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34 та иш

Иш: 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

    Мақола199930 иқтибос
    ABI

  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

    МақолаNuclear physics research studiesNuclear Physics A200624 иқтибос
    ABI

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

    C. M. Perey, F.G. Perey

    Мақола197614 иқтибос
    ABI

  4. Spectroscopic factors for the 1p shell

    S. Cohen, D. Kurath

    Мақола196712 иқтибос
    ABI

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

    F. C. Barker, T. Kajino

    Мақола199112 иқтибос
    ABI

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

    Pierre Descouvemont, Abderrahim Adahchour, Carmen Angulo +2

    Мақола200411 иқтибос
    ABI

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

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

    Мақола198010 иқтибос
    ABI

  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

    МақолаNuclear physics research studiesPhysics of Atomic Nuclei20089 иқтибос
    ABI

  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

    Мақола20039 иқтибос
    ABI

  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

    МақолаNuclear physics research studiesPhysics of Atomic Nuclei20078 иқтибос
    ABI

  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

    МақолаNuclear physics research studiesPhysical Review C20087 иқтибос
    ABI

  12. R-Matrix Theory of Nuclear Reactions

    A.M. Lane, R. G. Thomas

    Мақола19587 иқтибос
    ABI

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

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

    Мақола19937 иқтибос
    ABI

  14. How uncertain are solar neutrino predictions?

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

    Мақола19987 иқтибос
    ABI

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

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

    Мақола19897 иқтибос
    ABI

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

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

    Мақола20046 иқтибос
    ABI

  17. Сарлавҳасиз

    Бошқа6 иқтибос
    ABI

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

    John N. Bahcall, Marc H. Pinsonneault

    Мақола20046 иқтибос
    ABI

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

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

    Мақола19876 иқтибос
    ABI

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

    Uwe Schröder, Harry Becker, G. Bogaert +7

    Мақола19875 иқтибос
    ABI

  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

    Мақола20025 иқтибос
    ABI

  22. 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

    Мақола19784 иқтибос
    ABI

  23. 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
    ABI

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

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

    Мақола20044 иқтибос
    ABI

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

    C. Angulo, P. Descouvemont

    Мақола20012 иқтибос
    ABI