|
100 | 100 | [Lin2003a] I.V. Tokmakov, L.V. Moskaleva, D.V. Paschenko, M.C. Lin, J. Phys. Chem. A, 2003, 107(7), 1066-1076, doi: 10.1021/jp022024t |
101 | 101 | [Lin2003b] R.S. Zhu, M.C. Lin, J. Chem. Phys., 2003, 119, 10667, doi: 10.1063/1.1619373 |
102 | 102 | [Lin2003c] Z.F. Xu, M.C. Lin, Int. J. Chem. Kin., 2003, 35(5), 184-190, doi: 10.1002/kin.10115 |
| 103 | +[Lin2003d] R.S. Zhu, M.C. Lin, J. Chem. Phys., 2003, 119(20), 10667-10677, doi: 10.1063/1.1619373 |
103 | 104 | [Lin2004] Z.F. Xu, M.C. Lin, Int. J. Chem. Kin., 2004, 36(4), 205-215, doi: 10.1002/kin.10178 |
104 | 105 | [Lin2005a] R.S. Zhu, M.C. Lin, Int. J. Chem. Kin., 2005, 37(10), 593-598, doi: 10.1002/kin.20066 |
105 | 106 | [Lin2005b] R.S. Zhu, M.C. Lin, Ab initio study on the oxidation of NCN by O and HO radicals: Prediction of the total rate constant and product branching ratios, in: 6th International Conference of Chemical Kinetics, NIST, Gaithersberg, MD, 2005 |
|
4896 | 4897 | Optimized and characterized the stationary points of the PESs with the CCSD method (Detailed in Table 1). |
4897 | 4898 | """, |
4898 | 4899 | ) |
| 4900 | + |
| 4901 | +entry( |
| 4902 | + index = 275, |
| 4903 | + label = 'NO + HO2 <=> HNO3', |
| 4904 | + kinetics = Lindemann( |
| 4905 | + arrheniusHigh = Arrhenius(A=(2.85e+15, 'cm^3/(mol*s)'), n=-0.82, Ea=(-41.7, 'cal/mol'), |
| 4906 | + T0=(1, 'K'), Tmin=(200, 'K'), Tmax=(2000, 'K')), |
| 4907 | + arrheniusLow = Arrhenius(A=(1.20e+42, 'cm^6/(mol^2*s)'), n=-8.8, Ea=(3117.9, 'cal/mol'), |
| 4908 | + T0=(1, 'K'), Tmin=(200, 'K'), Tmax=(2000, 'K'))), |
| 4909 | + elementary_high_p = False, |
| 4910 | + shortDesc = u"""[Lin2003d]""", |
| 4911 | + longDesc = |
| 4912 | +u""" |
| 4913 | +Calculated at the G2(CC)//B3LYP/6-311+G(3df,2p) level of theory using RRKM. |
| 4914 | +He was used as the 3rd body collider in these computations. |
| 4915 | +""", |
| 4916 | +) |
| 4917 | + |
| 4918 | +entry( |
| 4919 | + index = 276, |
| 4920 | + label = 'NO + HO2 <=> HOONO', |
| 4921 | + kinetics = Lindemann( |
| 4922 | + arrheniusHigh = Arrhenius(A=(1.03e+14, 'cm^3/(mol*s)'), n=-0.24, Ea=(-198.7, 'cal/mol'), |
| 4923 | + T0=(1, 'K'), Tmin=(200, 'K'), Tmax=(2000, 'K')), |
| 4924 | + arrheniusLow = Arrhenius(A=(1.14e+50, 'cm^6/(mol^2*s)'), n=-12.3, Ea=(5136.9, 'cal/mol'), |
| 4925 | + T0=(1, 'K'), Tmin=(200, 'K'), Tmax=(2000, 'K'))), |
| 4926 | + elementary_high_p = False, |
| 4927 | + shortDesc = u"""[Lin2003d]""", |
| 4928 | + longDesc = |
| 4929 | +u""" |
| 4930 | +Calculated at the G2(CC)//B3LYP/6-311+G(3df,2p) level of theory using RRKM. |
| 4931 | +He was used as the 3rd body collider in these computations. |
4899 | 4932 | """, |
4900 | 4933 | ) |
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