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10988 Phys. Chem. Chem. Phys., 2010, 12, 10988–10995 This journal is c the Owner Societies 2010
Kinetics of thermoneutral intermolecular hydrogen migration in alkyl
radicalsw
Artur Ratkiewicz,a Barbara Bankiewicza and Thanh N. Truong*b
Received 20th April 2010, Accepted 23rd June 2010
DOI: 10.1039/c0cp00293c
High pressure limits of thermal rate constants of intramolecular hydrogen migrations, particularly
1,3 to 1,6 H-shift in propyl, butyl, pentyl and hexyl radicals, respectively, were calculated using
the canonical variational transition state theory (CVT) with a multi-dimensional small-curvature
tunneling (SCT) correction over the temperature range of 300–3000 K. The CCSD(T)/cc-pVDZ//
BH&HLYP/cc-pVDZ method was used to provide necessary potential energy surface
information. Rate constants for these reactions were used to extrapolate rate constants for
reactions of larger alkyls where experimental data are available using the Reaction Class
Transition State Theory (RC-TST). Excellent agreement with experimental data confirms the
validity of the RC-TST methodology and the accuracy of the calculated kinetic data in this study.
1. Introduction
The isomerization via intramolecular hydrogen atom migration,
also known as hydrogen-shift, forms an important class of alkyl
and alkenyl radical reactions. It has long been known that these
reactions are of importance in various complex reaction systems
such as combustion of hydrocarbons.1–5 The formation of some
products in such systems can be explained only in terms of
isomerization. Hydrogen shift reactions were also found to play
a significant role in determining product distribution in the last
stage of paraffin pyrolyses. Furthermore, radical isomerization
appears to compete in hydrocarbon oxidation systems with radical
decomposition and can be quite often encountered in the
postulation of mechanism of the processes involving radical
intermediates. Determination of the thermal rate coefficients of
these isomerization reactions is a prerequisite for the modeling of
combustion systems such as engines and furnaces operating
with hydrocarbon fuels. In spite of the latest experimental
achievements,6,7 relatively little information is currently available
for the kinetics of intramolecular hydrogen transfer reactions.
This is because direct measurements of the rate constants of
isomerization are difficult due to competing reactions in general.
Furthermore, for thermoneutral reactions, product and reactant
are identical, measuring the relative concentrations of reactants
and products is only possible via isotope labeling and is often
difficult. To the best of our knowledge, no direct experimental rate
data are available for these reactions to date.
There are a number of theoretical studies on the activation
energies and geometries of the transition states of H shift reactions
in alkyl radicals. Jitariu et al.8 studied in detail 1,2 to 1,5
isomerizations of 1-pentyl radical. Threshold energies, bottleneck
properties and the canonical variational transition state theory
(CVT) with multi-dimensional small-curvature tunneling (SCT)
rates for selected reactions were reported. Viskolcz et al.9,10
calculated the ab initio activation barriers and the ring strain
energies of the 1,2 to 1,5 H-atom transfer reactions in ethyl,
propyl, butyl, pentyl, and 2-methylhexyl radicals, respectively.
Pressure-dependent thermal rate constants were calculated for
2-methylhexyl radical. The authors showed that the barrier height
decreases as the number of atoms in the ring of the cyclic
transition structure increases. A similar conclusion was derived
by Curran et al.3,4 in their series of proposed hydrocarbon
combustion mechanisms. The authors approximated the activation
energies for isomerization reactions in terms of the number of
atoms in the transition state ring structure (including the transferring
H atom) and the type of carbon atom that the transferring
H atom originally binds to. Matheu et al.11 developed a set of
generic rules to estimate high pressure kinetic parameters of
intramolecular hydrogen shifts (from 1,2 to 1,6) in alkyl
radicals. These rules were derived from the results of DFT
quantum chemistry and TST calculations, for the simplest
reaction in the reaction class. Subsequent rate rules in
the family used the same A and n parameters in the
ATnexp(�Eactivation/RT) rate expression. Such a practice
assumed that the neutral H shift for the primary hydrocarbon is
