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Proton–proton chain (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "Proton–proton chain" in English language version.

refsWebsite
Global rank English rank
6doi.org
2nd place
2nd place
5harvard.edu
18th place
17th place
4arxiv.org
69th place
59th place
4semanticscholar.org
11th place
8th place
4worldcat.org
5th place
5th place
1web.archive.org
1st place
1st place
1utk.edu
4,653rd place
3,286th place
1books.google.com
3rd place
3rd place
1caltech.edu
887th place
714th place
1nih.gov
4th place
4th place
1in2p3.fr
low place
low place

arxiv.org

  • Adelberger, Eric G.; et al. (12 April 2011). "Solar fusion cross sections. II. The pp chain and CNO cycles". Reviews of Modern Physics. 83 (1): 201. arXiv:1004.2318. Bibcode:2011RvMP...83..195A. doi:10.1103/RevModPhys.83.195. S2CID 119117147. See Figure 2. The caption is not very clear but it has been confirmed that the percentages refer to how much of each reaction takes place, or equivalently how much helium-4 is produced by each branch.
  • Aldo Serenelli; et al. (Nov 2009). "New Solar Composition: The Problem With Solar Models Revisited". The Astrophysical Journal Letters. 705 (2): L123–L127. arXiv:0909.2668. Bibcode:2009ApJ...705L.123S. doi:10.1088/0004-637X/705/2/L123. S2CID 14323767. Calculated from model AGSS09 in Table 3.
  • Adelberger, E. G.; et al. (2010). "Solar fusion cross sections. II. Theppchain and CNO cycles". Reviews of Modern Physics. 83: 195–245. arXiv:1004.2318. doi:10.1103/RevModPhys.83.195. S2CID 119117147.
  • Bellini, G.; et al. (2 February 2012). "First Evidence of pep Solar Neutrinos by Direct Detection in Borexino". Physical Review Letters. 108 (5): 051302. arXiv:1110.3230. Bibcode:2012PhRvL.108e1302B. doi:10.1103/PhysRevLett.108.051302. PMID 22400925. S2CID 118444784.

books.google.com

caltech.edu

authors.library.caltech.edu

doi.org

  • Adelberger, Eric G.; et al. (12 April 2011). "Solar fusion cross sections. II. The pp chain and CNO cycles". Reviews of Modern Physics. 83 (1): 201. arXiv:1004.2318. Bibcode:2011RvMP...83..195A. doi:10.1103/RevModPhys.83.195. S2CID 119117147. See Figure 2. The caption is not very clear but it has been confirmed that the percentages refer to how much of each reaction takes place, or equivalently how much helium-4 is produced by each branch.
  • Hans Bethe (Mar 1, 1939). "Energy Production in Stars". Physical Review. 55 (5): 434–456. Bibcode:1939PhRv...55..434B. doi:10.1103/PhysRev.55.434.
  • Aldo Serenelli; et al. (Nov 2009). "New Solar Composition: The Problem With Solar Models Revisited". The Astrophysical Journal Letters. 705 (2): L123–L127. arXiv:0909.2668. Bibcode:2009ApJ...705L.123S. doi:10.1088/0004-637X/705/2/L123. S2CID 14323767. Calculated from model AGSS09 in Table 3.
  • Burbidge, E.; Burbidge, G.; Fowler, William; Hoyle, F. (1 October 1957). "Synthesis of the Elements in Stars" (PDF). Reviews of Modern Physics. 29 (4): 547–650. Bibcode:1957RvMP...29..547B. doi:10.1103/RevModPhys.29.547.
  • Adelberger, E. G.; et al. (2010). "Solar fusion cross sections. II. Theppchain and CNO cycles". Reviews of Modern Physics. 83: 195–245. arXiv:1004.2318. doi:10.1103/RevModPhys.83.195. S2CID 119117147.
  • Bellini, G.; et al. (2 February 2012). "First Evidence of pep Solar Neutrinos by Direct Detection in Borexino". Physical Review Letters. 108 (5): 051302. arXiv:1110.3230. Bibcode:2012PhRvL.108e1302B. doi:10.1103/PhysRevLett.108.051302. PMID 22400925. S2CID 118444784.

