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He-accreting white dwarfs with sub-Chandrasekhar mass are revisited. Theimpact of the use of an extended reaction network on the predicted energyproduction and characteristics of the detonating layers is studied. It is shownthat the considered scenario can be the site of an $\alpha$p-process combinedwith a p-process and with a variant of the rp-process we refer to as thepn-process. We define the conditions under which the derived distribution ofthe abundances of the p-nuclides in the ejecta, including the puzzling light Moand Ru isotopes, mimics the solar-system one.Comment: 4 pages; A&A Letters in pres

He-detonation in sub-Chandrasekhar CO white dwarfs: A new insight into energetics and $\mathsf{{\vec p}}$-process nucleosynthesis