Works citing this work

12 works

Work: Spectroscopic factors for the 1p shell

1. Modified 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

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2. New measurements of the astrophysical<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>S</mml:mi></mml:mrow></mml:math>factor for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mn>12</mml:mn></mml:mrow></mml:msup><mml:mi mathvariant="normal">C</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:msup><mml:mi/><mml:mrow><mml:mn>13</mml:mn></mml:mrow></mml:msup><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:math>reaction at low energies and the asymptotic normalization coefficient (nuclear vertex constant) for the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>+</mml:mo><mml:msup><mml:mi/><mml:mrow><mml:mn>12</mml:mn></mml:mrow></mml:msup><mml:mi mathvariant="normal">C</mml:mi><mml:mo>→</mml:mo><mml:msup><mml:mrow/><mml:mrow><mml:mn>13</mml:mn></mml:mrow></mml:msup><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:math>reaction

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   ABIABI:AkademIndex/openalex/2008.article.000043

3. Indirect 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

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4. Asymptotic normalization coefficients (nuclear vertex constants) for p + 7Be → 8B and the direct 7Be(p, γ)8B astrophysical S factors at solar energies

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5. Asymptotic normalization coefficient for the ⁶Li+n→7Li from the ⁶Li(d,p)7Li reaction and cross-section for the ⁶Li(n,γ)7Li reaction

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6. Effects of t- and α-transfer on the spectroscopic information from the reaction

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7. Extrapolation of astrophysical S factors for the reaction 14N((p, γ) 15O to near-zero energies

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8. Asymptotic normalization coefficient for⁶He+p→7Li from the proton transfer d(⁶He,⁷Li)n reaction

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   ABIABI:AkademIndex/openalex/2023.article.001000

9. Comparison of asymptotic normalization coefficients for 10B → 9B + n and 10B → 9Be + p configurations obtained from 10B(d,t)9B and 10B(d,3He)9Be reactions

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   ArticleNuclear physics research studiesBulletin of the Russian Academy of Sciences Physics20111 citations

   ABIABI:AkademIndex/openalex/2011.article.000201

10. Asymptotic normalization coefficient for ⁸ Be→ ⁷ Li+p from the ⁷ Li( ³ He,d) ⁸ Be reaction and astrophysical S factor for the radiative capture ⁷ Li(p,γ) ⁸ Be reaction

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11. The Nuclear Spin-Orbital Interaction and Characteristics of Light Pionic Atoms

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    ABIABI:AkademIndex/openalex/1992.chapter.000007

12. Asymptotic normalization coefficients for the ⁷ Li → { ⁶ He + <i>p</i> } configuration from the ⁷ Li ( <i>d</i> , ³ He) ⁶ He reaction

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