2004
DOI: 10.1007/s10894-004-1872-4
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The Oxygen to Carbon Ratio in the Solar Interior: Information from Nuclear Reaction Cross-Sections

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Cited by 4 publications
(20 citation statements)
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“…The atomic ratio, O/C ~ 2, at the surface of the Sun because fractionation moves lighter C selectively to the surface. O/C ~ 10 inside the Sun [83].…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…The atomic ratio, O/C ~ 2, at the surface of the Sun because fractionation moves lighter C selectively to the surface. O/C ~ 10 inside the Sun [83].…”
Section: Discussionmentioning
confidence: 99%
“…This mass fractionation is recorded in the abundances of 72 s-products in the photosphere spanning a mass range of 25-207 mu [22]. Te [82], but photospheric abundances of s-products [22] exponentially decline by ~5 orders of magnitude over the mass range of A = 25-207 mu [83], as shown on the right side of Fig. 6 [83].…”
Section: Ubiquitous Mass Fractionated Isotopesmentioning
confidence: 99%
“…The bulk of the Sun is made mostly of Fe, Ni, O, Si, and S, suggesting "that fusion of hydrogen is probably not the Sun's primary energy source" and origin of the solar system from radioactive supernova debris [10,36,37]. The Sun is powered by creation of atomic size dynamic fractals in the core of its stellar type 3D-spiral vortex structure (Figure 3).…”
Section: Tablementioning
confidence: 99%
“…Other measurements [7][8][9] independently confirmed that the Sun selectively moves lighter ions into the photosphere, over the mass range of A = 25-207 amu [8], leaving little doubt that the interior of the Sun is iron-rich [6] like the material that formed iron meteorites and iron cores of rocky planets at the birth of the solar system [20][21]. Iron is however made of tightly packed nucleons [2] and is therefore an unlikely source of nuclear energy.…”
Section: The Energy Source For An Iron-rich Stratified Sunmentioning
confidence: 99%
“…Except for Coulomb repulsion, the n-n and p-p interactions are symmetric [3]. H, from stars [3][4][5][7][8][9]. Thus, in the stellar interiors (neutron-emission) + (neutron-decay) = (hydrogen production), despite reports that neutron stars are "dead" nuclear matter with each neutron in a neutron star having about 93 MeV less energy than a free neutron [27].…”
Section: Insert Figurementioning
confidence: 99%