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PRECURSORS FOR METAL-ORGANIC CHEMICAL VAPOR DEPOSITION OF THIN FILMS
By
DAN R. DENOMME
A THESIS PRESENTED TO THE GRADUATE SCHOOL OF THE UNIVERSITY OF FLORIDA IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF
SCIENCE
UNIVERSITY OF FLORIDA
2012
2
© 2012 Dan Denomme
3
ACKNOWLEDGEMENTS
This thesis would not have been possible without the guidance and patience of my
research advisor Professor Lisa McElwee-White. I am also indebted to many
colleagues who have supported me along the way a couple of those who have been
crucial are Jürgen Koller and K. Randall McClain. I am extremely grateful to Khalil
Abboud for being a great mentor, friend, and boss. I owe my deepest gratitude to my
friends and family who have been crucial to my success.
4
TABLE OF CONTENTS
page ACKNOWLEDGEMENTS ............................................................................................... 3 LIST OF TABLES ............................................................................................................ 6 LIST OF FIGURES.......................................................................................................... 7 LIST OF SCHEMES ........................................................................................................ 8 ABSTRACT ..................................................................................................................... 9 CHAPTER 1 INTRODUCTION .................................................................................................... 11
Thin Films ............................................................................................................... 11 Chemical Vapor Deposition and Atomic Layer Deposition ...................................... 11
Interconnects .................................................................................................... 11 Refractory Metal Nitrides .................................................................................. 12
2 ZIRCONIUM CARBIDE PRECURSORS ................................................................ 14
Background............................................................................................................. 14 Results and Discussion........................................................................................... 16 Conclusion .............................................................................................................. 24 Experimental Section .............................................................................................. 25
3 COMPOUNDS FOR DEPOSITION OF RU AND FE THIN FILMS ......................... 28
Background............................................................................................................. 28 Results and Discussion........................................................................................... 29 Conclusion .............................................................................................................. 35 Experimental Section .............................................................................................. 37
4 PRECURSORS FOR TUNGSTEN NITRIDE THIN FILMS ..................................... 40
Background............................................................................................................. 40 Results and Discussion........................................................................................... 41 Experimental Section .............................................................................................. 42
APPENDIX A NMR DATA ............................................................................................................. 44 B IR SPECTRUM ....................................................................................................... 50
5
C X-RAY CRYSTALLOGRAPHY TABLES................................................................. 51 D MOLECULAR ORBITAL DIAGRAM OF 4............................................................... 61 REFERENCES.............................................................................................................. 62 BIOGRAPHICAL SKETCH ............................................................................................ 67
6
LIST OF TABLES Table page 2-1 Crystallographic Structural Data for 3 ................................................................. 19 2-2 Selected Bond Angles (°) and Distances (Å) for 3 .............................................. 20
2-3 Selected Bond Distances (Å) for 227 .................................................................. 21 3-1 Crystallographic Structural Data for 7 ................................................................. 30 3-2 Parameters for Selected CVD Runs with Compound 8 ...................................... 36
C-1 Atomic Coordinates for 3 .................................................................................... 51 C-2 Bond Lengths and Angles 3 ................................................................................ 51
C-3 Anisotropic Displacement Parameters for 3 ....................................................... 56 C-4 Atomic Coordinates and Equivalent Isotropic Displacement Parameters for 7 ... 57 C-5 Bond Lengths and Angles 7 ................................................................................ 60 C-6 Anisotropic Displacement Parameters for 7........................................................ 60
