First-principles modeling of sulfate incorporation and 34S/32S isotopic fractionation in different calcium carbonates

2014 ◽  
Vol 374-375 ◽  
pp. 84-91 ◽  
Author(s):  
Etienne Balan ◽  
Marc Blanchard ◽  
Carlos Pinilla ◽  
Michele Lazzeri
2019 ◽  
Vol 489 (1) ◽  
pp. 62-64 ◽  
Author(s):  
D. P. Krylov ◽  
A. B. Kuznetsov

Temperature relations of b-factors for 18O/16O substitutions in TiO2 polymorphs have been determined using the density functional theory (DFT): 1000lnbrt(18O/16O) = 6,93039x - 0,08158x2 + 0,00116x3 + 0,08305*P, 1000lnbant(18O/16O) = 7,34275x - 0,09906x2 + 0,00153x3 + 0,08027*P, 1000lnbbrk(18O/16O) = 7,19088x - 009157x2 + 0,00139x3 + 0,07601*P, x = 106/T(K)2, P - pressure (GPa). The relations can be applied for isotope thermometry if combined with -factors of coexisting phases.


2010 ◽  
Vol 74 (14) ◽  
pp. 3874-3882 ◽  
Author(s):  
Merlin Méheut ◽  
Michele Lazzeri ◽  
Etienne Balan ◽  
Francesco Mauri

2013 ◽  
Vol 13 (3) ◽  
pp. 1511-1520 ◽  
Author(s):  
J. A. Schmidt ◽  
M. S. Johnson ◽  
S. Hattori ◽  
N. Yoshida ◽  
S. Nanbu ◽  
...  

Abstract. The isotopic fractionation in OCS photolysis is studied theoretically from first principles. UV absorption cross sections for OCS, OC33S, OC34S, OC36S and O13CS are calculated using the time-depedent quantum mechanical formalism and a recently developed ab-initio description of the photodissociation of OCS which takes into account the lowest four singlet and lowest four triplet electronic states. The calculated isotopic fractionations as a function of wavelength are in good agreement with recent measurements by Hattori et al. (2011) and indicate that photolysis leads to only a small enrichment of 34S in the remaining OCS. The photodissociation dynamics provide strong evidence that the photolysis quantum yield is unity at all wavelengths for atmospheric UV excitation, for all isotopologues. A simple stratospheric model is constructed taking into account the main sink reactions of OCS and it is found that overall stratospheric removal slightly favors light OCS in constrast to the findings of Leung et al. (2002). These results show, based on isotopic considerations, that OCS is an acceptable source of background stratosperic sulfate aerosol in agreement with a recent model study of of Brühl et al. (2012). The 13C isotopic fractionation due to photolysis of OCS in the upper stratosphere is significant and will leave a clear signal in the remaining OCS making it a candidate for tracing using the ACE-FTS and MIPAS data sets.


2012 ◽  
Vol 319-320 ◽  
pp. 118-127 ◽  
Author(s):  
Marc Javoy ◽  
Etienne Balan ◽  
Merlin Méheut ◽  
Marc Blanchard ◽  
Michele Lazzeri

2011 ◽  
Vol 11 (17) ◽  
pp. 8965-8975 ◽  
Author(s):  
J. A. Schmidt ◽  
M. S. Johnson ◽  
R. Schinke

Abstract. For the first time, accurate first principles potential energy surfaces allow N2O cross sections and isotopic fractionation spectra to be derived that are in agreement with all available experimental data, extending our knowledge to a much broader range of conditions. Absorption spectra of rare N- and O-isotopologues (15N14N16O, 14N15N16O, 15N216O, 14N217O and 14N218O) calculated using wavepacket propagation are compared to the most abundant isotopologue (14N216O). The fractionation constants as a function of wavelength and temperature are in excellent agreement with experimental data. The study shows that excitations from the 3rd excited bending state, (0,3,0), and the first combination state, (1,1,0), are important for explaining the isotope effect at wavelengths longer than 210 nm. Only a small amount of the mass independent oxygen isotope anomaly observed in atmospheric N2O samples can be explained as arising from photolysis.


2014 ◽  
Vol 401 ◽  
pp. 33-37 ◽  
Author(s):  
Raffaella Demichelis ◽  
Paolo Raiteri ◽  
Julian D. Gale

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