Ушбу иш иқтибос қилган ишлар

12 та иш

Иш: 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

1. Compilation of phenomenological optical-model parameters 1954–1975

   C. M. Perey, F.G. Perey

   Мақола197614 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.212678

2. Spectroscopic factors for the 1p shell

   S. Cohen, D. Kurath

   Мақола196712 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.171512

3. Nuclear asymptotic normalization coefficients for 14N → 13C + p configurations and astrophysical S factor for radiative proton capture

   S. V. Artemov, A. G. Bajajin, S. B. Igamov +2

   МақолаNuclear physics research studiesPhysics of Atomic Nuclei20089 иқтибос

   ABIABI:AkademIndex/openalex/2008.article.000051

4. Method for selecting peripheral reactions dominated by the pole mechanism: Analysis of (d,t) reactions on 1p-shell and {sup 19}F nuclei

   I.R. Gulamov, A. M. Mukhamedzhanov, G. K. Nie

   Мақола19954 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.228741

5. Elastic scattering of 52 MeV deuterons

   F. Hinterberger, G. Mairle, U. Schmidt-Rohr +2

   Мақола19684 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.286705

6. Direct nuclear reaction theories

   N. Austern

   Китоб19703 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.171496

7. Asymptotic normalization coefficients from the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Ne</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>20</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">He</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>,<i>d</i>)<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Na</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>21</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>reaction and astrophysical factor for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Ne</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>20</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>(<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:mi>γ</mml:mi></mml:mrow></mml:math>)<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Na</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>21</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>

   A. M. Mukhamedzhanov, P. Bém, V. Burjan +9

   МақолаNuclear physics research studiesPhysical Review C20063 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.171544

8. Comparaison des réactions (d, 3He) ET (d, t) sur quelques noyaux N = Z

   M. J. Gaillard, R. Bouché, L. Feuvrais +5

   Мақола19683 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.212691

9. RADII AND BINDING ENERGIES OF NUCLEI IN THE ALPHA-CLUSTER MODEL

   G. K. Nie

   МақолаNuclear physics research studiesModern Physics Letters A20072 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.552794

10. RADII AND BINDING ENERGIES OF NUCLEI IN THE ALPHA-CLUSTER MODEL

    G. K. Nie

    Мақола20062 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.552795

11. Сарлавҳасиз

    Бошқа1 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.552792

12. Сарлавҳасиз

    Бошқа1 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.552793