H. Costantini

11 ta ish

National Institute for Nuclear Physics, Genoa

1. Solar fusion cross sections. II. The<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi><mml:mi>p</mml:mi></mml:math>chain and CNO cycles

   E. G. Adelberger, A. Garcı́a, R. G. H. Robertson +44

   MaqolaOAOchiq kirish201116 iqtibos

   ABIABI:AkademIndex/2026.other.178227

2. 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

3. 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

4. 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

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

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

   MaqolaOAOchiq kirish20045 iqtibos

   ABIABI:AkademIndex/2026.other.228744

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

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

   Maqola20175 iqtibos

   ABIABI:AkademIndex/2026.other.356325

7. <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

8. 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

9. AZURE: An<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>R</mml:mi></mml:mrow></mml:math>-matrix code for nuclear astrophysics

   R.E. Azuma, E. Uberseder, E. C. Simpson +8

   Maqola20103 iqtibos

   ABIABI:AkademIndex/2026.other.417223

10. 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

11. Electron screening effect in the reactions 3He(d, p)4He and d(3He, p)4He

    F. Raiola, Vincenzo Roca, H. Costantini +28

    Maqola20012 iqtibos

    ABIABI:AkademIndex/2026.other.365806