sufficient to capture the dominant entropic effects, namely the
internal rotor gain and loss in this type of reactions. Since the
thermoneutral hydrogen migrations are the simplest reactions in
their reaction classes, these processes can serve as reference
reactions to investigate all processes within their perspective
classes. For this reason, more accurate kinetic parameters are
needed for the four reactions, from 1,3 to 1,6 H shift, namely:
CCC� 2 C�CC (R1)
CCCC� 2 C�CCC (R2)
CCCCC� 2 C�CCCC (R3)
CCCCCC� 2 C�CCCCC (R4)
a Chemistry Institute, University of Bialystok, Hurtowa 1, 15-399Bialystok, Poland
bHenry Eyring Center for Theoretical Chemistry, Department ofChemistry, University of Utah, 315 S. 1400 E. Rm. 2020,Salt Lake City, Utah 84112, USA. E-mail: [email protected]
w Electronic supplementary information (ESI) available: Themolecular and frequency data of reagents, products and transitionstates for reactions R1-R8, potential energy data along the MEP forreactions R1-R4, high pressure limits of rate constants for reactionsR1-R4 calculated with POLYRATE, and RC-TST factors and highpressure limits of rate constants for reactions R5-R8. See DOI:10.1039/c0cp00293c
PAPER www.rsc.org/pccp | Physical Chemistry Chemical Physics
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CView Article Online / Journal Homepage / Table of Contents for this issue
This journal is c the Owner Societies 2010 Phys. Chem. Chem. Phys., 2010, 12, 10988–10995 10989
In this study, the high pressure limits of thermal rate constants
for the reactions (R1)–(R4) were computed, using the canonical
variational transition state theory augmented with multi-
dimensional semi classical tunneling correction (CVT/SCT), with
potential energy surface calculated at a sufficiently accurate level
of theory. Among these four reaction classes, the 1,4 H-shift class
with the reference reaction (R2) were considered previously.12 In
this study, however, we present a more accurate rate expression
for the reference (R2) reaction.
2. Methodology
All the electronic structure calculations were carried out using
the GAUSSIAN 03 suite of programs.13 Since a hybrid non-
local Density Functional Theory (DFT), particularly Becke’s
half-and-half (BH&H) non-local exchange and
Lee–Yang–Parr (LYP) non-local correlation functionals, has
previously been found to be sufficiently accurate for predicting
the transition state properties,14–22 geometries of reactants,
transition states, and products were optimized at the
BH&HLYP level of theory with Dunning’s correlation-
consistent polarized valence double-zeta basis set [3s2p1d/2s1p],
denoted as cc-pVDZ,23,24 which is sufficient to capture the
physical change along the reaction coordinate for this type of
reaction. In particular, in our previous study,12 for the (R2)
reaction the BH&HLYP/cc-pVDZ method predicts geometries
close to those from the QCISD/cc-pVDZ level of theory for
the reactant and transition state, with the largest difference of
0.014 A. Similarly for frequencies, the average absolute
difference is about 32 cm�1 between those from the
BH&HLYP/cc-pVDZ and QCISD/cc-pVDZ calculations.
This leads to the insignificant (i.e. less than 0.05 kcal mol�1)
differences in the total ZPE’s of the reactant and transition
state for these two levels of theory. For this reason,
all geometry optimizations and frequency calculations were
performed at the BH&HLYP/cc-pVDZ level of theory.
Normal mode analysis was performed at each stationary
point to ensure its characteristics, i.e. stable structure has zero
imaginary vibrational frequency, whereas transition state (TS)
structure has one imaginary vibrational frequency, whose
mode corresponds to the reaction coordinate of the reaction
being considered. The minimum energy path (MEP) is also
obtained at the BH&HLYP/cc-pVDZ level using the
Gonzalez–Schlegel method25 in the mass weighted Cartesian
coordinates, with a step size of 0.01 (amu)12 bohr. In addition,
force constants at 300 points along the MEP were determined
to ensure convergence of the Small Curvature Tunneling
calculations. However, since the MEP is symmetric, thus
actual calculations were only done for 150 points on the
reactant side. The points were chosen based on the curvatures
of the MEP, and the geometrical parameters as functions of
the reaction coordinate according to our auto-focusing
technique.26 Energetic information along the MEP is further
refined by single-point energy CCSD(T)/cc-pVDZ calculations.