harvard.edu

ui.adsabs.harvard.edu

  • Adelberger, Eric G.; et al. (12 April 2011). "Solar fusion cross sections. II. The pp chain and CNO cycles". Reviews of Modern Physics. 83 (1): 201. arXiv:1004.2318. Bibcode:2011RvMP...83..195A. doi:10.1103/RevModPhys.83.195. S2CID 119117147. See Figure 2. The caption is not very clear but it has been confirmed that the percentages refer to how much of each reaction takes place, or equivalently how much helium-4 is produced by each branch.
  • Hans Bethe (Mar 1, 1939). "Energy Production in Stars". Physical Review. 55 (5): 434–456. Bibcode:1939PhRv...55..434B. doi:10.1103/PhysRev.55.434.
  • Aldo Serenelli; et al. (Nov 2009). "New Solar Composition: The Problem With Solar Models Revisited". The Astrophysical Journal Letters. 705 (2): L123–L127. arXiv:0909.2668. Bibcode:2009ApJ...705L.123S. doi:10.1088/0004-637X/705/2/L123. S2CID 14323767. Calculated from model AGSS09 in Table 3.
  • Burbidge, E.; Burbidge, G.; Fowler, William; Hoyle, F. (1 October 1957). "Synthesis of the Elements in Stars" (PDF). Reviews of Modern Physics. 29 (4): 547–650. Bibcode:1957RvMP...29..547B. doi:10.1103/RevModPhys.29.547.
  • Bellini, G.; et al. (2 February 2012). "First Evidence of pep Solar Neutrinos by Direct Detection in Borexino". Physical Review Letters. 108 (5): 051302. arXiv:1110.3230. Bibcode:2012PhRvL.108e1302B. doi:10.1103/PhysRevLett.108.051302. PMID 22400925. S2CID 118444784.

in2p3.fr

indico.ijclab.in2p3.fr

  • Int'l Conference on Neutrino and Dark Matter, 7 Sept 2006, Session 14.

nih.gov

pubmed.ncbi.nlm.nih.gov

semanticscholar.org

api.semanticscholar.org

  • Adelberger, Eric G.; et al. (12 April 2011). "Solar fusion cross sections. II. The pp chain and CNO cycles". Reviews of Modern Physics. 83 (1): 201. arXiv:1004.2318. Bibcode:2011RvMP...83..195A. doi:10.1103/RevModPhys.83.195. S2CID 119117147. See Figure 2. The caption is not very clear but it has been confirmed that the percentages refer to how much of each reaction takes place, or equivalently how much helium-4 is produced by each branch.
  • Aldo Serenelli; et al. (Nov 2009). "New Solar Composition: The Problem With Solar Models Revisited". The Astrophysical Journal Letters. 705 (2): L123–L127. arXiv:0909.2668. Bibcode:2009ApJ...705L.123S. doi:10.1088/0004-637X/705/2/L123. S2CID 14323767. Calculated from model AGSS09 in Table 3.
  • Adelberger, E. G.; et al. (2010). "Solar fusion cross sections. II. Theppchain and CNO cycles". Reviews of Modern Physics. 83: 195–245. arXiv:1004.2318. doi:10.1103/RevModPhys.83.195. S2CID 119117147.
  • Bellini, G.; et al. (2 February 2012). "First Evidence of pep Solar Neutrinos by Direct Detection in Borexino". Physical Review Letters. 108 (5): 051302. arXiv:1110.3230. Bibcode:2012PhRvL.108e1302B. doi:10.1103/PhysRevLett.108.051302. PMID 22400925. S2CID 118444784.

utk.edu

csep10.phys.utk.edu

web.archive.org

worldcat.org

search.worldcat.org

worldcat.org