7
LIST OF FIGURES Figure page 1-1 Dual Damascene Structure................................................................................. 13 2-1 Examples of phenyl propargyl zirconium complexes .......................................... 16 2-2 1H and 13C chemical shifts for one of the four equivalent phenylpropargyl
ligands of 3 ......................................................................................................... 17 2-3 Thermal ellipsoids drawing of the molecular structure of 3 ................................. 19 2-4 Resonance structures of propargyl zirconium complex ...................................... 21 2-5 Optimized derivative of 3 for DFT calculations ................................................... 22 2-6 Degenerate HOMO (top) and HOMO-2 (bottom) of propargyl complex 4........... 23 2-7 LUMO (top left), LUMO+1 (top right), and degenerate LUMO+2 (bottom) of
propargyl complex 4 ........................................................................................... 24 3-1 Ruthenium β-diketonates.................................................................................... 28 3-2 Compound 7 ....................................................................................................... 29 3-3 Thermal ellipsoids drawing of the molecular structure of 7................................. 31 3-4 Compound 8 ....................................................................................................... 32 3-5 TGA data of 7 and 8 ........................................................................................... 33 3-6 Atomic composition of films from three separate CVD runs ............................... 34 4-1 Single-source precursors for WN thin films ........................................................ 40 4-2 Diazo-tungsten complex 15-17 ........................................................................... 41 A-1 1H NMR spectrum of 3 ....................................................................................... 44 A-2 1H-13C gHMBC spectrum of 3 ............................................................................ 45 A-3 Expansion of the 1H-13C gHMBC spectrum of 3 ............................................... 46 A-4 1H NMR spectrum of 7 ...................................................................................... 47 A-5 1H NMR spectrum of 8........................................................................................ 48 A-6 1H NMR spectrum of 9........................................................................................ 49 B-1 IR of 7 .................................................................................................................. 50
8
LIST OF SCHEMES Scheme page 2-1 Synthesis of Complex 3. ..................................................................................... 16 3-1 Synthesis of 7 ..................................................................................................... 30 3-2 Synthesis of 9 ..................................................................................................... 35
9
Abstract of Thesis Presented to the Graduate School of the University of Florida in Partial Fulfillment of the
Requirements for the Degree of Master of Science
PRECURSORS FOR METAL-ORGANIC CHEMICAL VAPOR DEPOSITION OF THIN FILMS
By
Dan R. Denomme
December 2012
Chair: Lisa McElwee-White Major: Chemistry
A variety of metal-organic complexes to be used as precursors for chemical vapor
deposition (CVD) of thin films were designed and synthesized. Tetra(η3-
phenylpropargyl)zirconium was created as a precursor for zirconium carbide (ZrC) thin
films. ZrC thin films have been used in many applications, one of those being a
component in field emitter arrays replacing thermionic emitters in vacuum tubes as
electron sources.
The phenylpropargyl zirconium compound was created by reacting ZrCl4 with
phenylpropargylmagnesium bromide to yield the first known example of a homoleptic
propargyl complex. Characterization was done by 1H NMR spectroscopy and X-ray
crystallography showing all four phenylpropargyl ligands coordinated to the Zr center in
an η3-mode resulting in a complex of D2d symmetry.
Dicarbonylmethylcyclopentadienyl ruthenium was synthesized from triruthenium dodecacarbonyl and characterized by 1H NMR, X-ray crystallography, and TGA. This
volatile compound is an effective precursor for deposition of ruthenium metal thin films,
which have great potential as a copper diffusion barrier in integrated circuits. Initial
CVD experiments have been conducted. An analogous compound,
10
dicarbonylmethylcyclopentadienyl iron was synthesized to further study the thermal
decomposition during CVD. The iron derivative is similar in structure and volatility
allowing it to be a viable model compound for CVD optimization.
A third group of metal-organic precursors was researched. These compounds
contain the general formula W(NNCR2)Cl4, where R = phenyl or tolyl. The diazo
complexes of tungsten are a new class of potential precursors for deposition of WNx
and WNxCy thin films, a proven copper diffusion barrier material. Synthesis has been
attempted by combining WCl4 with the corresponding diazo ligand. Preliminary results
and characterization with 1H NMR spectroscopy indicate the compounds have been produced with CVD experiments pending.
