Ushbu ish iqtibos qilgan ishlar

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

   Maqola199733 iqtibos

   ABIABI:AkademIndex/2026.other.171551

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

   A. J. Koning, J. P. Delaroche

   Maqola200214 iqtibos

   ABIABI:AkademIndex/2026.other.003936

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

   Maqola201312 iqtibos

   ABIABI:AkademIndex/2026.other.286704

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 Physics20099 iqtibos

   ABIABI:AkademIndex/2009.article.000054

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

   Haixia An, Chonghai Cai

   Maqola20069 iqtibos

   ABIABI:AkademIndex/2026.other.003991

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

   MaqolaOAOchiq kirishNuclear physics research studiesPhysical review. C20168 iqtibos

   ABIABI:AkademIndex/2026.other.178243

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

   Maqola19947 iqtibos

   ABIABI:AkademIndex/2026.other.286709

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

   N. K. Timofeyuk

   Maqola20105 iqtibos

   ABIABI:AkademIndex/2026.other.366913

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

   Robert Malaney, William A. Fowler

   Maqola19884 iqtibos

   ABIABI:AkademIndex/2026.other.375089

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

    ABIABI:AkademIndex/2026.other.450993

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

    ABIABI:AkademIndex/2026.other.178228

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

    J. Lohr, W. Haeberli

    Maqola19742 iqtibos

    ABIABI:AkademIndex/2026.other.450987

13. Sarlavhasiz

    Boshqa2 iqtibos

    ABIABI:AkademIndex/2026.other.450992

14. 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

    ABIABI:AkademIndex/2026.other.450995

15. Transfer reaction code with nonlocal interactions

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

    Maqola20162 iqtibos

    ABIABI:AkademIndex/2026.other.450997

16. <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

    ABIABI:AkademIndex/2026.other.450999

17. Sarlavhasiz

    Boshqa1 iqtibos

    ABIABI:AkademIndex/2026.other.450980

18. Sarlavhasiz

    Boshqa1 iqtibos

    ABIABI:AkademIndex/2026.other.450981

19. Sarlavhasiz

    Boshqa1 iqtibos

    ABIABI:AkademIndex/2026.other.450982

20. Sarlavhasiz

    Boshqa1 iqtibos

    ABIABI:AkademIndex/2026.other.450983

21. Sarlavhasiz

    Boshqa1 iqtibos

    ABIABI:AkademIndex/2026.other.450984

22. Sarlavhasiz

    Boshqa1 iqtibos

    ABIABI:AkademIndex/2026.other.450985

23. Sarlavhasiz

    Boshqa1 iqtibos

    ABIABI:AkademIndex/2026.other.450986

24. Sarlavhasiz

    Boshqa1 iqtibos

    ABIABI:AkademIndex/2026.other.450988

25. Sarlavhasiz

    Boshqa1 iqtibos

    ABIABI:AkademIndex/2026.other.450989