These energies, combined with the BH&HLYP/cc-pVDZ
geometries and frequencies, were then used for rate constant
calculations. Utility software tools were used to compose these
PES data for rate calculations and are available from the
authors upon request.27
High-pressure limits of thermal rate constants were calculated
using both the classical Transition State Theory28 (TST)28 with
the 1D Eckart tunneling, and the Canonical Variational
Transition State Theory (CVT)28 with the Small Curvature
Tunneling (SCT)28 methods, for the temperature range of
300–3000 K. To model vibrations transverse to the reaction
path, we used curvilinear coordinates based on bond stretches,
valence angle bends, and bond torsions from the
POLYRATE29 program. The 1D Eckart transmission coefficients
and partition functions were obtained with the TheRate,
available at the Computational Science and Engineering
Online (CSEO) website.30 The overall rotations were treated
classically and vibrations were treated quantum mechanically
within the harmonic approximation except for the modes
corresponding to the internal rotations of the CH2 and CH3
groups, which were treated as the hindered rotations (HR)
using the method of Ayala and Schlegel.31 In our previous
studies (for example, see ref. 12, 19, 20, and 22), this
methodology was found to be accurate by direct comparison
of our calculated results with experimental data available. The
reaction symmetry number of 3 was used to account for the
number of symmetrically equivalent reaction paths.
3. Results and discussion
3.1 Stationary points
It is known that intramolecular hydrogen migration proceeds
through formation of a cyclic transition structure.3,9,32 The
formation of a strained ring leads to a high reaction barrier.
The optimized transition state structures for all reference
reactions are shown in Fig. 1. The optimized geometries,
frequencies, zero point energies for reagents and transition states
of these reactions are available in the ESIw (Tables S1–S9).
From these geometries, ring strain at the transition state
increases from (R4) to (R1). Since in the more strained ring
more energy is needed for its formation, the barrier for
intramolecular atom transfer is expected to increase when ring
size decreases.
The classical barrier heights of the reference reactions
(R1)–(R4), calculated at various levels of theory with the
inclusion of ZPE corrections, are listed in Table 1. Comparisons
on the performance of different levels of theory enable the
selection of the most cost effective method for generating
potential energy surface information along the MEP for
CVT/SCT rate calculations.
Amongst different correlated methods considered here, the
compound CBS-QB333 model chemistry is expected to be the
most accurate and has been validated for its ability to predict
accurate hydrogen shift barriers.34,35 CBS-QB3 barrier heights
are 42.1, 24.2, 15.4 and 12.8 kcal mol�1 for the reactions
(R1)–(R4), respectively, and are used as reference points for
determining accuracy of other methods. Mean Absolute
Deviation (MAD) of barrier heights calculated with a given
method from the CBS-QB3 value is also given in Table 1.
CCSD(T)/cc-pVDZ//BH&HLYP/cc-pVDZ was found to have
the smallest MAD of 0.7 kcal mol�1. The performance of the
DFT methods is slightly worse, however it is still acceptable.
This fact is consistent with our previous work,17–20 DFT
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methods give rather accurate results, comparable to those
obtained with more expensive MO-based correlation methods.
Due to spin contamination, larger errors were found for the
MPn (n = 2,4) methods. Consequently, CCSD(T)/cc-pVDZ//
BH&HLYP/cc-pVDZ method is used to provide energetic
information for rate calculations.
As shown in Table 1 the largest barrier was found for the
1,3 H-shift and the lowest for the 1,6 H-shift. In agreement
with the expectation and the previous findings,9,10 the barrier
heights increase as the size of the ring in the transition state
decreases. Fig. 2 shows the classical, Vc, and vibrationally
adiabatic ground state, VGa , potential energy curves along the
MEP for the four title reactions. Total zero-point energies of
the reactants and transition states and the imaginary frequencies
at the transition states are listed in Table 2. The other potential
energy surface data are available in the ESIw (Tables S19–S22).ZPE corrections lower the classical barrier heights about
2 kcal mol�1, which corresponds to 5–15% of the total barrier
Fig. 1 Optimized, at the BH&HLYP/cc-pVDZ level of theory, geometries (distances in A and angles in degrees) of the transition states of the
reactions: C�CC - CCC�, C�CCC - CCCC�, C�CCCC - CCCCC�, and C�CCCCC - CCCCCC�.
