Transcript phacet.pptx

65th OSU International Symposium on Molecular Spectroscopy
RH14
Background information:
a = 0.656(5) D
= 0.375(10) D ( toluene )
v24 =  140 cm-1
v36 = 151.9 cm-1
Gauche
cmw, first:
cmw, details:
FTMW, geometry:
Zeil + Winnewisser +…, Z.Naturforsch. 15a, 1011 (1960)
Cox et al., JCS Farad.Trans. II 71, 93 (1975)
Dreizler et al., J.Mol. Struct. 698, 1 (2004)
ir, normal modes:
LIF, v24,v36:
King + So, J.Mol. Struct. 36, 468 (1970)
Bacon + Hollas + Ridley, Can.J.Phys. 62, 1254 (1984)
ab-initio:
Csaszar + Fogarasi + Boggs, J.Phys.Chem. 93, 7644 (1989)
astro related:
made from benzene, acetylene, vinylacetylene…
Marker of aromatic chemistry? Titan?
Assignment of the phenylacetylene ground state:
Spectrum dominated by specific bands formed by high-J, aR-type transitions
[ type-II+ n=2  classification and properties in Kisiel, Pszczolkowski,
J.Mol.Spectrosc. 178, 125 (1996) ]
J”
AABS has been applied to many different types of broadband spectra:
FASSST, cascaded multiplication THz, chirped pulse FTMW, Bruker FTIR..
Quantum number coverage for the ground state:
Symbol size is proportional to
(nobs-ncalc)/dn
STARK = Zeil et al.
Cox et al.
FTMW = Dreizler et al.
+ this work
Spectroscopic constants for the ground state of
phenylacetylene:
n  340 GHz
J  140
Ka  59
Rather rudimentary HF/4-21G
calculation with scaling,
Csaszar et al , J.Phys.Chem. 93,
7644 (1989).

Excited state type-II+ bands in phenylacetylene:
Changes in excited state line patterns relative to g.s. are usually moderate and dependant on
changes in inertia defect.
In this case the changes are much greater requiring the interstate perturbation treatment.
Lowest normal modes in phenylacetylene:
These are the out-of-plane and inplane distortion of –CCH relative
to the phenyl ring.
The next higher mode is
n23(B1)=349 cm-1.
140 cm-1
151.9 cm-1
The Hamiltonian:
The symmetry point group for phenylacetylene is C2v and 24=1 (B1) and 36=1 (B2) can
couple around the axis, which transforms as:
B1  B2 = A2,
This is the z-axis and, since phenylacetylene is prolate, the two states can thus perturb
through a-axis Coriolis interactions.
The Hamiltonian is set up in 22 block form, where the diagonal blocks are Watson’s
rotational terms for each state, the 36=1 block is augmented by the vibrational energy
separation DE, and the off-diagonal terms are:
Hc(24 ,36) = i (Ga + GaJP2 + GaKPz2 + …) Pz +
(Fbc + FbcJP2 + FbcKPz2 + …) (Px Py + Py Px ) + …,
The major coupling constant Ga is related to the Coriolis coefficient za24,36 by:
Ga = A za24,36 [ (w24/w36)1/2 + (w36/w24)1/2 ]
Fits and predictions were made with the SPFIT/SPCAT package of H.M.Pickett.
Nuclear spin statistical weights in phenylacetylene:
 5:3 weights arise from the presence of two pairs of symmetry-equivalent protons.
 weights will reverse between g.s. and B-symmetry excited states.
 each doublet below consists of 444,41 434,40 transition (left) and
443,41 433,40 transition (right)
24 = 1
g.s.
36 = 1
The Coriolis fit for (24=1  36=1) in phenylacetylene:
za24,36=0.8393(3)
Calculated:
za24,36=0.84
Two alternative fits of interstate interaction:
Solution I:
A24 < A0 < A36 sfit=36.1 kHz
Solution II:
A24 > A0 > A36 sfit=36.8 kHz
Discrimination on the basis of
standard deviation or values of
other constants not very sharp.
Clearest distinction is provided by
calculation of Av-A0 made with the
CFOUR package.
Vibrational changes in rotational constants (MHz):
MP2/6-31G(d,p)
Deperturbed values obtained from
the effective values:
A24 - A0 = -173.45 MHz and
A36 - A0 = 172.09 MHz
calculated by CFOUR.
The perturbation contribution
subtracted from the effective values
is given by:
Solution I
J.Mol.Spectrosc. in press
SUMMARY:
 Room temperature rotational spectrum of phenylacetylene was studied up to
340 GHz.
 Ground state transitions were measured up to J =140 and Ka=59.
 Transitions in the two lowest vibrationally excited states have been assigned
and the strong a-axis Coriolis resonance between the two states was
successfully fitted (sfit=36 kHz).
 All excited state lines that are strong enough for confident assignment are in the
fits, including several nominal interstate transitions, but all of these lines are
almost equally well fitted with two different solutions.
 Anharmonic force field calculations of vibrational changes in rotational
constants allowed unambiguous discrimination between alternative solutions.
 Strongest lines in the rotational spectrum can be predicted well into the
submillimeter.