V. Zhaunerchyk
Stockholm University
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Featured researches published by V. Zhaunerchyk.
Journal of Chemical Physics | 2009
Brian A. Tom; V. Zhaunerchyk; Michael B. Wiczer; Andrew A. Mills; Kyle N. Crabtree; M. Kaminska; Wolf D. Geppert; M. Hamberg; Magnus af Ugglas; Erik Vigren; Wim J. van der Zande; Mats Larsson; Richard D. Thomas; Benjamin J. McCall
The determination of the dissociative recombination rate coefficient of H(3) (+) has had a turbulent history, but both experiment and theory have recently converged to a common value. Despite this convergence, it has not been clear if there should be a difference between the rate coefficients for ortho-H(3) (+) and para-H(3) (+). A difference has been predicted theoretically and could conceivably impact the ortho:para ratio of H(3) (+) in the diffuse interstellar medium, where H(3) (+) has been widely observed. We present the results of an experiment at the CRYRING ion storage ring in which we investigated the dissociative recombination of highly enriched ( approximately 83.6%) para-H(3) (+) using a supersonic expansion source that produced ions with T(rot) approximately 60-100 K. We observed an increase in the low energy recombination rate coefficient of the enriched para-H(3) (+) by a factor of approximately 1.25 in comparison to H(3) (+) produced from normal H(2) (ortho:para=3:1). The ratio of the rate coefficients of pure para-H(3) (+) to that of pure ortho-H(3) (+) is inferred to be approximately 2 at low collision energies; the corresponding ratio of the thermal rate coefficients is approximately 1.5 at electron temperatures from 60 to 1000 K. We conclude that this difference is unlikely to have an impact on the interstellar ortho:para ratio of H(3) (+).
The Astrophysical Journal | 2004
Wolf D. Geppert; A. Ehlerding; Fredrik Hellberg; J. Semaniak; Fabian Österdahl; M. Kaminska; A. Al-Khalili; V. Zhaunerchyk; Richard D. Thomas; M. af Ugglas; A. Källberg; Ansgar Simonsson; Mats Larsson
Branching ratios and absolute cross sections have been measured for the dissociative recombination of DCCCN+ and DCCCND+ using the CRYRING ion storage ring. In the case of DCCCN+ the dissociation y ...
Journal of Chemical Physics | 2005
Albert A. Viggiano; A. Ehlerding; Fredrik Hellberg; Richard D. Thomas; V. Zhaunerchyk; Wolf D. Geppert; Helene Montaigne; Mats Larsson; Magda Kaminska; Fabian Österdahl
Product branching ratios and thermal rate coefficients for the dissociative recombination of CO2+ have been measured in the cryogenic ion source ring ion storage ring. The rate constants were found to be 4.2×10−7(Te∕300)−0.75cm3s−1. The 300-K result is in agreement with previous flowing afterglow values and is somewhat smaller than a recent determination made at the Aarhas storage ring in Denmark (ASTRID) storage ring. The electron temperature dependence is, however, in good agreement with the ASTRID result of T−0.8. The present results show that only CO plus O are formed, other product branching ratios are zero within experimental error. This is in contradiction to the ASTRID results which show that 9% of the reactivity goes to C+O2. The new results show that the C+O2 channel does not need to be included in the models of the ionospheres of Venus and Mars.
Journal of Physics: Conference Series | 2005
Wolf D. Geppert; Richard D. Thomas; A. Ehlerding; Fredrik Hellberg; Fabian Österdahl; M. Hamberg; J. Semaniak; V. Zhaunerchyk; M. Kaminska; A. Källberg; A Paal; Mats Larsson
Cross sections and branching ratios for the dissociative recombination (DR) reactions of the astrophysically important ions HN2+, HCO+, DOCO+, and SO2+ at reactant kinetic energies from 1 to 1000 meV have been measured using the CRYRING ion storage ring facility at the Manne Siegbahn Laboratory, Stockholm University. Whereas the break-up of the N-N bond leading to NH + N is the major pathway in the DR of HN2+, the analogous reaction in HCO+ almost exclusively leads to H and CO. In the DR of both DOCO+ and SO2+ three-body break-up was observed. Inclusion of the newly measured branching ratios into a standard model on dark interstellar clouds leads to an improvement of the predictions of such models, especially concerning the abundances of nitrogen compounds. The impact of these newly found branching ratios and reaction rates on the chemistry of different astronomical environments like dark clouds, circumstellar envelopes and planetary ionospheres, is discussed.
Physical Chemistry Chemical Physics | 2008
Erik Vigren; M. Kaminska; M. Hamberg; V. Zhaunerchyk; Richard D. Thomas; Mathias Danielsson; J. Semaniak; Patrik U. Andersson; Mats Larsson; Wolf D. Geppert
The dissociative recombination of fully deuterated protonated acetonitrile, CD(3)CND(+), has been investigated at the CRYRING heavy ion storage ring, located at the Manne Siegbahn Laboratory, Stockholm, Sweden. Branching fractions were measured at approximately 0 eV relative collision energy between the ions and the electrons and in 65% of the DR events there was no rupture of bonds between heavy atoms. In the remaining 35%, one of the bonds between the heavy atoms was broken. The DR cross-section was measured between approximately 0 eV and 1 eV relative collision energy. In the energy region between 1 meV and 0.1 eV the cross section data were best fitted by the expression sigma = 7.37 x 10(-16) (E/eV)(-1.23) cm(2), whereas sigma = 4.12 x 10(-16) (E/eV)(-1.46) cm(2) was the best fit for the energy region between 0.1 and 1.0 eV. From the cross section a thermal rate coefficient of alpha(T) = 8.13 x 10(-7) (T/300)(-0.69) cm(3) s(-1) was deduced.
