FTIR Isotopic and DFT Studies of Transition MetalCarbon Clusters Condensed in Solid Argon: CrC3 - PowerPoint PPT Presentation

1 / 20
About This Presentation
Title:

FTIR Isotopic and DFT Studies of Transition MetalCarbon Clusters Condensed in Solid Argon: CrC3

Description:

Abundance of C2v isomer increased with hotter source ... 13C isotopic shift frequencies were also calculated for the linear isomer. Cr rod 30% 13C rod ... – PowerPoint PPT presentation

Number of Views:101
Avg rating:3.0/5.0
Slides: 21
Provided by: djew
Category:

less

Transcript and Presenter's Notes

Title: FTIR Isotopic and DFT Studies of Transition MetalCarbon Clusters Condensed in Solid Argon: CrC3


1
FTIR Isotopic and DFT Studies of Transition
Metal-Carbon Clusters Condensed in Solid Argon
CrC3
S.A. Bates, C.M.L. Rittby, and W.R.M. Graham
Department of Physics and Astronomy Texas
Christian University Fort Worth, TX 76129 61st
Meeting of the International Symposium on
Molecular Spectroscopy The Ohio State
University June 19-23, 2006
2
Motivation
  • Astrophysical
  • Metals observed in small molecules found in
    circumstellar shells and in the ISM
  • CrO in M stars (Davis, ApJ, 1947)
  • AlNC, NaCl in IRC10216
  • (Cernicharo, AA, 1987 Ziurys, ApJ, 2002)
  • NaCN, MgNC in CRL 2688 (Highberger, ApJ, 2001)
  • Pure carbon chains observed in circumstellar
    shells (e.g. C3, C5)
  • (Hinkle, Science, 1988 Cernicharo, ApJ, 2000
    Bernath, Science, 1989)
  • Silicon-bearing species observed in IRC10216
    include SiCN and SiC3 (Apponi, ApJ, 1999
    Guélin, AA, 2000)
  • See WH10 on TiC3 (Kinzer, Astronomical Species
    and Processes)

3
Motivation
  • Metallocarbohedrenes
  • Small metal carbon clusters important in
    understanding the formation of metcars
  • (Guo, Science, 1992 Guo Castleman, Advances
    in Metal and Semiconductor Clusters, 1994
    Castleman, Nano Lett, 2001)
  • TiC2, VC2 as building blocks for larger metcars
  • (Castleman, JPC, 1992 Tono, JCP, 2002)
  • Previous photoelectron spectroscopy (PES) and
    density functional theory (DFT) studies on MC2
    and MC3 clusters (MSc, V, Cr, Mn, Fe, Co, and
    Ni)
  • (Wang Li, JCP, 1999 Wang Li, JCP, 2000)

4
Motivation
  • Uncertain ground state for CrC3 (Zhai, JCP,
    2004)

DFT predictions for the lowest energy isomers of
CrC3 and CrC3
aDenotes ground state energy
  • PES spectra
  • Exhibit features consistent with both isomers.
  • Abundance of C2v isomer increased with hotter
    source
  • conditions indicating to the authors the linear
    isomer may be
  • more stable.

5
Research Objectives
  • To measure the vibrational fundamentals and
    isotopic shifts of metal carbon (MCn) species
    produced by NdYAG laser ablation and trapped in
    solid Ar at 10 K.
  • To identify and determine the structures of the
    MCn species created by comparing Fourier
    transform Infrared (FTIR) measurements with DFT
    predictions.

6
Strategy
  • 13C isotopic shifts necessary for species and
    structure determination.
  • Low 13C enrichment (10) limits isotopic shifts
    to single 13C isotopomers, which is useful for
    large Cn clusters (ngt6).
  • But for small clusters (nlt5), using 50 13C
    enrichment produces all of the 13C isotopomers.

7
Experimental Procedures
See previous talk, WG04 (Gonzalez,
Matrix/Condensed Phase)
8
?5
?7
?4
?6
?6
C7
?3
C11
C7
C10
?3
C9
C5
C3
1894.3
?9
2074.9
1946.1
2127.8
1998.0
?5
C12
?5
?7
2164.1
2038.9
C6
C10
C8
?8
?5
C11
1818.0
C9
1952.5
12C rod Cr rod
1915.8
2071.7
?9
1856.7
2078.1
C8
1789.5
1710.5
Absorption
12C rod
Frequency (cm-1)
9
Cr rod 15 13C rod
1789.5
Absorption
1721.8
1735.1
1777.8
1746.1
1779.7
1743.4
Frequency (cm-1)
10
Cr rod 15 13C rod
1789.5
  • Three remaining features
  • Nominal enrichment 15 13C
  • Observed effective enrichment 7 (based on
  • other Cn species)

Absorption
  • Three features are consistent with a molecule
  • containing three inequivalent C atoms.

