Gy. Gyürky

18 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. Stellar and Primordial Nucleosynthesis of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:math>: Measurement of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi>He</mml:mi><mml:mprescripts/><mml:none/><mml:mn>3</mml:mn></mml:mmultiscripts><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:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:math>

   A. Di Leva, L. Gialanella, R. Kunz +16

   MaqolaOAOchiq kirish20097 iqtibos

   ABIABI:AkademIndex/2026.other.178219

4. 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

5. 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 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>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</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">Be</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>7</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>reaction measured at low energy via detection of prompt and delayed γ rays

   F. Confortola, D. Bemmerer, H. Costantini +28

   MaqolaOAOchiq kirish20076 iqtibos

   ABIABI:AkademIndex/2026.other.178220

6. 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

7. Activation Measurement of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi>He</mml:mi><mml:mprescripts/><mml:none/><mml:mn>3</mml:mn></mml:mmultiscripts><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:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:math>Cross Section at Low Energy

   D. Bemmerer, F. Confortola, H. Costantini +27

   MaqolaOAOchiq kirish20066 iqtibos

   ABIABI:AkademIndex/2026.other.178257

8. 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

9. Astrophysical S-factor of 14N(p,γ)15O

   A. Formicola, G. Imbriani, H. Costantini +29

   MaqolaOAOchiq kirish20045 iqtibos

   ABIABI:AkademIndex/2026.other.228744

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

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

    Maqola20175 iqtibos

    ABIABI:AkademIndex/2026.other.356325

11. <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>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</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">Be</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>7</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>cross section at low energies

    Gy. Gyürky, F. Confortola, H. Costantini +27

    MaqolaOAOchiq kirish20074 iqtibos

    ABIABI:AkademIndex/2026.other.178221

12. 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

13. First measurement of the d(p,γ)3He cross section down to the solar Gamow peak

    C. Casella, H. Costantini, A. Lemut +33

    MaqolaOAOchiq kirish20023 iqtibos

    ABIABI:AkademIndex/2026.other.228814

14. S-factor of 14N(p,γ)15O at astrophysical energies⋆

    G. Imbriani, H. Costantini, A. Formicola +31

    MaqolaOAOchiq kirish20052 iqtibos

    ABIABI:AkademIndex/2026.other.228747

15. Enhanced electron screening in d(d, p)t for deuterated metals: a possible classical explanation

    C. Bonomo, G. Fiorentini, Zsolt Fülöp +9

    Maqola20032 iqtibos

    ABIABI:AkademIndex/2026.other.365781

16. Enhanced d(d,p)t fusion reaction in metals

    F. Raiola, B. Burchard, Zs. Fülöp +22

    Maqola20062 iqtibos

    ABIABI:AkademIndex/2026.other.365811

17. 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

18. 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