11
CHAPTER 1 INTRODUCTION
Thin Films
The ability to produce thin films of various materials has had a broad impact on
many applications. “Thin” is a relative term, and films with thicknesses less than a
micrometer will be addressed herein. While the first reported studies of thin films were
in the 17th century by Sir Isaac Newton it was not until the 20th century that their
relevance became well known.1 Thin films have been found to be useful in an enormous array of applications. These applications include optics, where thin films can
be used as reflective or anti-reflective coatings. This was first seen in silvering, a
technique used to manufacture mirrors in the 19th century. Tools have benefited from
thin film coatings to enhance properties and effectiveness. One of the most interesting
fields in thin films is microelectronics. Batteries, chips, boards, and integrated circuits
have advanced with the help of thin films.
Chemical Vapor Deposition and Atomic Layer Deposition
Chemical vapor deposition (CVD) and atomic layer deposition (ALD) are valuable
techniques used in the production of thin films .2,3 One of the advantages CVD and
ALD have over PVD is higher conformality when covering features with high aspect
ratios compared to the physical methods that rely on “line of sight” deposition. Also the
selection of precursors for CVD and ALD is larger allowing for a greater variety of
materials that can be deposited. 4
Interconnects
Interconnects in microelectronic devices were made from aluminum up until the
turn of the millennium when Intel and other companies began the transition to copper as
12
the material for metallization. Copper has less RC delays, the slowing of electrons
along a wire due to resistance and capacitance, than aluminum and is less likely to
electromigrate. This has been known for some time, however the technology to use
copper was not available when microelectronics were first mass produced. It wasn’t
until 1991 when Howard demonstrated reactive ion etching on copper which was the
common practice in fabricating aluminum based interconnect material.5 Now the length and complexity of the interconnects are growing and copper is needed to maintain high
speed transfer of electrons. While copper has advantages over aluminum it still diffuses
into the silicon and dielectric substrates it rests on forming copper silicide. To prevent
device failure a diffusion barrier is needed. The barrier has to have a low solubility for
copper, be durable, and not impede the flow of electrons.6
Refractory Metal Nitrides
Refractory metal nitrides have been implemented as diffusion barriers due to their
superb physical and chemical properties. These transition metal nitrides are extremely
hard, have high melting points, resistant to corrosion and chemical reactivity, and are
conductive.4 Titanium nitride was the industry standard for aluminum diffusion barriers,
currently tantalum nitride is most commonly used for copper interconnects.7 Tantalum nitride is an effective diffusion barrier, however copper does not adhere well to its
surface, therefore is a need for an additional layer, a tantalum bilayer.
Current interconnect technology is being pushed to its limits in integrated circuits.
Microprocessors have followed Moore’s law doubling the number of transistors in a
given area on an IC every two years.8 The manufacturing of ICs employs the Dual
Damascene process. 9 This process consists of deposition of a dielectric material, etching of the desired feature, physical vapor deposition (PVD) of a diffusion barrier
13
material, PVD of a metal bilayer that Cu will adhere to, PVD of a Cu seed layer,
electrochemical deposition (ECD) of the Cu interconnect, and finally chemical
mechanical polishing.
Figure 1-1. Dual Damascene Structure
The significant volume of the three diffusion barrier and seed layers, coupled with
the decreasing size of the interconnects and their features, demands a change in
diffusion barrier material and/or deposition techniques. The thickness of these layers
needs to continually shrink in size; however PVD is not an appropriate technique for the
production of ultra thin films. Physical vapor deposition techniques rely on “line of sight”
deposition and consequently conformality becomes a greater issue as the film thickness
decreases.10 CVD and ALD are superior alternatives to PVD, providing conformal coverage when depositing diffusion barriers.
14
CHAPTER 2 ZIRCONIUM CARBIDE PRECURSOR1S
Background
Zirconium carbide (ZrC) has promise in many different applications. With a
hardness of 25,000 N/mm2, ZrC is an ideal coating for tools that are susceptible to
wear, especially tools used for cutting other hard materials. Zirconium carbide is also
used as a coating for nuclear fuel pellets because of its high melting point, 3400 °C.
