S. Cherubini

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. Few-body problems in nuclear astrophysics20050 iqtibos
4. Indirect techniques in nuclear astrophysics20060 iqtibos
5. Pole approximation validation in the study of the [sup 6]Li(d,α)[sup 4]He reaction20100 iqtibos
6. Indirect techniques in nuclear astrophysics20100 iqtibos
7. 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
8. Determination of the astrophysical factor of the ³He(α,γ)⁷Be down to zero energy using the asymptotic normalization coefficient method20230 iqtibos

Hammualliflar

1. C. Spitaleri8 ta umumiy asarSkelet yozuvlar: 32004–2023
2. S. Romano8 ta umumiy asarSkelet yozuvlar: 32004–2023
3. А. Туміно8 ta umumiy asarSkelet yozuvlar: 32004–2023
4. R. G. Pizzone7 ta umumiy asarSkelet yozuvlar: 32004–2023
5. A. M. Mukhamedzhanov7 ta umumiy asarSkelet yozuvlar: 12005–2023
6. R. E. Tribble7 ta umumiy asar2005–2023
7. M. La Cognata5 ta umumiy asarSkelet yozuvlar: 32004–2023
8. L. Lamia5 ta umumiy asarSkelet yozuvlar: 32004–2023
9. J. Mrázek5 ta umumiy asar2010–2023
10. G. Kiss5 ta umumiy asar2010–2023

Barcha hammualliflar →