20-24 September 2021
Africa/Johannesburg timezone
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Resonances in 11C above 10B+p threshold using thick target in inverse kinematics

23 Sep 2021, 15:30
2h
Gather.Town

Gather.Town

Poster Nuclear Astrophysics Poster Session 2

Speaker

Gurpreet Kaur

Description

The resonance structure in 11C is important to understand 7Be(α,γ)11C reaction in the pp-chain of Sun and for the 10B(p,α)7Be reaction as the contamination of the candidate of aneutronic fusion reaction 11B(p,2α) 4 He. Above the proton threshold, there are discrepancies in the excitation energies and lack of spin-assignment for the resonances in 11C nucleus. For this, an elastic scattering experiment of 10B+p was conducted and the R-matrix calculations are performed for the inverse kinematics data using the code Azure2 [1]. The resonant parameters such as the energy, spin-parity Jπ , and the proton-decay partial width are extracted and a comparison is performed with the results obtained from direct kinematic data [2]. Prior to this, similar calculations were performed for the reaction 12C+p [3,4] where the resonance structure is well established.
References:
[1] R. E. Azuma, E. Uberseder, E. C. Simpson, C. R. Brune, H. Costantini, R. J. de Boer, J. Görres, M. Heil, P. J. LeBlanc, C. Ugalde, and M. Wiescher. Phys. Rev. C 81, 045805 (2010).
[2] M. Chiari, L. Giuntini, P. Mandò, and N. Taccetti, Nucl. Instrum. Methods Phys. Res., Sect. B 184, 309 (2001).
[3] S. Sambi et al., Eur. Phys. J. A 51 (2015).
[4] H.O. Meyer, G.R. Plattner, I. Sick, Z. Phys. A 279, 41 (1976).

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