Another use of ZrC is in field emitter arrays (FEAs). FEAs are replacing thermionic
emitters in vacuum tubes as electron sources. While FEAs have many advantages over
the heat-induced flow of electrons, they are still subject to failure. Vacuum arcing or tip
dulling can lead to the destruction of the cathode. A zirconium carbide thin film coating
over the cathode can provide the needed strength to FEAs without dampening the
transfer of electrons, due to its electrical conductivity of 2 ×104 /Ω cm and relatively low
work function of 4.0 eV. 11
Alkylzirconium compounds have been used as single-source precursors for CVD
of ZrC thin films12-16 as an alternative to growth from ZrCl4 and methane under a
reducing H2 atmosphere at high temperatures (>1500 °C).17-19 The best established
single-source precursor for the CVD of ZrC is tetraneopentyl zirconium (Np4Zr).12,14,15,20
Successful CVD from Np4Zr is possible because the lack of β-hydrogen atoms on the alkyl ligands renders it stable enough for volatilization and transport in a CVD reactor.
1 (Portions of Chapter 2 were taken directly from, Denomme, D. R.; Dumbris, S. M.; Hyatt, I. F. D.; Abboud, K. A.; Ghiviriga, I.; McElwee-White, L., “Synthesis and Electronic Structure of Tetrakis(η3-phenylpropargyl)zirconium.” Organometallics 2010, 29 (21), 5252-5256.)
15
The range of compounds that have been used as single source precursors for
early metal carbides is very small. Ligands that contain heteroatoms are undesirable,
as incorporation of the additional element into the resulting thin films can be an issue.
Early transition metal alkyls with β-Hs are known to undergo β-H elimination under mild
conditions,21 making them unsuitable for CVD. The result is that few ligands meet the
necessary criteria for use in single source ZrC precursors. Propargyl ligands are
potential candidates, as they contain no heteroatoms and no β-H atoms.22-25 We thus
undertook a study of zirconium propargyl complexes as possible precursors for the CVD of ZrC.
To our knowledge, no homoleptic propargyl complex had been previously reported. However, propargyl derivatives of zirconocene have been previously reported
in the literature.22,24,26-29 The 18-electron bis(phenylpropargyl)zirconocene complex 1
contains one η1-propargyl ligand, with the second propargyl coordinated in the η3-
bonding mode.24 The signals of the methylene protons of the propargyl ligand in the 1H
NMR spectrum are characteristic of the bonding mode and were assigned at δ 1.9 for
the η1-ligand while the corresponding protons in the η3-ligand were observed at 3.3
ppm. The 16-electron phenylpropargyl methylzirconocene complex 2 was subsequently
described and a crystal structure confirmed η3-coordination of the phenylpropargyl
ligand.27 The 1H NMR spectrum of this compound also showed the methylene protons
of the η3-ligand at the expected value of 3.37 ppm.
16
Figure 2-1. Examples of phenyl propargyl zirconium complexes.
Results and Discussion
In an effort to prepare homoleptic propargylzirconium compounds for use in the CVD of ZrC, we first reacted ZrCl4 with CH3C CCH2MgBr. Since we were unable to
isolate tetra(η3-methylpropargyl)zirconium from the oligomeric material that resulted, we
synthesized tetra(η3-phenylpropargyl)zirconium (3) as a model compound for the
preparation of more volatile homoleptic propargyl zirconium species. The
phenylpropargyl Grignard reagent was synthesized as described in the literature
(Scheme 1).30,31 The commercially available phenylpropargyl alcohol was reacted with
PBr3 and the resulting bromide was then converted to the corresponding Grignard
reagent. Reaction with ZrCl4 afforded 3 in 74% crude yield. Single crystals of the pure
material can be obtained by recrystallization but continued handling of the complex
resulted in decomposition, rendering it unsuitable for CVD studies.
