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Ish: 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
MaqolaNuclear physics research studiesBulletin of the Russian Academy of Sciences Physics20099 iqtibosABIAsymptotic 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
ABISimple optical model treatment of the elastic 3He scattering
H.J. Trost, P. Lezoch, U. Strohbusch
Maqola19876 iqtibosABIA global nucleon optical model potential
R. L. Varner, William J. Thompson, T.L. McAbee +2
Maqola19915 iqtibosABIThe (d, n) reaction on 1p shell nuclei at Ed = 11.8 MeV
G. S. Mutchler, D. Rendić, Donald E. Velkley +2
Maqola19714 iqtibosABIComparaison des réactions (d, 3He) ET (d, t) sur quelques noyaux N = Z
M. J. Gaillard, R. Bouché, L. Feuvrais +5
Maqola19684 iqtibosABITransfer reaction code with nonlocal interactions
L. J. Titus, A. Ross, F. M. Nunes
Maqola20162 iqtibosABI<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
Maqola20172 iqtibosABISignatures of inhomogeneity in the early universe
Lawrence Kawano, William A. Fowler, Ralph W. Kavanagh +1
Maqola19912 iqtibosABI