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Иш: Asymptotic Normalization Coefficients for Proton Coupling in 12C
Determination of nuclear vertex constants (asymptotic normalization coefficients) for the virtual decays 3He → d + p and 17F → 16O + p and their use for extrapolating astrophysical S-factors of the radiative proton capture by the deuteron and the 16O nucleus at very low energies
S. V. Artemov, S. B. Igamov, K. I. Tursunmakhatov +1
МақолаNuclear physics research studiesBulletin of the Russian Academy of Sciences Physics20098 иқтибосABISimple optical model treatment of the elastic 3He scattering
H.J. Trost, P. Lezoch, U. Strohbusch
Мақола19876 иқтибосABIThe (d, n) reaction on 1p shell nuclei at Ed = 11.8 MeV
G. S. Mutchler, D. Rendić, Donald E. Velkley +2
Мақола19714 иқтибосABIA global nucleon optical model potential
R. L. Varner, William J. Thompson, T.L. McAbee +2
Мақола19914 иқтибосABIAsymptotic normalization coefficient for $${{}^{12}\mathrm{C}}+p\rightarrow {{}^{13}\mathrm{N}}$$ from the $${}^{12}{\mathrm{C}}({}^{10}\mathrm{B},{}^{9}{\mathrm{Be}}){}^{13}\mathrm{N}$$ reaction and the $${}^{12}\mathrm{C}(p,\gamma ){}^{13}\mathrm{N}$$ astrophysical S factor
S. V. Artemov, R. Yarmukhamedov, N. Burtebayev +22
ABIComparaison des réactions (d, 3He) ET (d, t) sur quelques noyaux N = Z
M. J. Gaillard, R. Bouché, L. Feuvrais +5
Мақола19683 иқтибосABITransfer reaction code with nonlocal interactions
L. J. Titus, A. Ross, F. M. Nunes
Мақола20162 иқтибосABI<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mo>(</mml:mo><mml:mi>d</mml:mi><mml:mo>,</mml:mo><mml:mi>n</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math> proton-transfer reactions on <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>9</mml:mn></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mo> </mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mn>11</mml:mn></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mo> </mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">C</mml:mi><mml:mprescripts/><mml:none/><mml:mn>13</mml:mn></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mo> </mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">N</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>14</mml:mn><mml:mo>,</mml:mo><mml:mn>15</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>, and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">F</mml:mi><mml:mprescripts/><mml:none/><mml:mn>19</mml:mn></mml:mmultiscripts></mml:math> and spectroscopic factors at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mi>d</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>16</mml:mn><mml:mspace width="0.16em"/><mml:mi>MeV</mml:mi></mml:mrow></mml:math>
M. Febbraro, F.D. Becchetti, R. O. Torres-Isea +4
Мақола20172 иқтибосABISignatures of inhomogeneity in the early universe
Lawrence Kawano, William A. Fowler, Ralph W. Kavanagh +1
Мақола19912 иқтибосABI