L. E. Marcucci

4 ta ish

National Institute for Nuclear Physics, Pisa Division

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. <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>α</mml:mi><mml:mo>+</mml:mo><mml:mi>d</mml:mi><mml:mo>→</mml:mo><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</mml:mn></mml:mmultiscripts><mml:mo>+</mml:mo><mml:mi>γ</mml:mi></mml:mrow></mml:math> astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>S</mml:mi></mml:math> factor and its implications for Big Bang nucleosynthesis

   Alessandro Grassi, G. Mangano, L. E. Marcucci +1

   MaqolaOAOchiq kirish20174 iqtibos

   ABIABI:AkademIndex/2026.other.191681

3. 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

4. Theoretical calculation of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:mi>p</mml:mi><mml:mo>−</mml:mo><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:mrow></mml:math> radiative capture reaction

   Alex Gnech, L. E. Marcucci

   MaqolaOAOchiq kirish20193 iqtibos

   ABIABI:AkademIndex/2026.other.197454