Πυρηνική αντίδραση αλυσίδας πρωτονίου-πρωτονίου (Greek Wikipedia)

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Hans Bethe (Mar 1, 1939). «Energy Production in Stars». Physical Review 55 (5): 434–456. doi:10.1103/PhysRev.55.434. Bibcode: 1939PhRv...55..434B. https://archive.org/details/sim_physical-review_1939-03-01_55_5/page/434.
Adelberger, Eric G. (12 April 2011). «Solar fusion cross sections. II. The pp chain and CNO cycles». Reviews of Modern Physics 83 (1): 201. doi:10.1103/RevModPhys.83.195. Bibcode: 2011RvMP...83..195A. 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 (Nov 2009). «New Solar Composition: The Problem With Solar Models Revisited». The Astrophysical Journal Letters 705 (2): L123–L127. doi:10.1088/0004-637X/705/2/L123. Bibcode: 2009ApJ...705L.123S. Calculated from model AGSS09 in Table 3.
Burbidge, E.; Burbidge, G.; Fowler, William; Hoyle, F. (1 October 1957). «Synthesis of the Elements in Stars». Reviews of Modern Physics 29 (4): 547–650. doi:10.1103/RevModPhys.29.547. Bibcode: 1957RvMP...29..547B. This value excludes the 2% neutrino energy loss.
Bellini, G. (2 February 2012). «First Evidence of pep Solar Neutrinos by Direct Detection in Borexino». Physical Review Letters 108 (5): 051302. doi:10.1103/PhysRevLett.108.051302. PMID 22400925. Bibcode: 2012PhRvL.108e1302B.

Hans Bethe (Mar 1, 1939). «Energy Production in Stars». Physical Review 55 (5): 434–456. doi:10.1103/PhysRev.55.434. Bibcode: 1939PhRv...55..434B. https://archive.org/details/sim_physical-review_1939-03-01_55_5/page/434.
Adelberger, Eric G. (12 April 2011). «Solar fusion cross sections. II. The pp chain and CNO cycles». Reviews of Modern Physics 83 (1): 201. doi:10.1103/RevModPhys.83.195. Bibcode: 2011RvMP...83..195A. 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 (Nov 2009). «New Solar Composition: The Problem With Solar Models Revisited». The Astrophysical Journal Letters 705 (2): L123–L127. doi:10.1088/0004-637X/705/2/L123. Bibcode: 2009ApJ...705L.123S. Calculated from model AGSS09 in Table 3.
Burbidge, E.; Burbidge, G.; Fowler, William; Hoyle, F. (1 October 1957). «Synthesis of the Elements in Stars». Reviews of Modern Physics 29 (4): 547–650. doi:10.1103/RevModPhys.29.547. Bibcode: 1957RvMP...29..547B. This value excludes the 2% neutrino energy loss.
Bellini, G. (2 February 2012). «First Evidence of pep Solar Neutrinos by Direct Detection in Borexino». Physical Review Letters 108 (5): 051302. doi:10.1103/PhysRevLett.108.051302. PMID 22400925. Bibcode: 2012PhRvL.108e1302B.

Bellini, G. (2 February 2012). «First Evidence of pep Solar Neutrinos by Direct Detection in Borexino». Physical Review Letters 108 (5): 051302. doi:10.1103/PhysRevLett.108.051302. PMID 22400925. Bibcode: 2012PhRvL.108e1302B.

«The Proton–Proton Chain». Astronomy 162: Stars, Galaxies, and Cosmology. Αρχειοθετήθηκε από το πρωτότυπο στις 20 Ιουνίου 2016. Ανακτήθηκε στις 30 Ιουλίου 2018.

«The Proton–Proton Chain». Astronomy 162: Stars, Galaxies, and Cosmology. Αρχειοθετήθηκε από το πρωτότυπο στις 20 Ιουνίου 2016. Ανακτήθηκε στις 30 Ιουλίου 2018.
Int'l Conference on Neutrino and Dark Matter, Thursday 07 Sept 2006, https://indico.lal.in2p3.fr/getFile.py/access?contribId=s16t1&sessionId=s16&resId=1&materialId=0&confId=a05162 Αρχειοθετήθηκε 2009-08-04 στο Wayback Machine. Session 14.