Table 1 Calculated barrier heights and reaction energies for the C�CC2 CCC�, C�CCC2 CCCC�, C�CCCC2 CCCCC� and C�CCCCC2CCCCCC� reactions (numbers are in kcal mol�1). Zero-point energy corrections were included
Level of theory
DVGa for reaction
Mean absolutedeviation fromCBS-QB3 resultsaC�CC - CCC� C�CCC - CCCC� C�CCCC- CCCCC�
C�CCCCC-CCCCCC�
B3LYP/cc-pVDZ 38.711 23.111 15.311 10.5 2.2B3LYP/cc-pVTZ 39.6 23.1 15.1 12.2 1.2BH&HLYP/cc-pVDZ 43.3 26.9 17.8 14.4 2.2BH&HLYP/cc-pVTZ 44.2 27.9 19.1 15.8 3.1CCSD(T)/cc-pVDZ//BH&HLYP/cc-pVDZ 41.1 24.8 16.2 13.2 0.7QCISD/cc-pVDZ//BH&HLYP/cc-pVDZ 42.5 29.7 17.8 14.6 2.5MP2/cc-pVDZ//BH&HLYP/cc-pVDZ 42.0 8.1 16.7 13.5 4.8MP2/cc-pVTZ//BH&HLYP/cc-pVDZ 41.3 9.5 16.8 14.1 4.6MP4/cc-pVDZ//BH&HLYP/cc-pVDZ 42.6 7.4 16.5 13.4 4.8MP4/cc-pVTZ//BH&HLYP/cc-pVDZ 42.2 8.7 — — 7.8CBS-QB3 42.1 24.2 15.4 12.8 —MP2/6-311G**//HF/6-31G*9 43.1 26.4 19.1 — 2.4
a MAD ¼PjbarrierCBS�QB3�barrier for specific methodj
number of barriers calculated
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height. In consistence with the trend in the barrier height, the
imaginary frequencies decrease as the size of the transition
state ring increases. In addition, the positions of the maxima of
the ground-state adiabatic potential energy curves VGa are very
close to the corresponding transition states for all reactions.
This suggests the re-crossing effect would be small for these
reactions.
3.2 Rate constants
The high pressure limits of rate constants of the four titled
H-shift reactions studied were calculated using the Canonical
Variational Transition State Theory (CVT) with the Small
Curvature Tunneling (SCT) and Ayala–Schlegel31 hindered
rotations treatment (HR), over a wide range of temperature
from 300 to 3000 K. The final CVT/SCT/HR rate constants
for reactions (R1)–(R4) are plotted in Fig. 3. For practical
applications, the predicted rates were fitted by least-squares
analysis as given below:
kC�CC$CCC�
¼4:71�10�71T25:836 expð�3897:78=TÞ 300K�To700K
5:91�106T1:938 expð�18716:81=TÞ 700K�To3000K½s�1�
(
ð1Þ
kC�CCC$CCCC� ¼1:187�102�T3:042�exp �8826:73T
� �½s�1�;
ð2Þ
Fig. 2 Potential energy curves along the reaction coordinates of the reactions: C�CC - CCC�, C�CCC - CCCC�, C�CCCC - CCCCC� and
C�CCCCC - CCCCCC�. VGa is the vibrationally adiabatic ground state potential curve and VC is the classical adiabatic ground state potential curve.
Table 2 Calculated total zero point energies for reactants and transition states and imaginary frequencies of the C�CC 2 CCC�, C�CCC 2CCCC�, C�CCCC 2 CCCCC� and C�CCCCC 2 CCCCCC� reactions
Reaction Reactant ZPE/kcal mol�1 Transition state ZPE/kcal mol�1 Imaginary frequency/i cm�1
C�CC 2 CCC� 56.8 54.0 2285.2C�CCC 2 CCCC� 75.3 73.3 2073.5C�CCCC 2 CCCCC� 94.0 91.8 1925.0C�CCCCC 2 CCCCCC� 112.3 110.3 1881.8
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kC�CCCC$CCCCC� ¼2:51�105�T1:886�exp �5312:82T
� �½s�1�;
ð3Þ
kC�CCCCC$CCCCCC� ¼2:49�106�T1:6037�exp �4527:82T
� �½s�1�;
ð4Þ
The CVT/HR, TST/HR, and TST/Eckart/HR rate constants
are also plotted for the sake of comparison. Numeric values of
all the rates, used to prepare Fig. 3, are available in the ESIw(Tables S23–S26). The Eckart and SCT transmission coefficients
are listed in Table 3. It is well known that tunneling is significant
for hydrogen transfer reactions at lower temperatures. For all the
reactions investigated, the magnitude of SCT transmission
coefficients confirms this expectation as illustrated by the
differences between CVT/SCT/HR and CVT/HR curves shown
in Fig. 3. At T = 300 K, the SCT transmission coefficients are
105, 364, 39, and 18 for (R1)–(R4), respectively. Eckart
coefficients are much larger than SCT values particularly at low
temperatures. It is known34,36,37 that 1D Eckart function often
yields the potential width too narrow compared to the real ones
and thus leads to an overestimation of the tunneling coefficients.
