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• W1578324240 abstract "The ${}^{18}text{F}(p,ensuremath{alpha}){}^{15}$O reaction rate is crucial for understanding the final abundance of $^{18}mathrm{F}$ predicted by nova models. The $ensuremath{gamma}$-ray emission in the first few hours after a nova outburst is expected to be dominated by 511 keV annihilation photons from the decay of $^{18}mathrm{F}$, and so understanding its production can provide important constraints on the conditions during the outburst when compared with observations. Results are presented from the lowest-energy direct measurement to date, performed at the Isotope Separator and Accelerator radioactive beam facility at the TRIUMF laboratory, Canada. Cross section measurements at center-of-mass energies of 250, 330, 453, and 673 keV are obtained and the results compared to previous data and $R$-matrix calculations. The implications for the overall reaction rate in the context of nova explosions have been discussed." @default.
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• W1578324240 date "2011-04-12" @default.
• W1578324240 modified "2023-10-17" @default.
• W1578324240 title "Direct measurement of the<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mmultiscripts><mml:mi mathvariant=normal>F</mml:mi><mml:mprescripts /><mml:none /><mml:mrow><mml:mn>18</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mrow><mml:mi>p</mml:mi></mml:mrow></mml:math>,<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mrow><mml:mi>α</mml:mi></mml:mrow…" @default.
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• W1578324240 doi "https://doi.org/10.1103/physrevc.83.042801" @default.
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