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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.
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.
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