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Works cited by this work

70 works

Work: 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

  1. Interference effects in 12C(p, γ)13N and direct capture to unbound states

    C. Rolfs, R.E. Azuma

    Article19745 citations
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  2. Thermonuclear Reaction Rates

    William A. Fowler, Georgeanne R. Caughlan, Barbara A. Zimmerman

    Article19675 citations
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  3. Thermonuclear reaction rates V

    Georgeanne R. Caughlan, William A. Fowler

    Article19885 citations
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  4. The (d, n) reaction on 1p shell nuclei at Ed = 11.8 MeV

    G. S. Mutchler, D. Rendić, Donald E. Velkley +2

    Article19714 citations
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  5. Astrophysical S factor of 3H(α,γ) 7Li

    Uwe Schröder, A. Redder, C. Rolfs +5

    Article19874 citations
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  6. Untitled

    Other4 citations
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  7. Neutrino Astrophysics

    Hong‐Yee Chiu, John N. Bahcall

    Book19654 citations
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  8. Direct nuclear reaction theories

    N. Austern

    Book19703 citations
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  9. THE T(α,γ)Li<sup>7</sup> REACTION

    G. M. Griffiths, J. B. Warren, Richard A. Morrow +1

    Article19613 citations
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  10. Asymptotic normalization coefficients and astrophysical direct capture rates

    C. A. Gagliardi, A. Azhari, V. Burjan +7

    Article20023 citations
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  11. 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

    ABI
  12. Clusters as Subsystems in Light Nuclei

    V. I. Kukulin, V. G. Neudatchin, I. T. Obukhovski +1

    Chapter19833 citations
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