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Work: Asymptotic normalization coefficient for<sup>6</sup>He+p→7Li from the proton transfer d(<sup>6</sup>He,<sup>7</sup>Li)n reaction
Asymptotic normalization coefficients for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>10</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">B</mml:mi><mml:mrow><mml:msup><mml:mrow><mml:mo>→</mml:mo></mml:mrow><mml:mrow><mml:mn>9</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">Be</mml:mi><mml:mo>+</mml:mo><mml:mi>p</mml:mi></mml:math>
A. M. Mukhamedzhanov, H. L. Clark, C. A. Gagliardi +9
Article199729 citationsABIGlobal optical model potential for elastic deuteron scattering from 12 to 90 MeV
W. W. Daehnick, J.D. Childs, Zoran Vrcelj
Article198010 citationsABIIndirect determination of the astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>S</mml:mi></mml:math> factor for the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</mml:mn></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> reaction using the asymptotic normalization coefficient method
G. Kiss, M. La Cognata, R. Yarmukhamedov +38
ABIDeuteron global optical model potential for energies up to 200 MeV
Yinlu Han, Yuyang Shi, Qingbiao Shen
Article20067 citationsABIElastic scattering of 52 MeV deuterons
F. Hinterberger, G. Mairle, U. Schmidt-Rohr +2
Article19684 citationsABIA global nucleon optical model potential
R. L. Varner, William J. Thompson, T.L. McAbee +2
Article19914 citationsABIAsymptotic 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
ABI<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:mrow></mml:math>reaction rate in the light of the new data of the Laboratory for Underground Nuclear Astrophysics
S. B. Dubovichenko, A. S. Tkachenko, Roman Ya. Kezerashvili +2
Article20224 citationsABIA systematic study of elastic scattering of polarized deuterons around 30 MeV by complex nuclei
G. Perrin, Nguyen Van Sen, J. Arvieux +6
Article19772 citationsABIFirst measurement of the 2H(6He,7Li)n angular distribution and proton spectroscopic factor in 7Li
Zhihong Li, E. T. Li, Bing Guo +10
Article20102 citationsABI