R. G. Pizzone

12 ta ish

Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Sud

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

   MaqolaOAOchiq kirishNuclear physics research studiesPhysical review. C20218 iqtibos

   ABIABI:AkademIndex/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

   MaqolaOAOchiq kirishNuclear physics research studiesPhysics Letters B20205 iqtibos

   ABIABI:AkademIndex/2020.article.000135

3. Indirect Techniques in Nuclear Astrophysics. Asymptotic Normalization Coefficient and Trojan Horse

   A. M. Mukhamedzhanov, L. D. Blokhintsev, S. Brown +18

   MaqolaOAOchiq kirish20065 iqtibos

   ABIABI:AkademIndex/2026.other.198868

4. New astrophysical<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>S</mml:mi></mml:mrow></mml:math>factor for the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">N</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>15</mml:mn></mml:mrow></mml:mmultiscripts></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mo stretchy="false">(</mml:mo><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>16</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>reaction via the asymptotic normalization coefficient (ANC) method

   A. M. Mukhamedzhanov, P. Bém, V. Burjan +17

   Maqola20082 iqtibos

   ABIABI:AkademIndex/2026.other.178228

5. Validity test of the “Trojan horse” method applied to the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>6</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">Li</mml:mi><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>α</mml:mi><mml:mrow><mml:msup><mml:mrow><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">He</mml:mi></mml:math>reaction

   А. Туміно, C. Spitaleri, A. Di Pietro +9

   Maqola20032 iqtibos

   ABIABI:AkademIndex/2026.other.352394

6. Bare-nucleus astrophysical factor of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">He</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>d</mml:mi><mml:mo>,</mml:mo><mml:mi>p</mml:mi></mml:mrow></mml:math>)<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">He</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>4</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>reaction via the “Trojan horse” method

   M. La Cognata, C. Spitaleri, А. Туміно +10

   Maqola20052 iqtibos

   ABIABI:AkademIndex/2026.other.352400

7. The<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>11</mml:mn></mml:mrow></mml:mmultiscripts><mml:mrow><mml:mo>(</mml:mo><mml:mrow><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>α</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:mrow><mml:mo>)</mml:mo></mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>8</mml:mn></mml:mmultiscripts></mml:mrow></mml:math>reaction at sub-Coulomb energies via the Trojan-horse method

   C. Spitaleri, L. Lamia, А. Туміно +11

   Maqola20042 iqtibos

   ABIABI:AkademIndex/2026.other.352405

8. Indirect techniques in nuclear astrophysics

   A. M. Mukhamedzhanov, L. D. Blokhintsev, B. A. Brown +14

   MaqolaOAOchiq kirishNuclear physics research studiesThe European Physical Journal A20060 iqtibos

   ABIABI:AkademIndex/2006.article.000074

9. Pole approximation validation in the study of the [sup 6]Li(d,α)[sup 4]He reaction

   R. G. Pizzone, C. Spitaleri, L. Lamia +17

   MaqolaSuperconducting Materials and ApplicationsAIP conference proceedings20100 iqtibos

   ABIABI:AkademIndex/2010.article.000370

10. Indirect techniques in nuclear astrophysics

    A. M. Mukhamedzhanov, L. D. Blokhintsev, B. A. Brown +14

    BobNuclear physics research studies20100 iqtibos

    ABIABI:AkademIndex/2010.chapter.000026

11. 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

    MaqolaOAOchiq kirishNuclear physics research studiesEPJ Web of Conferences20230 iqtibos

    ABIABI:AkademIndex/2023.article.005771

12. 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

    MaqolaOAOchiq kirishNuclear physics research studiesJournal of Physics Conference Series20230 iqtibos

    ABIABI:AkademIndex/2023.article.010700