Tunneling effects become less important when T > 1000 K. On
the other hand, not much difference between the TST and CVT
rates was found. This indicates the re-crossing effects are small as
mentioned earlier.
Fig. 3 Arrhenius plots of the calculated rate constants for the C�CC - CCC�, C�CCC - CCCC�, C�CCCC - CCCCC�, and C�CCCCC -
CCCCCC reactions along with those available in the literature. Since, for all four reactions, TST/HR and CVT/HR rates are almost the same, the
corresponding curves coincide and are difficult to resolve.
Table 3 Calculated transmission coefficients for the C�CC2 CCC� , C�CCC2 CCCC�, C�CCCC2 CCCCC� and C�CCCCC2 CCCCCC�
reactions. The third column for each reaction shows the ratio of the Eckart and SCT tunneling coefficients
Temperature/K
C�CC 2 CCC� C�CCC 2 CCCC� C�CCCC 2 CCCCC� C�CCCCC 2 CCCCCC�
Eckart SCT Eckart/SCT Eckart SCT Eckart/SCT Eckart SCT Eckart/SCT Eckart SCT Eckart/SCT
300 5 053 000 136 417 37.1 4686 364.0 12.9 223.1 38.5 5.8 98.9 17.7 5.6400 360.7 128.3 2.8 34.6 21.7 1.6 12.9 7.0 1.8 10.0 5.1 2.0500 15.6 11.6 1.4 7.0 6.5 1.1 4.7 3.3 1.4 4.2 2.8 1.51000 1.9 1.6 1.2 1.7 1.5 1.1 1.6 1.2 1.3 1.6 1.2 1.32000 1.3 1.1 1.2 1.2 1.1 1.1 1.2 1.0 1.2 1.2 1.0 1.23000 1.2 1.0 1.1 1.1 1.0 1.1 1.1 1.0 1.2 1.1 1.0 1.2
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4. Comparisons with literature data
The only kinetic data available for reactions (R1)–(R3) in the
NIST database38 are based on the B3LYP/cc-pVDZ calculations
and Transition State Theory performed by Matheu et al.11 In
these calculations, barrier heights were adjusted on a basis of
the value of the reference reaction and the relative heats of
reaction. Tunneling corrections were not included. Except for
the 1,5 H-shift (R3) reaction, where the rate data of Matheu
et al. agree well with our results, for the other two reactions,
1,3 and 1,4 H-shift reactions, their predicted data are too small
compared to our most accurate CVT/SCT/HR data. For
lower temperatures, the differences are noticeable. Since in
the present study, multidimensional tunneling and hindered
rotation corrections were included and thus rate constants are
expected to be more accurate.
Experimental data are available for the following H-shift
reactions:
C�CCCCC 2 CC�CCCC (1,5 H-shift) (R5)
C�CCCCC 2 CCC�CCC (1,4 H-shift) (R6)
C�CCCCCCC 2 CCC�CCCCC (1,6 H-shift) (R7)
C�CCCCCCC 2 CCCC�CCCC (1,5 H-shift) (R8)
among other H migrations in hexyl and octyl radicals done by
Tsang and co-workers.6,7 The experiments were performed in
a single pulse shock tube at temperatures in the 850–1000 K
range. High-pressure rate constants have been derived over
700–1900 K range with an uncertainty factor of less than 2.
The value of a given rate constant, k, could lie between
km/f and km � f, where km is the reported value and f is an
uncertainty factor.