Linear CrC3?
1777.8
1779.7
1743.4
Frequency (cm-1)
11
1789.5
Absorption
Cr rod 15 13C rod
1777.8
1779.7
1743.4
Frequency (cm-1)
12
Calculations Linear and C2v Isomers of CrC3
DFT (B3LYP/6-311G 3df) predicted vibrational
frequencies and intensities
(1789.5)
aFrequencies for fanlike structure initially
published by Wang and Li, 2000.
13
Theoretical Calculations
  • Used Gaussian 03
  • Used density functional theory (DFT) with B3LYP
    functional and 6-311G(3df) basis set
  • Calculations performed for linear and C2v (fan)
    structures
  • Calculations for C2v structure vibrational
    frequencies in good agreement with previous
    (Wang Li, JCP, 2000)
  • 13C isotopic shift frequencies were also
    calculated for the linear isomer

14
Cr rod 30 13C rod
1789.5
1720.6
1731.4
1733.5
Absorption
1777.8
1767.1
1779.7
1743.4
Cr rod 15 13C rod
DFT simulation 10 13C
Frequency (cm-1)
15
Calculations Isotopic Shift Frequenciesfor the
?1(s) Mode of Linear CrC3
Comparison of observed vibrational frequencies
(cm-1) of the ?1(s) mode for 13C-substituted
isotopomers of linear CrC3 with the predictions
of B3LYP/6-311G (3df) calculations
aDFT calculations scaled by a factor of
1789.5/1947.40.91892.
16
Cr rod 30 13C rod
1789.5
1720.6
1731.4
Absorption
1779.5
1733.5
1777.8
1767.1
1743.3
DFT simulation 10 13C
Frequency (cm-1)
17
Conclusions
  • The linear isomer of CrC3 has been observed.
  • The ?1(s) mode is assigned to 1789.5 cm-1.
  • No evidence of the C2v (fan) structure is
    observed.
  • Four modes are predicted to lie within detector
    range.
  • The strongest mode at 544 cm-1 is predicted to
    be 20 of the intensity of the ?1(s) mode of the
    linear structure and should be observable.
  • Observation of the linear ground state structure
    is consistent with the thermal behavior in PES
    experiments.

18
Acknowledgments
  • Our group would like to acknowledge funding from
  • Welch Foundation
  • TCU Research and Creative Activities Fund
    (TCURCAF)
  • W.M. Keck Foundation
  • Personal funding acknowledgments
  • Barnett Scholarship
  • Texas Space Grant Consortium Fellowship (TSGC)

19
References
  • D.N. Davis, Astrophys. J. 106, 28 (1947).
  • J. Cernicharo and M. Guélin, Astron. and
    Astrophys. 183, L10 (1987).
  • L.M. Ziurys, C. Savage, J.L. Highberger, A.J.
    Apponi, M. Guélin, and J. Cernicharo, Astrophys.
    J. 564, L45 (2002).
  • J.L. Highberger, C.S. Savage, J.H. Bieging, and
    L.M. Ziurys, Astrophys. J. 562, 790 (2001).
  • A.J. Apponi, M.C. McCarthy, C.A. Gottlieb, and P.
    Thaddeus, Astrophys. J. 516, L103 (1999).
  • M. Guélin, S. Muller, J. Cernicharo, A.J. Apponi,
    M.C. McCarthy, C.A. Gottlieb, and P. Thaddeus,
    Astron. and Astrophys. 363, L9 (2000).
  • K.H. Hinkle, J.J. Keady, and P.F. Bernath,
    Science 241, 1319 (1988).
  • J. Cernicharo, J.R. Goicoechea, and E. Caux,
    Astrophys. J. 534, L199 (2000).
  • P.F. Bernath, K.H. Hinkle, and J.J. Keady,
    Science 244, 562 (1989).
  • B.C. Guo, K.P. Kerns, and A.W. Castleman, Jr.,
    Science 255, 1411 (1992).

20
References
  • B.C. Guo and A.W. Castleman, Jr., in Advances in
    Metal and Semiconductor Clusters, ed. M.A. Duncan
    (Jai Press, London, 1994), Vol. 2, 137.
  • S.E. Kooi, B.D. Leskiw, and A.W. Castleman, Jr.,
    Nano Letters 1, 113 (2001).
  • S. Wei, B.C. Guo, J. Purnell, S. Buzza, and A.W.
    Castleman, Jr., J. Phys. Chem. 96, 4166 (1992).
  • K. Tono, A. Terasaki, T. Ohta, and T. Kondow, J.
    Chem. Phys. 117, 7010 (2002).
  • S.-L. Wang and X. Li, J. Chem. Phys. 112, 3602
    (2000).
  • H.-J. Zhai, L.-S. Wang, P. Jena, G. L. Gustev,
    and C.W. Bauschlicher, Jr., J. Chem. Phys. 120,
    8996 (2004).
  • M.E. Jacox, NIST Vibrational and Electronic
    Energy Levels Database (http//webbook.nist.gov/ch
    emistry)
  • J. Szczepanski, S. Eckern, C. Chapo, and M. Vala,
    Chem. Phys. 211, 359 (1996).
  • P.F. Souter and L. Andrews, J. Am. Chem. Soc.
    119, 7350 (1997).
  • J. Szczepanski, C. Wehlburg, M. Vala, J. Phys.
    Chem. A 101, 7039 (1997).
Write a Comment
User Comments (0)
About PowerShow.com