The accuracy of the predictions of the γ flux produced by a classical nova during the first hours after the outburst is limited by the uncertainties on several reaction rates, including the 18F(p,α)15O one. Better constraints on this reaction rate can be obtained by determining the spectroscopic properties of the compound nucleus 19Ne. This was achieved in a new inelastic scattering method using a 19Ne radioactive beam (produced by the GANIL-SPIRAL 1 facility) impinging onto a proton target. The experiment was performed at the VAMOS spectrometer. In this article the performances (excitation energy range covered and excitation energy resolution) and limitations of the new technique are discussed. Excitation energy resolution of σ = 33 keV and low background were obtained with this inverse kinematics method, which will allow extracting the spectroscopic properties of 19Ne.
|Publication status||Published - 31 Jan 2018|
|Event||Nuclear Physics in Astrophysics VII: 28th EPS Nuclear Physics Divisional Conference - The Royal York Hotel, York, United Kingdom|
Duration: 18 May 2015 → 22 May 2015
|Conference||Nuclear Physics in Astrophysics VII|
|Period||18/05/15 → 22/05/15|