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1. Measurements of ¹⁸ O ¹⁸ O and ¹⁷ O ¹⁸ O in the atmosphere and the role of isotope-exchange reactions: ¹⁸ O ¹⁸ O AND ¹⁷ O ¹⁸ O IN THE ATMOSPHERE

   https://doi.org/10.1029/2012JD017992  

   Yeung, Laurence Y.; Young, Edward D.; Schauble, Edwin A. (September 2012, Journal of Geophysical Research: Atmospheres)
2. The Role of Ozone Vibrational Resonances in the Isotope Exchange Reaction ¹⁶ O ¹⁶ O + ¹⁸ O → ¹⁸ O ¹⁶ O + ¹⁶ O: The Time-Dependent Picture

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   Yuen, Chi Hong; Lapierre, David; Gatti, Fabien; Kokoouline, Viatcheslav; Tyuterev, Vladimir G. (August 2019, The Journal of Physical Chemistry A)
3. Nuclear Structures of ¹⁷ O and Time-dependent Sensitivity of the Weak s -process to the ¹⁶ O( n , γ ) ¹⁷ O Rate

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4. Spectroscopic and Reactivity Comparisons of a Pair of bTAML Complexes with Fe ^V ═O and Fe ^IV ═O Units

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   Pattanayak, Santanu; Jasniewski, Andrew J.; Rana, Atanu; Draksharapu, Apparao; Singh, Kundan K.; Weitz, Andrew; Hendrich, Michael; Que, Lawrence; Dey, Abhishek; Sen Gupta, Sayam (June 2017, Inorganic Chemistry)
5. Atmospheric Chemistry of HOHg ^(II) O ^• Mimics That of a Hydroxyl Radical

   https://doi.org/10.1021/acs.jpca.3c04159  

   Hewa_Edirappulige, Darshi T; Kirby, Ilena J; Beckett, Camille K; Dibble, Theodore S (October 2023, The Journal of Physical Chemistry A)

   HOHg(II)O•, formed from HOHg(I)• + O3, is a key intermediate in OH-initiated oxidation of Hg(0) in the atmosphere. As no experimental data is available for HOHg(II)O•, we use computational chemistry (CCSD(T)//M06-2X/AVTZ) to characterize its reactions with atmospheric trace gases (NO, NO2, CH4, C2H4, CH2O and CO). In summary, HOHg(II)O•, like the analogous BrHg(II)O• radical, largely mimics the reactivity of •OH in reactions with NOx, alkanes, alkenes, and aldehydes. The rate constant for its reaction with methane (HOHg(II)O• + CH4 → Hg(II)(OH)2 + •CH3) is about four times higher than that of •OH at 298 K. All these reactions maintain mercury as Hg(II), except for HOHg(II)O• + CO → HOHg(I)• + CO2. Considering only the six reactions studied here, we find that reduction by CO dominates the fate of HOHg(II)O• (79-93%) in many air masses (in the stratosphere and at ground level in rural, marine, and polluted urban regions) with only modest competition from HOHg(II)O• + CH4 (<15%). We expect that this work will help global modeling of atmospheric mercury chemistry. 

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