S. Hayakawa

Eng koʻp iqtibos qilingan asarlar

1. Indirect determination of the astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>S</mml:mi></mml:math> factor for the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</mml:mn></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> reaction using the asymptotic normalization coefficient method20218 iqtibos
2. Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method20205 iqtibos
3. Trojan Horse Method for the Oxygen-Burning Process Reactions20170 iqtibos
4. Determination of the ³He(<i>α</i>, <i>γ</i>)⁷Be and ⁶Li(<i>p</i>, <i>γ</i>)⁷Be astrophysical factors down to zero energy using the asymptotic normalization coefficients20230 iqtibos
5. Determination of the astrophysical factor of the ³He(α,γ)⁷Be down to zero energy using the asymptotic normalization coefficient method20230 iqtibos

Hammualliflar

1. S. B. Igamov5 ta umumiy asar2017–2023
2. G. Kiss5 ta umumiy asar2017–2023
3. M. La Cognata5 ta umumiy asar2017–2023
4. C. Spitaleri5 ta umumiy asar2017–2023
5. P. Figuera5 ta umumiy asar2017–2023
6. G. L. Guardo5 ta umumiy asar2017–2023
7. I. Indelicato5 ta umumiy asar2017–2023
8. L. Lamia5 ta umumiy asar2017–2023
9. М. Латтуада5 ta umumiy asar2017–2023
10. G. G. Rapisarda5 ta umumiy asar2017–2023

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