Study of the <sup>18</sup>Ne(α,p)<sup>21</sup>Na reaction with ANASEN and its significance in the breakout from the hot CNO cycle
ORAL
Abstract
18Ne(α,p)21Na reaction is one of the reactions providing a pathway for breakout from the hot CNO cycles to the rp process in x-ray bursts.The actual conditions under which the breakout occurs depend critically on the thermonuclear reaction rate. This rate has not been sufficiently determined yet over stellar temperatures on x-ray burst conditions. We study the direct 18Ne(α,p)21Na reaction with the Array for Nuclear Astrophysics Studies with Exotic Nuclei (ANASEN), using a helium gas target and an 18Ne radioactive beam. ANASEN is an active gas target detection system with the ability to measure excitation function using a single beam energy while the beam slows down in the target gas. Utilizing also the particle tracking capability of the experimental array the center of mass energy can be reconstructed at the reaction point. Heavy recoil detection for coincidence with the light particle is also attempted for the first time in the ANASEN detector. Preliminary results will be presented for the experiment performed in reaction energies relevant to those in the breakout leading to an x-ray burst.
*Supported by the US NSF MRI program Grant no. PHY-0820941, NSF Grant no. PHY-1712953.
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Presenters
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Maria Anastasiou
- Florida State Univ