I. Wiedenhöver

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. High-Seniority Intrinsic and Collective Structures in $^174$Hf and $^175$Hf20010 iqtibos
4. Yrast structure of neutron-rich<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Ti</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>53</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>20050 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. A. M. Mukhamedzhanov4 ta umumiy asar2020–2023
2. J. Mrázek4 ta umumiy asar2020–2023
3. S. B. Igamov4 ta umumiy asar2020–2023
4. R. Yarmukhamedov4 ta umumiy asar2020–2023
5. R. E. Tribble4 ta umumiy asar2020–2023
6. G. Kiss4 ta umumiy asar2020–2023
7. M. La Cognata4 ta umumiy asar2020–2023
8. C. Spitaleri4 ta umumiy asar2020–2023
9. L. T. Baby4 ta umumiy asar2020–2023
10. S. Cherubini4 ta umumiy asar2020–2023

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