Scheme 2-1. Synthesis of Complex 3.
17
8
After recrystallization, the 1H NMR of 3 at room temperature in toluene-d8 showed
only a single aliphatic resonance at δ 3.21 ppm, consistent with η3-phenylpropargyl
ligands. All of the ligands were symmetry equivalent by NMR and although the complex
was prepared in ethereal solvents, no other signals corresponding to additional ligands
such as coordinated solvent were observed in the 1H NMR spectrum.
The 1H spectrum in THF-d8 at -60 °C displays distinct signals for the aromatic protons of the four equivalent phenyl rings at 7.35 (t, 7.7 Hz, 8H), 7.23 (t, 7.7 Hz, 4H)
and 6.96 (d, 7.7 Hz, 8H) which were assigned as meta, para and ortho,
correspondingly, based on their multiplicity and intensity (Figure 1).
Figure 2-2. 1H and 13C chemical shifts for one of the four equivalent phenylpropargyl
ligands of 3.2
The intensity was referenced to the signal for the four CH2 groups at 3.10 ppm.
The 13C chemical shifts were measured in the gHMBC spectrum, which was acquired
2 NMR spectra were obtained at -60 °C in THF-d .
18
with two different spectral windows in f1 to detect possible folding. One-bond couplings
with the protons identified the ortho, meta and para carbons at 127.5, 128.8 and 126.7
ppm, correspondingly. The quaternary carbon on the phenyl moiety (Cipso), at 129.1
ppm, coupled with the meta protons. The ortho protons coupled with a quaternary
carbon at 113.5, which was assigned as alpha to the phenyl. The methylene protons, on
the carbon at 38.7 ppm, coupled with this later carbon, with another quaternary at
129.4, assigned as beta to the phenyl, and, surprisingly, to the ortho carbons on the
phenyl ring. These 13C shifts are consistent with those previously reported for η3-
phenylpropargyl zirconium compounds 1 and 2. The quaternary carbons of 1 were
shown to be located at 120.5 and 114.1 ppm with the methylene shift at 55.5 ppm.
Dynamic exchange between η3 and η1 coordination of the phenylpropargyl ligand of 2 in
solution gave shifts of 112.9, 98.8, and 30.7 ppm.26 The methylene protons displayed an nOE with the ortho protons in the NOESY spectrum. Examination of the X-ray crystal
structure (vide infra) leads to the conclusion that the nOe is from the methylene group
on one propargyl ligand to the phenyl group of an adjacent ligand.
Crystallographic structure determination (Table 2-1) confirmed the identification of 3 as tetra(η3-phenylpropargyl)zirconium. The crystal structure of 3 verified the presence
of only the four propargyl ligands, all displaying η3-coordination (Figure 2-2). Complex 3
has an overall D2d symmetry, a point group previously but rarely observed in other Zr
compounds.32,33 An EAN of 16 electrons for 3 results from each phenylpropargyl ligand
donating four electrons. Selected bond angles and distances of 3 are shown in Table 2.
19
Figure 2-3. Thermal ellipsoids drawing of the molecular structure of 3.3
Table 2-1. Crystallographic Structural Data for 3.4
Empirical formula C36 H28 Zr Formula weight 551.8 Temperature 173(2) K Wavelength 0.71073 Å Crystal system Monoclinic Space group C2/c
3Thermal ellipsoids are drawn at 50% probability. Hydrogens on the phenyl rings are omitted for clarity.
4 R1 = Σ(||Fo| - |Fc||) / Σ |Fo|
wR2 = [Σ [w(Fo2 - Fc2)2] / Σ [w((Fo2))2]]1/2
S = [Σ [w(Fo2 - Fc2)2] / (n-p)]1/2
w= 1/[σ2(Fo2)+(m*p)2+n*p], p = [max(Fo2,0)+ 2* Fc2]/3, m and n are constants.
