<ul><li>Researchers achieved a milestone in nuclear astrophysics by measuring ^12C+^12C fusion at 2.22 MeV.</li><li>The fusion process plays a crucial role in stellar evolution and explosive astrophysical events.</li><li>The experiment utilized a high-intensity carbon beam on HOPG target for increased sensitivity.</li><li>A sophisticated detection system enabled real-time tracking of fusion particle emissions.</li><li>The study focused on ground-state alpha emission and attained unprecedented sensitivity levels.</li><li>Experimental data aligned with theoretical predictions for fusion at sub-barrier energies.</li><li>Significant radiation damage to the target surface impacted fusion yields during prolonged irradiation.</li><li>Corrective measures were applied to interpret data accurately amid target degradation effects.</li><li>The research sheds light on carbon ignition in massive stars and its implications on stellar evolution.</li><li>The methodology sets a new standard for nuclear astrophysics, enabling robust particle identification.</li></ul>

Investigating the 12C+12C Fusion Reaction at Astrophysical Energies with HOPG Targets

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