G. D’Agata

4 ta ish

Nuclear Physics Institute of the Czech Academy of Sciences, 250 68 Řež, Czech Republic

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 method

   G. Kiss, M. La Cognata, R. Yarmukhamedov +38

   MaqolaNuclear physics research studiesPhysical review. C20217 iqtibos

   ABIABI:AkademIndex/openalex/2021.article.000211

2. Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method

   G. Kiss, M. La Cognata, C. Spitaleri +38

   MaqolaNuclear physics research studiesPhysics Letters B20205 iqtibos

   ABIABI:AkademIndex/openalex/2020.article.000135

3. 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 coefficients

   M. La Cognata, G. Kiss, R. Yarmukhamedov +38

   MaqolaNuclear physics research studiesEPJ Web of Conferences20230 iqtibos

   ABIABI:AkademIndex/openalex/2023.article.005771

4. Determination of the astrophysical factor of the ³He(α,γ)⁷Be down to zero energy using the asymptotic normalization coefficient method

   M. La Cognata, G. Kiss, R. Yarmukhamedov +38

   MaqolaNuclear physics research studiesJournal of Physics Conference Series20230 iqtibos

   ABIABI:AkademIndex/openalex/2023.article.010700