G. L. Guardo

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

Hammualliflar

1. M. La Cognata6 ta umumiy asarSkelet yozuvlar: 12016–2023
2. S. B. Igamov6 ta umumiy asar2016–2023
3. G. Kiss6 ta umumiy asar2016–2023
4. C. Spitaleri6 ta umumiy asar2016–2023
5. P. Figuera6 ta umumiy asar2016–2023
6. I. Indelicato6 ta umumiy asar2016–2023
7. L. Lamia6 ta umumiy asar2016–2023
8. М. Латтуада6 ta umumiy asar2016–2023
9. G. G. Rapisarda6 ta umumiy asar2016–2023
10. S. Romano6 ta umumiy asar2016–2023

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