2004A&A...420..405G

In this paper we present the results of new experiments on ion irradiation of water ice performed on thin films to study the synthesis of the hydrogen peroxide molecule and discuss the possibility of detecting it in icy mantles on interstellar grains. The used experimental technique has been in situ infrared spectroscopy. We have irradiated thin films (i.e. the ice thickness was smaller than the penetration depth of the used ion) with three different ions, namely 200keV of H⁺ and He⁺ and 400 keV of Ar⁺⁺. The experiments were carried out at temperatures of 16 and 77K. We have found that hydrogen peroxide is produced by all of the different ions at both temperatures. The detection of such a molecule has been possible from the study of its infrared feature centered at about 2850/cm (3.5µm). The obtained results also show that the produced H₂O₂/H₂O(%) ratio is greater for the heaviest ion (∼6% for the case of Ar⁺⁺) and that H⁺ is the ion that produces the smallest quantity (∼1%). These upper limits in the production of hydrogen peroxide constrain the quantity of H₂O₂ that can be formed after bombardment by cosmic particles on icy mantles of grains in the interstellar medium.