T. Szücs

10 ta ish

HUN-REN Institute for Nuclear Research

1. First Direct Measurement of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mrow><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">H</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow><mml:mo stretchy="false">(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mmultiscripts><mml:mrow><mml:mi>Li</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>6</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow></mml:mrow></mml:math>Cross Section at Big Bang Energies and the Primordial Lithium Problem

   M. Anders, D. Trezzi, R. Menegazzo +26

   MaqolaOAOchiq kirish20149 iqtibos

   ABIABI:AkademIndex/2026.other.191674

2. 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

3. Activation measurement of the reaction cross section at high energies

   C. Bordeanu, Gy. Gyürky, Z. Halász +6

   MaqolaOAOchiq kirish20136 iqtibos

   ABIABI:AkademIndex/2026.other.178218

4. Cross section of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>He</mml:mi><mml:mprescripts/><mml:none/><mml:mn>3</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>α</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> around the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:math> proton separation threshold

   T. Szücs, G. Kiss, Gy. Gyürky +3

   MaqolaOAOchiq kirish20196 iqtibos

   ABIABI:AkademIndex/2026.other.178253

5. 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

6. Constraining big bang lithium production with recent solar neutrino data

   M. P. Takács, D. Bemmerer, T. Szücs +1

   MaqolaOAOchiq kirish20155 iqtibos

   ABIABI:AkademIndex/2026.other.178216

7. Big Bang 6 Li nucleosynthesis studied deep underground (LUNA collaboration)

   D. Trezzi, M. Anders, M. Aliotta +34

   Maqola20175 iqtibos

   ABIABI:AkademIndex/2026.other.356325

8. Underground experimental study finds no evidence of low-energy resonance in the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><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

   D. Piatti, T. Chillery, R. Depalo +42

   MaqolaOAOchiq kirish20204 iqtibos

   ABIABI:AkademIndex/2026.other.197460

9. 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

10. 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