Room-temperature reactions of the atomic cations Sr(+) and Rb(+) have been surveyed systematically with a variety of gases using an Inductively-Coupled Plasma/Selected-Ion Flow Tube (ICP/SIFT) tandem mass spectrometer. Rate coefficients and product distributions have been measured in He buffer gas at 0.35 Torr and 295 K for reactions of Sr(+) and Rb(+) with CH(3)F, CH(3)Cl, N(2)O, CO(2), CS(2), SF(6), D(2)O and NH(3). Rb(+) (s(0)) is seen to be quite inert with these molecules and reacts either slowly by molecule addition or not at all, while Sr(+) (s(1)) is much more reactive with all these 8 molecules, especially with CH(3)F, CH(3)Cl, N(2)O and SF(6). Sr(+) reacts with CH(3)F and SF(6) by F-atom transfer, with CH(3)Cl by Cl-atom transfer and with N(2)O by O-atom transfer, and the reaction rate coefficients are all quite high, k > or = 1.4x10(-11) cm(3) molecules(-1) s(-1). The extreme differences in reactivity with CH(3)F, SF(6), CH(3)Cl and N(2)O provide a chemical basis for the separation of isobaric interferences of (87)Rb(+) and (87)Sr(+) often encountered in ICP-MS. Among these four molecules, SF(6) exhibits the largest difference in reactivity, almost a factor of 10(4), and so is identified as the kinetically recommended reagent for the chemical resolution of the isobaric interference of (87)Rb(+) and (87)Sr(+).
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http://dx.doi.org/10.1016/j.aca.2008.03.057 | DOI Listing |
J Phys Chem A
February 2017
Department of Theoretical Chemistry and Amsterdam Center for Multiscale Modeling (ACMM), Vrije Universiteit Amsterdam, De Boelelaan 1083, 1081 HV Amsterdam, The Netherlands.
Fundamental principles that determine chemical reactivity and reaction mechanisms are the very foundation of chemistry and many related fields of science. Bimolecular nucleophilic substitutions (S2) are among the most common and therefore most important reaction types. In this report, we examine the trends in the S2 reactions with respect to increasing electronegativity of the reaction center by comparing the well-studied backside S2 Cl + CHCl with similar Cl substitutions on the isoelectronic series with the second period elements N, O, and F in place of C.
View Article and Find Full Text PDFAstrobiology
June 2016
1 Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts.
Unlabelled: Thousands of exoplanets are known to orbit nearby stars. Plans for the next generation of space-based and ground-based telescopes are fueling the anticipation that a precious few habitable planets can be identified in the coming decade. Even more highly anticipated is the chance to find signs of life on these habitable planets by way of biosignature gases.
View Article and Find Full Text PDFAstrobiology
March 2013
Harvard Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA.
We present model atmospheres for an Earth-like planet orbiting the entire grid of main sequence FGK stars with effective temperatures ranging from Teff=4250 K to Teff=7000 K in 250 K intervals. We have modeled the remotely detectable spectra of Earth-like planets for clear and cloudy atmospheres at the 1 AU equivalent distance from the VIS to IR (0.4 to 20 μm) to compare detectability of features in different wavelength ranges in accordance with the James Webb Space Telescope and future design concepts to characterize exo-Earths.
View Article and Find Full Text PDFJ Phys Chem A
June 2012
Department of Natural Sciences, University of Michigan-Dearborn, 4901 Evergreen Road, Dearborn, Michigan 48128, United States.
The rate constant of the reaction Cl + CF(3)CF═CH(2) (k(1)) has been measured relative to several reference species using the relative rate technique with either gas chromatographic analysis with flame-ionization detection (GC/FID) or Fourier transform infrared (FTIR) analysis. Cl atoms were generated by UV irradiation of Cl(2)/CF(3)CF═CH(2)/reference/N(2)/O(2) mixtures. At 300-400 K in the presence of >20 Torr O(2), k(1) = 1.
View Article and Find Full Text PDFPhys Chem Chem Phys
December 2011
Institut UTINAM UMR CNRS 6213, Université de Franche-Comté, 16 Route de Gray, 25030 Besançon cedex, France.
The case of symmetric tops CH(3)X (X = Br, Cl, F, …) perturbed by non-polar diatoms Y(2) (Y = N(2), O(2), …) is analysed from the viewpoint of theoretical collisional broadening of their rotational lines observed in atmospheric spectra. A semi-classical approach involving an exponential representation of the scattering operator and exact trajectories governed by the isotropic potential is presented. For the first time the active molecule is strictly treated as a symmetric top and the atom-atom interactions are included in the intermolecular potential model.
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