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Иш: Extraction of 15N ANC from the 14N(d,p)15N 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
Мақола199729 иқтибосABIModified two-body potential approach to the peripheral direct capture astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:mi>a</mml:mi><mml:mo>+</mml:mo><mml:mi>A</mml:mi><mml:mo>→</mml:mo><mml:mi>B</mml:mi><mml:mo>+</mml:mo><mml:mi>γ</mml:mi></mml:math> reaction and asymptotic normalization coefficients
S. B. Igamov, R. Yarmukhamedov
ABINucleon-Nucleus Optical-Model Parameters,<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>A</mml:mi><mml:mo>></mml:mo><mml:mn/><mml:mn>40</mml:mn><mml:mn/></mml:math>,<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>E</mml:mi><mml:mo><</mml:mo><mml:mn/><mml:mn>50</mml:mn><mml:mn/></mml:math>MeV
F. D. Becchetti, G. W. Greenlees
Мақола19699 иқтибосABIDeuteron global optical model potential for energies up to 200 MeV
Yinlu Han, Yuyang Shi, Qingbiao Shen
Мақола20067 иқтибосABIStudy of the (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>d</mml:mi><mml:mo>,</mml:mo><mml:mi> </mml:mi><mml:mi>p</mml:mi></mml:math>) Reaction in the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mn>1</mml:mn><mml:mi>p</mml:mi></mml:math>Shell
J. P. Schiffer, G. C. Morrison, R.H. Siemssen +1
Мақола19673 иқтибосABINew method of analytic continuation of elastic-scattering data to the negative-energy region, and asymptotic normalization coefficients for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>17</mml:mn></mml:mmultiscripts></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">C</mml:mi><mml:mprescripts/><mml:none/><mml:mn>13</mml:mn></mml:mmultiscripts></mml:math>
L. D. Blokhintsev, A. S. Kadyrov, A. M. Mukhamedzhanov +1
Мақола20192 иқтибосABI