. Prati
  • , M. Couder
  • , E. Uberseder
  • , M. Wiescher
  • , R. Cyburt
  • , B. Davids
  • , S. J. Freedman
  • , M. Gai
  • D. Gazit, L. Gialanella, G. Imbriani, U. Greife, M. Hass, W. C. Haxton, T. Itahashi, K. Kubodera, K. Langanke, D. Leitner, M. Leitner, P. Vetter, L. Winslow, L. E. Marcucci, T. Motobayashi, A. Mukhamedzhanov, R. E. Tribble, Kenneth M. Nollett, F. M. Nunes, T. S. Park, P. D. Parker, R. Schiavilla, E. C. Simpson, C. Spitaleri, F. Strieder, H. P. Trautvetter, K. Suemmerer, S. Typel
  • University of Washington
  • University of Wisconsin-Madison
  • Helmholtz-Zentrum Dresden-Rossendorf
  • Texas A&M University
  • National Taiwan University
  • University of Genoa
  • University of Notre Dame
  • Michigan State University
  • TRIUMF
  • University of California at Berkeley
  • Lawrence Berkeley National Laboratory
  • University of Connecticut
  • Yale University
  • Hebrew University of Jerusalem
  • University of Naples Federico II
  • Colorado School of Mines
  • Weizmann Institute of Science
  • The University of Osaka
  • University of South Carolina
  • GSI Helmholtz Centre for Heavy Ion Research
  • Technische Universität Darmstadt
  • Goethe University Frankfurt
  • University of Pisa
  • RIKEN
  • United States Department of Energy
  • Argonne National Laboratory
  • Old Dominion University
  • University of Surrey
  • Jefferson Lab
  • University of Catania
  • Ruhr University Bochum
  • Technische Universität München

Research output: Contribution to journalArticlepeer-review

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, 1265RMPHAT0034-686110.1103/RevModPhys.70.1265.

Original languageEnglish
Pages (from-to)195-245
Number of pages51
JournalReviews of Modern Physics
Volume83
Issue number1
DOIs
StatePublished - 12 Apr 2011

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