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33 ta ish

Ish: ANC and SF of bound states in 15N→14C+p, 16O→15N+p, 19F→18O+p, 32S→31P+p

  1. 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

    Maqola199729 iqtibos
    ABI

  2. Local and global nucleon optical models from 1 keV to 200 MeV

    A. J. Koning, J. P. Delaroche

    Maqola200212 iqtibos
    ABI

  3. Spectroscopic factors and asymptotic normalization coefficients for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mn>0</mml:mn><mml:mi>p</mml:mi></mml:mrow></mml:math>-shell nuclei: Recent updates

    N. K. Timofeyuk

    Maqola201310 iqtibos
    ABI

  4. 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 Physics20098 iqtibos
    ABI

  5. Global deuteron optical model potential for the energy range up to 183 MeV

    Haixia An, Chonghai Cai

    Maqola20068 iqtibos
    ABI

  6. Asymptotic normalization coefficients for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts><mml:mspace width="0.16em"/><mml:mo>+</mml:mo><mml:mspace width="0.16em"/><mml:mi>p</mml:mi><mml:mo>→</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mn>8</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> from the peripheral <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>d</mml:mi><mml:mo>,</mml:mo><mml:mi>n</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mn>8</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> reaction and their astrophysical application

    O. R. Tojiboev, R. Yarmukhamedov, S. V. Artemov +1

    MaqolaNuclear physics research studiesPhysical review. C20168 iqtibos
    ABI

  7. Spectroscopic factors from one-proton stripping reactions on sd-shell nuclei: experimental measurements and shell-model calculations

    J. Vernotte, G. Berrier-Ronsin, J. Kalifa +2

    Maqola19946 iqtibos
    ABI

  8. Overlap functions, spectroscopic factors, and asymptotic normalization coefficients generated by a shell-model source term

    N. K. Timofeyuk

    Maqola20105 iqtibos
    ABI

  9. Late-time neutron diffusion and nucleosynthesis in a post-QCD inhomogeneous Omega(b) = 1 universe

    Robert Malaney, William A. Fowler

    Maqola19884 iqtibos
    ABI

  10. Global optical model potential for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>A</mml:mi><mml:mo>=</mml:mo><mml:mn>3</mml:mn></mml:mrow></mml:math>projectiles

    D. Y. Pang, P. Roussel-Chomaz, H. Savajols +2

    Maqola20094 iqtibos
    ABI

  11. New 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 the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">N</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>15</mml:mn></mml:mrow></mml:mmultiscripts></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><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:mrow></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>16</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>reaction via the asymptotic normalization coefficient (ANC) method

    A. M. Mukhamedzhanov, P. Bém, V. Burjan +17

    Maqola20082 iqtibos
    ABI

  12. Elastic scattering of 9–13 MeV vector polarized deuterons

    J. Lohr, W. Haeberli

    Maqola19742 iqtibos
    ABI

  13. Optical model potential of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>A</mml:mi><mml:mo>=</mml:mo><mml:mn>3</mml:mn></mml:mrow></mml:math>projectiles for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mn>1</mml:mn><mml:mi>p</mml:mi></mml:mrow></mml:math>-shell nuclei

    D. Y. Pang, W. M. Dean, A. M. Mukhamedzhanov

    Maqola20152 iqtibos
    ABI

  14. Transfer reaction code with nonlocal interactions

    L. J. Titus, A. Ross, F. M. Nunes

    Maqola20162 iqtibos
    ABI

  15. <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 iqtibos
    ABI

  16. Sarlavhasiz

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  19. Sarlavhasiz

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  20. Sarlavhasiz

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  21. Sarlavhasiz

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  22. Sarlavhasiz

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  23. Sarlavhasiz

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  24. Sarlavhasiz

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  25. Sarlavhasiz

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