Kiviniemi Tiina, Pettersson Mika, Khriachtchev Leonid, Räsänen Markku, Runeberg Nino
Department of Chemistry, University of Jyvaskyla, Finland.
J Chem Phys. 2004 Jul 22;121(4):1839-48. doi: 10.1063/1.1766008.
IR spectroscopy, laser induced fluorescence (LIF), and thermoluminescence (TL) measurements have been combined to monitor trapping, thermal mobility, and reactions of oxygen atoms in solid xenon. HXeO and O(3) have been used as IR active species that probe the reactions of oxygen atoms. N(2)O and H(2)O have been used as precursors for oxygen atoms by photolysis at 193 nm. Upon annealing of matrices after photolysis, ozone forms at two different temperatures: at 18-24 K from close O ...O(2) pairs and at approximately 27 K due to global mobility of oxygen atoms. HXeO forms at approximately 30 K reliably at higher temperature than ozone. Both LIF and TL show activation of oxygen atoms around 30 K. Irradiation at 240 nm after the photolysis at 193 nm depletes the oxygen atom emission at 750 nm and reduces the amount of HXeO generated in subsequent annealing. Part of the 750 nm emission can be regenerated by 266 nm and this process increases the yield of HXeO in annealing as well. Thus, we connect oxygen atoms emitting at 750 nm with annealing-induced formation of HXeO radicals. Ab initio calculations at the CCSD(T)/cc-pV5Z level show that XeO (1(1)Sigma(+)) is much more deeply bound [D(e) = 1.62 eV for XeO --> Xe+O((1)D)] than previous calculations have predicted. Taking into account the interactions with the medium in an approximate way, it is estimated that XeO (1(1)Sigma(+)) has a similar energy in solid xenon as compared with interstitially trapped O((3)P) suggesting that both possibly coexist in a low temperature solid. Taking into account the computational results and the behavior of HXeO and O(3) in annealing and irradiations, it is suggested that HXeO may be formed from singlet oxygen atoms which are trapped in a solid as XeO (1(1)Sigma(+)).
红外光谱、激光诱导荧光(LIF)和热释光(TL)测量已被结合起来,以监测固态氙中氧原子的俘获、热迁移率和反应。HXeO和O(3)已被用作探测氧原子反应的红外活性物种。N(2)O和H(2)O已被用作通过193nm光解产生氧原子的前驱体。光解后对基质进行退火处理时,臭氧在两个不同温度下形成:在18 - 24K时由紧密的O...O(2)对形成,在约27K时由于氧原子的整体迁移形成。HXeO在约30K时可靠地形成,温度高于臭氧。LIF和TL都显示氧原子在约30K时被激活。在193nm光解后用240nm照射会耗尽750nm处的氧原子发射,并减少后续退火中产生的HXeO量。750nm发射的一部分可以通过266nm再生,并且这个过程也会增加退火中HXeO的产率。因此,我们将在750nm处发射的氧原子与退火诱导的HXeO自由基形成联系起来。在CCSD(T)/cc - pV5Z水平上的从头算计算表明,XeO(1(1)Σ(+))的束缚要比先前计算预测的深得多[对于XeO→Xe + O((1)D),D(e)=1.62eV]。以近似方式考虑与介质的相互作用后,估计XeO(1(1)Σ(+))在固态氙中的能量与间隙俘获的O((3)P)相似,这表明两者可能在低温固体中共存。考虑到计算结果以及HXeO和O(3)在退火和照射中的行为,有人提出HXeO可能由作为XeO(1(1)Σ(+))被困在固体中的单线态氧原子形成。