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The 12 C +12 C reaction is just one of the most crucial responses in the evolution of substantial stars. The cross-section and the astrophysical S factor were calculated making use of the possibility of AW95 and the new optimized capacity. The new enhanced possibility in replicating the combination random sample and astrophysical S aspect is very successful at reduced energies, the barrier and maximum in S aspect shows up in this exact same energy range and is in good agreement with the experimental outcomes.
Source link: https://ui.adsabs.harvard.edu/abs/2021NewA...8901649M/abstract
The measured transparency was constant with no Q2 dependence, as much as proton momenta of 8. 5 GeV/ c, ruling out the quantum chromodynamics effect of shade openness at the gauged Q2 scales in special responses.
Source link: https://ui.adsabs.harvard.edu/abs/2021PhRvL.126h2301B/abstract
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