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Measurement of <sup>19</sup>Ne spectroscopic properties via a new method of inelastic scattering to study novae

F. R. H. DU BOULAYGANIL CaenB. BastinGANIL CaenF. de Oliveira SantosGANIL CaenT. DavinsonUniversity of EdinburghA. LemassonGANIL CaenP. UjićINS Vinca BelgradeJ. MrázekNuclear Physics Institute of RezÁ. M. Sánchez-BenítezGANIL CaenE. TraykovGANIL CaenD. RamosUniversidade de Santiago de CompostelaL. AchouriLPC CaenL. AcostaUniversity of HuelvaC. BorceaIFIN-HH BucharestM. CiemałaInstitute of Nuclear Physics KrakòwP. DelahayeGANIL CaenA. EstradéUniversity of EdinburghG. de FranceGANIL CaenJ. GrinyerGANIL CaenB. JacquotGANIL CaenO. KamalouGANIL CaenA. M. LairdUniversity of YorkV. MargerinUniversity of EdinburghG. Marquínez-DuránUniversity of HuelvaF. NegoiţăIFIN-HH BucharestM. RejmundGANIL CaenC. Rodríguez–TajesGANIL CaenF. RotaruIFIN-HH BucharestC. SchmittGANIL CaenN. de SérévilleIPN OrsayO. SorlinGANIL CaenM. StănoiuIFIN-HH BucharestJ. C. ThomasGANIL CaenP. J. WoodsUniversity of Edinburgh
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Abstract

The accuracy of the predictions of the γ flux produced by a classical nova during the first&#13;\nhours after the outburst is limited by the uncertainties on several reaction rates, including the&#13;\n18F(p,α)15O one. Better constraints on this reaction rate can be obtained by determining the&#13;\nspectroscopic properties of the compound nucleus 19Ne. This was achieved in a new inelastic&#13;\nscattering method using a 19Ne radioactive beam (produced by the GANIL-SPIRAL 1 facility)&#13;\nimpinging onto a proton target. The experiment was performed at the VAMOS spectrometer. In&#13;\nthis article the performances (excitation energy range covered and excitation energy resolution)&#13;\nand limitations of the new technique are discussed. Excitation energy resolution of σ=33&#13;\nkeV and low background were obtained with this inverse kinematics method, which will allow&#13;\nextracting the spectroscopic properties of 19Ne.

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