Ushbu ish iqtibos qilgan ishlar

34 ta ish

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

1. A compilation of charged-particle induced thermonuclear reaction rates

   C. Angulo, M. Arnould, M. Rayet +25

   MaqolaOAOchiq kirish199932 iqtibos

   ABIABI:AkademIndex/2026.other.171531

2. 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

   S. B. Igamov, R. Yarmukhamedov

   MaqolaNuclear physics research studiesNuclear Physics A200627 iqtibos

   ABIABI:AkademIndex/2006.article.000039

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

   C. M. Perey, F.G. Perey

   Maqola197617 iqtibos

   ABIABI:AkademIndex/2026.other.212678

4. Spectroscopic factors for the 1p shell

   S. Cohen, D. Kurath

   Maqola196716 iqtibos

   ABIABI:AkademIndex/2026.other.171512

5. Compilation and R-matrix analysis of Big Bang nuclear reaction rates

   Pierre Descouvemont, Abderrahim Adahchour, Carmen Angulo +2

   MaqolaOAOchiq kirish200412 iqtibos

   ABIABI:AkademIndex/2026.other.171526

6. The 12C(a,g)16O Cross Section at Low Energies

   F. C. Barker, T. Kajino

   MaqolaOAOchiq kirish199112 iqtibos

   ABIABI:AkademIndex/2026.other.171593

7. Global optical model potential for elastic deuteron scattering from 12 to 90 MeV

   W. W. Daehnick, J.D. Childs, Zoran Vrcelj

   Maqola198010 iqtibos

   ABIABI:AkademIndex/2026.other.212683

8. 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

   MaqolaNuclear physics research studiesPhysics of Atomic Nuclei20089 iqtibos

   ABIABI:AkademIndex/2008.article.000051

9. 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>14</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">N</mml:mi><mml:mo>+</mml:mo><mml:mrow><mml:msup><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mn>15</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">O</mml:mi></mml:math>and the astrophysical<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>S</mml:mi></mml:math>factor for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>14</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">N</mml:mi><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mrow><mml:msup><mml:mrow><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn>15</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">O</mml:mi></mml:math>

   A. M. Mukhamedzhanov, P. Bém, B. A. Brown +10

   Maqola20039 iqtibos

   ABIABI:AkademIndex/2026.other.178250

10. Influence of the three-body coulomb effects on the values of asymptotic normalization coefficients (nuclear vertex constants) of astrophysical interest extracted from the modified DWBA approach for the peripheral proton-transfer reactions

    S. B. Igamov, M. S. Nadirbekov, R. Yarmukhamedov

    MaqolaNuclear physics research studiesPhysics of Atomic Nuclei20078 iqtibos

    ABIABI:AkademIndex/2026.other.171578

11. 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

    N. Burtebaev, S. B. Igamov, R. J. Peterson +2

    MaqolaNuclear physics research studiesPhysical Review C20087 iqtibos

    ABIABI:AkademIndex/2008.article.000043

12. R-Matrix Theory of Nuclear Reactions

    A.M. Lane, R. G. Thomas

    Maqola19587 iqtibos

    ABIABI:AkademIndex/2026.other.003933

13. Alpha scattering and capture reactions in the<i>A</i>=7 system at low energies

    P. Mohr, H. Abele, R. Zwiebel +6

    MaqolaOAOchiq kirish19937 iqtibos

    ABIABI:AkademIndex/2026.other.171519

14. How uncertain are solar neutrino predictions?

    John N. Bahcall, Sarbani Basu, Marc H. Pinsonneault

    MaqolaOAOchiq kirish19987 iqtibos

    ABIABI:AkademIndex/2026.other.171532

15. <i>Cauldrons in the Cosmos</i>

    C. Rolfs, W.S. Rodney, Donald D. Clayton

    Maqola19897 iqtibos

    ABIABI:AkademIndex/2026.other.171584

16. Sarlavhasiz

    Boshqa7 iqtibos

    ABIABI:AkademIndex/2026.other.171589

17. Compilation and R-matrix analysis of Big Bang nuclear reaction rates

    Descouvemont, Pierre, Adahchour, Abderrahim, Angulo, Carmen +2

    MaqolaOAOchiq kirish20046 iqtibos

    ABIABI:AkademIndex/2026.other.171556

18. What Do We (Not) Know Theoretically about Solar Neutrino Fluxes?

    John N. Bahcall, Marc H. Pinsonneault

    MaqolaOAOchiq kirish20046 iqtibos

    ABIABI:AkademIndex/2026.other.178232

19. Simple optical model treatment of the elastic 3He scattering

    H.J. Trost, P. Lezoch, U. Strohbusch

    Maqola19876 iqtibos

    ABIABI:AkademIndex/2026.other.212682

20. Stellar reaction rate of 14N(p, γ)15O and hydrogen burning in massive stars

    Uwe Schröder, Harry Becker, G. Bogaert +7

    Maqola19875 iqtibos

    ABIABI:AkademIndex/2026.other.171588

21. <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>14</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">N</mml:mi><mml:mrow><mml:msup><mml:mrow><mml:mo>(</mml:mo></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">He</mml:mi><mml:mrow><mml:msup><mml:mrow><mml:mo>,</mml:mo><mml:mi>d</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn>15</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">O</mml:mi></mml:math>as a probe of direct capture in the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>14</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">N</mml:mi><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mrow><mml:msup><mml:mrow><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn>15</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">O</mml:mi></mml:math>reaction

    P. F. Bertone, A. E. Champagne, M. Boswell +4

    MaqolaOAOchiq kirish20025 iqtibos

    ABIABI:AkademIndex/2026.other.228743

22. Astrophysical S-factor of 14N(p,γ)15O

    A. Formicola, G. Imbriani, H. Costantini +29

    MaqolaOAOchiq kirish20045 iqtibos

    ABIABI:AkademIndex/2026.other.228744

23. Effects of channel and potential radiative transitions in the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>17</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow><mml:mo>(</mml:mo><mml:mi>γ</mml:mi><mml:mo>,</mml:mo><mml:mi> </mml:mi><mml:mrow><mml:msub><mml:mrow><mml:mi>n</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:mrow><mml:mo>)</mml:mo><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>16</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow></mml:math>reaction

    R. J. Holt, H. E. Jackson, R. M. Laszewski +2

    Maqola19784 iqtibos

    ABIABI:AkademIndex/2026.other.171571

24. 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

    Maqola19954 iqtibos

    ABIABI:AkademIndex/2026.other.228741

25. The 14N(p,)15O low-energy -factor

    C. Angulo, P. Descouvemont

    Maqola20012 iqtibos

    ABIABI:AkademIndex/2026.other.228742