G. G. Rapisarda

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. Pole approximation validation in the study of the [sup 6]Li(d,α)[sup 4]He reaction20100 iqtibos
4. Indirect Study of the¹⁶O+¹⁶O Fusion Reaction Toward Stellar Energies by the Trojan Horse Method20160 iqtibos
5. Trojan Horse Method for the Oxygen-Burning Process Reactions20170 iqtibos
6. 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
7. Determination of the astrophysical factor of the ³He(α,γ)⁷Be down to zero energy using the asymptotic normalization coefficient method20230 iqtibos

Hammualliflar

1. G. Kiss7 ta umumiy asar2010–2023
2. M. La Cognata7 ta umumiy asar2010–2023
3. C. Spitaleri7 ta umumiy asar2010–2023
4. L. Lamia7 ta umumiy asar2010–2023
5. S. Romano7 ta umumiy asar2010–2023
6. А. Туміно7 ta umumiy asar2010–2023
7. S. B. Igamov6 ta umumiy asar2016–2023
8. P. Figuera6 ta umumiy asar2016–2023
9. G. L. Guardo6 ta umumiy asar2016–2023
10. I. Indelicato6 ta umumiy asar2016–2023

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