G. Imbriani

13 ta ish

National Institute for Nuclear Physics, Naples Unit

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. 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

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. <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

7. Monte Carlo uncertainty of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">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 mathvariant="normal">Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:mrow></mml:math>reaction rate

   R. J. deBoer, J. Görres, K. Smith +6

   Maqola20144 iqtibos

   ABIABI:AkademIndex/2026.other.178245

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. 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

10. The Chemical Composition of White Dwarfs as a Test of Convective Efficiency during Core Helium Burning

    O. Straniero, I. Domı́nguez, G. Imbriani +1

    MaqolaOAOchiq kirish20032 iqtibos

    ABIABI:AkademIndex/2026.other.207473

11. The¹²C(α, γ)¹⁶O Reaction Rate and the Evolution of Stars in the Mass Range 0.8 ≤ <i>M</i>/<i>M</i>_⊙ ≤ 25

    G. Imbriani, Marco Limongi, L. Gialanella +3

    MaqolaOAOchiq kirish20012 iqtibos

    ABIABI:AkademIndex/2026.other.207477

12. 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

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

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

    Maqola20062 iqtibos

    ABIABI:AkademIndex/2026.other.365811