| dbo:abstract |
El factor S astrofísico es la variante reescalada de la sección transversal que considera la repulsión culombiana entre reactantes cargados. (es) In nuclear physics, the astrophysical S-factor S(E) is a rescaling of a nuclear reaction's total cross section σ(E) to account for the Coulomb repulsion between the charged reactants. It determines the rates of nuclear fusion reactions that occur in the cores of stars. (en) |
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dbr:Electric_charge dbr:Velocity dbr:Cross_section_(physics) dbr:Nuclear_physics dbr:Sommerfeld_parameter dbr:Star dbc:Equations_of_astronomy dbr:Nuclear_fusion dbr:Nuclear_reaction dbc:Astrophysics dbc:Nuclear_physics dbr:Reduced_Planck_constant dbr:Astrophysical dbr:Coulomb_repulsion dbr:Permittivity_of_free_space |
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dbc:Equations_of_astronomy dbc:Astrophysics dbc:Nuclear_physics |
| gold:hypernym |
dbr:Variant |
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owl:Thing |
| rdfs:comment |
El factor S astrofísico es la variante reescalada de la sección transversal que considera la repulsión culombiana entre reactantes cargados. (es) In nuclear physics, the astrophysical S-factor S(E) is a rescaling of a nuclear reaction's total cross section σ(E) to account for the Coulomb repulsion between the charged reactants. It determines the rates of nuclear fusion reactions that occur in the cores of stars. (en) |
| rdfs:label |
Factor S (es) S-factor (en) |
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dbr:Gamow_factor |
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freebase:S-factor wikidata:S-factor dbpedia-es:S-factor https://global.dbpedia.org/id/2PUki |
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wikipedia-en:S-factor?oldid=1059310580&ns=0 |
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wikipedia-en:S-factor |
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dbr:S_Factor |
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dbr:S_Factor dbr:Sommerfeld_parameter dbr:Nuclear_fusion |
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wikipedia-en:S-factor |