The Astrophysical Journal | 2005
H. Montaigne; Wolf D. Geppert; J. Semaniak; Fabian Österdahl; Fredrik Hellberg; Richard D. Thomas; M. af Ugglas; Helen Roberts; T. J. Millar; V. Zhaunerchyk; M. Kaminska; A. Al-Khalili; A. Källberg; Mats Larsson
Branching ratios and absolute cross sections have been measured for the dissociative recombination of HCS+ and OCS+ at the CRYRING ion storage ring. In the case of OCS+, the channel leading to CO + S (83%) dominates, whereas the other exoergic pathways leading to CS + O (14%) and C + SO (3%) are of lesser importance. In the case of HCS+, fracture of the C–S bond is predominant (81%), with the production of H + CS accounting for the remainder (19%). The cross section of the reaction could be fitted by the expressions σ = 1.41 × 10-15E(eV)-1.11 and 4.47 × 10-16E(eV)-1.14 cm2 for HCS+ and OCS+, respectively. The derived energy dependences of the thermal reaction rate coefficients can be fitted by k(T) = 9.7 × 10-7(T/300)-0.57 and 3.5 × 10-7(T/300)-0.62 cm3 s-1 for HCS+ and OCS+, respectively. We use these data to perform model calculations on the HCS+/CS abundance ratio in dark clouds and find that the models using the UMIST and Ohio State University databases have even more difficulty in accounting for the large observed ratio.
Molecular Physics | 2007
Mattias Hamberg; Wolf D. Geppert; Richard D. Thomas; V. Zhaunerchyk; Fabian Österdahl; A. Ehlerding; M. Kaminska; J. Semaniak; Magnus af Ugglas; A. Källberg; A. Paal; Ansgar Simonsson; Mats Larsson
Measurements of the cross-sections and branching ratios of the dissociative recombination of the ions CH2OH þ, CD2OD þ and CD2OD þ 2 have been performed at the CRYRING storage ring located in Stockholm, Sweden. Evaluation of the data yielded reaction rate coefficients of: 7.0 10 (T/300) 0.78 cmmol 1 s 1 for CH2OH; 7.5 10 (T/300) 0.70 cmmol 1 s 1 for CD2OD þ and 1.51 10 (T/300) 0.66 cmmol 1 s 1 for CD2OD2 . Calculation of the branching ratios for CH2OH þ and its deuterated isotopologue gave the following results for the DR reaction channels involving C–O bond fissure: H2OþCH (2.2%) and CH2þOH (5.5%) in the reaction of CH2OH þ as well as D2OþCD (5%) and CD2þOD (18%) for the dissociative recombination of CD2OD þ. The remainder of the reaction flux kept the C–O bond intact: 92% for CH2OH þ and 77% for CD2OD þ, respectively. Other recent measurements on the CH3OH þ 2 ion indicate dominating bond breaking between the heavy atoms, which is in contrast to this experiment. For CD2OD þ 2 CO-bond breaking was observed for 43% of the reaction flux.Measurements of the cross-sections and branching ratios of the dissociative recombination of the ions CH2OH+, CD2OD+ and CD2OD2+ have been performed at the CRYRING storage ring located in Stockholm, Sweden. Evaluation of the data yielded reaction rate coefficients of: 7.0 x 10-7( T/300) -0.78 cm3mol-1s -1 for CH2OH+; 7.5 x 10-7(T/300) -0.70 cm3 mol-1s-1 for CD2OD+ and 1.51 x 10-6(T/300)-0.66 cm3 mol-1s-1 for CD2OD2+. Calculation of the branching ratios for CH2OH+ and its deuterated isotopologue gave the following results for the DR reaction channels involving C-O bond fissure: H2O+CH (2.2%) and CH2+OH (5.5%) in the reaction of CH2OH+ as well as D2O+CD (5%) and CD2+OD (18%) for the dissociative recombination of CD2OD+. The remainder of the reaction flux kept the C-O bond intact: 92% for CH2OH+ and 77% for CD2OD+, respectively. Other recent measurements on the CH3OH2+ ion indicate dominating bond breaking between the heavy atoms which is conversely to this experiment. For CD2OD2+ CO-bond breaking was observed for 57% of the reaction flux.
The Astrophysical Journal | 2012
Erik Vigren; V. Zhaunerchyk; M. Hamberg; M. Kaminska; J. Semaniak; M. af Ugglas; Mats Larsson; Richard D. Thomas; Wolf D. Geppert
The dissociative recombination (DR) of N2H+ has been reinvestigated at the heavy ion storage ring CRYRING at the Manne Siegbahn Laboratory in Stockholm, Sweden. Thermal rate coefficients for electr ...
Astronomy and Astrophysics | 2010
M. Hamberg; F. Österdahl; Richard D. Thomas; V. Zhaunerchyk; Erik Vigren; M. Kaminska; M. af Ugglas; A. Källberg; Ansgar Simonsson; A. Paal; Mats Larsson; Wolf D. Geppert
Aims: Determination of branching fractions, cross sections and thermal rate coefficients for the dissociative recombination of CD3OCD2+ (0-0.3 eV) and (CD3)2OD+ (0-0.2 eV) at the low relative kinet ...
The Astrophysical Journal | 2009
Erik Vigren; M. Hamberg; V. Zhaunerchyk; M. Kaminska; Richard D. Thomas; Mats Larsson; T. J. Millar; Catherine Walsh; Wolf D. Geppert
Measurements on the dissociative recombination (DR) of protonated acrylonitrile, CH2CHCNH+, have been performed at the heavy ion storage ring CRYRING located in the Manne Siegbahn Laboratory in Sto ...