Wong Natalie G K, Berenbeim Jacob A, Hawkridge Mathew, Matthews Edward, Dessent Caroline E H
Department of Chemistry, University of York, Heslington, York YO10 5DD, UK.
Phys Chem Chem Phys. 2019 Jul 3;21(26):14311-14321. doi: 10.1039/c8cp06794e.
Sunscreens provide vital protection against the photodamaging effects of UV radiation, however, many fundamental questions remain about the detailed mechanisms by which they dissipate UV energy. One such issue is the extent to which the pH environment of an organic sunscreen molecule alters its effectiveness, both in terms of ability to absorb UV radiation, and also its potential to photodegrade. Here, we use gas-phase laser photodissociation spectroscopy for the first time to measure the intrinsic UVA-UVC absorption spectra and associated photodegradation products of protonated and deprotonated oxybenzone, away from the complications of bulk mixtures. Our results reveal that protonation state has a dramatic effect on the absorption and photodissociation properties of this sunscreen. While the UV absorption profile of oxybenzone is only modestly affected by protonation across the range from 400-216 nm, deprotonated oxybenzone displays a significantly modified absorption spectrum, with very low photoabsorption between 370-330 nm. Protonated oxybenzone primarily photofragments by rupture of the bonds on either side of the central carbonyl group, producing cationic fragments with m/z 151 and 105. Additional lower mass photofragments (e.g. m/z 95 and 77) are also observed. The production spectra for the photofragments from protonated oxybenzone fall into two distinct categories, which we discuss in the context of different excited state decay pathways. For deprotonated oxybenzone, the major photofragments observed are m/z 211 and 212, which are associated with the ejection of methane and the methyl free radical from the parent ion, respectively. Implications for the suitability of oxybenzone in its protonated and deprotonated forms as an optimum sunscreen molecule are discussed.
防晒霜能有效抵御紫外线辐射的光损伤作用,然而,关于其消散紫外线能量的详细机制仍存在许多基本问题。其中一个问题是有机防晒分子的pH环境在多大程度上会改变其有效性,这既涉及吸收紫外线辐射的能力,也涉及其光降解的可能性。在此,我们首次使用气相激光光解离光谱法来测量质子化和去质子化氧苯酮的固有UVA - UVC吸收光谱以及相关的光降解产物,避免了本体混合物带来的复杂性。我们的结果表明,质子化状态对这种防晒霜的吸收和光解离特性有显著影响。虽然在400 - 216 nm范围内,质子化对氧苯酮的紫外线吸收曲线影响较小,但去质子化的氧苯酮显示出明显改变的吸收光谱,在370 - 330 nm之间光吸收非常低。质子化的氧苯酮主要通过中心羰基两侧的键断裂进行光碎片化,产生质荷比为151和105的阳离子碎片。还观察到了其他较低质量的光碎片(如质荷比为95和77)。质子化氧苯酮光碎片的产生光谱分为两个不同类别,我们将在不同激发态衰变途径的背景下进行讨论。对于去质子化的氧苯酮,观察到的主要光碎片是质荷比为211和212,它们分别与母体离子中甲烷和甲基自由基的逸出有关。本文讨论了质子化和去质子化形式的氧苯酮作为最佳防晒分子的适用性。