Institute of Chemistry, Edmund J. Safra Campus, Givat Ram, The Hebrew University of Jerusalem, Jerusalem 91904, Israel.
Langmuir. 2023 Feb 21;39(7):2838-2849. doi: 10.1021/acs.langmuir.2c03441. Epub 2023 Feb 10.
Mixtures of methanol and amorphous solid water (ASW) ices are observed in the interstellar medium (ISM), where they are subject to irradiation by UV photons and bombardment by charged particles. The charged particles, if at high enough density, induce a local electric field in the ice film that potentially affects the photochemistry of these ices. When CDOD@ASW ices grown at 38 K on a Ru(0001) substrate are irradiated by 193 nm (6.4 eV) photons, products such as HD, D, CO, and CO are formed in large abundances relative to the initial amount of CDOD. Other molecules such as DO, CD, acetaldehyde, and ethanol and/or dimethyl ether are also observed, but in smaller relative abundances. The reactivity cross sections range from (2.6 ± 0.3) × 10 to (3.8 ± 0.3) × 10 cm/photon. The main products are formed through two competing mechanisms: direct photodissociation of methanol and water and dissociative electron attachment (DEA) by photoelectrons ejected from the Ru(0001) substrate. An electric field of 2 × 10 V/m generated within the ASW film during Ne ions bombardment is apparently not strong enough to affect the relative abundances (selectivity) of the photochemical products observed in this study.
甲醇和非晶态水(ASW)冰的混合物在星际介质(ISM)中被观测到,它们会受到紫外线光子的辐照和带电粒子的轰击。如果带电粒子的密度足够高,它们会在冰膜中产生局部电场,这可能会影响这些冰的光化学反应。当 CDOD@ASW 冰在 Ru(0001)基底上于 38 K 生长并受到 193 nm(6.4 eV)光子的辐照时,会形成大量的 HD、D、CO 和 CO 等产物,相对于 CDOD 的初始量而言。还观察到其他分子,如 DO、CD、乙醛和乙醇和/或二甲醚,但相对丰度较小。反应截面范围为(2.6 ± 0.3)× 10 到(3.8 ± 0.3)× 10 cm/光子。主要产物是通过两种竞争机制形成的:甲醇和水的直接光解以及从 Ru(0001)基底中逐出的光电子的离化电子俘获(DEA)。在 Ne 离子轰击期间,在 ASW 膜内产生的 2×10 V/m 的电场显然不够强,无法影响本研究中观察到的光化学产物的相对丰度(选择性)。