To make direct comparisons with these experimental data,
rate constants for reactions (R5)–(R8) were extrapolated from
those of (R2)–(R4) using as the reference reactions within the
Reaction Class Transition State Theory (RC-TST) methodology.17
Within the RC-TST framework, the high pressure limit of the
rate constant of an arbitrary reaction (denoted as ka) in a
given reaction class is proportional to the rate constant of a
reference reaction of that class, kr:
ka(T) = f(T) � kr(T) (5)
The key idea of the RC-TST method is to factor f(T) into
different components under the TST framework:
f(T) = fs � fk(T) � fQ(T) � fV(T) � fHR(T) (6)
where fs, fk, fQ, fV and fHR are the symmetry number,
tunneling, partition function, potential energy and hindered
rotations factors, respectively. These factors are simply the
ratios of the corresponding components in the TST expression
for the two reactions:
fs ¼sasr
ð7Þ
fkðTÞ ¼kaðTÞkrðTÞ
ð8Þ
fQðTÞ ¼Qaa ðTÞ
FRa ðTÞ
� �Qar ðTÞ
FRr ðTÞ
� � ¼Qaa ðTÞ
Qar ðTÞ
� �FRa ðTÞ
FRr ðTÞ
� � ð9Þ
fVðTÞ ¼ exp �ðDVaa � DVa
r ÞkBT
� �¼ exp �DDVa
kBT
� �ð10Þ
fHRðTÞ ¼cHR;aðTÞcHR;rðTÞ
ð11Þ
where k(T) is the transmission coefficient accounting for the
quantummechanical tunneling effects; s is the reaction symmetry
number; Qa and FR are the total partition functions (per unit
volume) of the transition state and reactants, respectively;
DVa is the classical reaction barrier height; cHR symbolizes
the correction to the total partition function due to the
hindered rotation treatment, T is the temperature in Kelvin;
kB and h are the Boltzmann and Planck constants, respectively.
Among these, only the symmetry factor can be easily calculated
from the molecular topology of the reactant. Obtaining the
exact value of four other factors requires structures, energies,
and vibrational frequencies of the reactant and transition state
for the reaction investigated. In the present study, we have
employed this formalism for reactions (R5)–(R8). In other
words, we used eqn (6)–(11) to extrapolate rate constants
calculated for small (R1)–(R4) reactions to those of
(R5)–(R8) reactions. Resulting high pressure limits of rate
constants are shown in Fig. 4 (RC-TST). The geometries,
frequencies, ZPE values for reactants and transition states,
explicit values of all the factors for (R5)–(R8) and resulting rates
are available in the ESIw, Tables S8, S10 and 11 and S27–S31.
The potential energy factor can be calculated using the
reaction barrier heights of the arbitrary reaction and the
reference reaction. The classical reaction barrier height DVa
for the arbitrary reaction can be obtained using the Linear
Energy Relationship (LER), similar to the well-known
Evans–Polanyi linear free energy relationship, between
classical barrier heights and reaction energies of reactions in
a given reaction class. Combining averaged values for expressions
(7)–(11) with Linear Energy Relationship (LER),17 one can
extrapolate rate constants for any reaction by knowing only
the reaction energy as has been done for the 1,4 hydrogen
migration12 and others.17,18,20,22 Since application of the
RC-TST/LER methodology for the 1,4 H-shift in alkyl radicals
reaction class was done,12 its prediction for the (R6) reaction,
labeled as RC-TST/LER, is also shown in Fig. 4. Within the
experimental temperature range from 850–1000 K, our
predicted rate constants agree very well with those from
experimental data even with the reasonably large uncertainty
factor of 2. The agreement is still satisfactory within the
temperature range of 700–1900 K, where the high pressure
limits of rate constants were derived in ref. 6 and 7.
Performance of the RC-TST/LER method is slightly worse
than RC-TST. The convenience of rate expressions without TS
knowledge would off-set the lower accuracy of the LER
approach, however.
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5. Conclusion
In this work, rate constants of the H-shift reactions in linear
alkyls, namely propyl, butyl, pentyl, and hexyl radicals have
been investigated theoretically. We found that:
� A CCSD(T)/cc-pVDZ//BH&HLYP/cc-pVDZ method is a
cost effective method for exploring the potential energy surface
of the intramolecular hydrogen migration in alkyl radicals.
� Tunneling is significant in all reactions considered here at
low temperatures even at the room temperature.
� By using the RC-TST formalism, rate constants of H-shift
in larger alkyls can be accurately extrapolated from those of
smaller alkyls when compared to available experimental data.
This further confirms the validity of the RC-TST
methodology.
Although the above observations are based on only four
selected reactions, they are expected to be valid for all
members of the intramolecular hydrogen migrations in alkyls.
Thus, approximate expressions within the RC-TST/LER
framework for these 1,3 to 1,6 H-shift classes for alkyls would
be useful and will be reported in a future study.
References
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Fig. 4 Arrhenius plots of the calculated and experimental rate constants for the reactions: (a) (R5): C�CCCCC 2 CC�CCCC, (b) (R6):
C�CCCCC2 CCC�CCC, (c) (R7): C�CCCCCCC2 CCC�CCCCC and (d) (R8): C�CCCCCCC2 CCCC�CCCC. Experimental data are taken
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