20
Table 2-1. Crystallographic Structural Data (Continued) a = 20.7551(14) Å α= 90°
Unit cell dimensions b = 8.6203(6) Å β= 11° c = 17.4685(11) Å γ = 90°
Volume 2808.1(3) Å3
Z 4 Density (calculated) 1.305 Mg/m3
Absorption coefficient 0.413 mm-1
F(000) 1136 Crystal size 0.19 x 0.11 x 0.04 mm3
Theta range for data collection 2.18 to 27.50° Index ranges -20≤h≤26, -11≤k≤11, -22≤l≤15 Reflections collected 9334 Independent reflections 3226 [R(int) = 0.0272]
Completeness to theta = 27.50° 99.80%
Absorption correction Integration Max. and min. transmission 0.9861 and 0.9103 Refinement method Full-matrix least-squares on F2
Data / restraints / parameters 3226 / 0 / 168 Goodness-of-fit on F2 1.065 Final R indices [I>2sigma(I)] R1 = 0.0244, wR2 = 0.0676 [2730] R indices (all data) R1 = 0.0312, wR2 = 0.0700 Largest diff. peak and hole hole 0.300 and -0.346 e.Å-3
Table 2-2. Selected Bond angles (°) and distances (Å) for 3. Zr-C1 2.4955(2) C2-C1-Zr 70.08(9) Zr-C2 2.4043(1) C3-C2-C1 154.38(2) Zr-C3 2.4474(2) C3-C2-Zr 77.01(1) C1-C2 1.3760(2) C4-C3-Zr 137.87(1) C2-C3 1.2490(0) C1-Zr-C1A 128.88(8) C3-C4 1.4500(2) C11-Zr-C1 131.95(5) C2-Zr- 98.49(5) C2-Zr-C11 108.31(6) C22-Zr- C2A
96.11(7) C3-Zr-C11 82.21(5)
Although structural data have been reported for several η3-propargyl complexes,27
the (phenylpropargyl) methylzirconocene complex 2 (Table 3) is perhaps the best model
for the geometry of the propargyl ligands of 3. The phenylpropargyl ligands of
21
complexes 2 and 3 exhibit nearly identical C-C-C bond angles of 154.4(3)° and 154.38(2)°, respectively, indicating similar bonding of the propargyl moiety to the Zr
center.
Table 2-3. Selected Bond Distances (Å) for 2.27
C1-C2a 1.344(5) C2-C3 1.259(4) Zr-C1 2.658(4) Zr-C2 2.438(3) Zr-C3 2.361(3)
aThe numbering system of the propargyl ligand is as shown for compound 3 in Figure 2.
The Zr-C2 bond length is approximately the same in the two structures. However, the three Zr-C bond distances in 3 are roughly the same length, differing only
by a net 0.09 Å overall, whereas those in 2 differ by a much larger value, 0.29 Å, with
the C1-C2-C3 plane of 2 canted so that the methylene carbon C1 is further from the
metal center. For both complexes, an assignment of the phenylpropargyl bonding as
intermediate between the η3-propargyl and allenyl limiting resonance structures (A and
B) is supported by the bond lengths and angles. A similar assignment of the bonding in
Cp*(TBM)Zr(η3-CH2C CCH3) was made based on the crystal structure.28
Figure 2-4. Resonance structures of propargyl zirconium complex.
The bonding of the propargyl ligands to the metal center in 3 was further analyzed
by density functional theory calculations. Geometry optimizations and single-point
calculations were performed using the DFT B3LYP34,35 functional and the lanl2dz36,37
22
basis set utilized in the Gaussian 03 program package.38 Compositions of molecular
orbitals were calculated using the AOMix program.39,40 Molecular orbital pictures were
generated from Gabedit.41 Initial calculations were performed on 3 itself, however the
presence of the phenyl rings complicated the interpretation by delocalizing the
molecular orbitals to such an extent that visualization was difficult. In order to simplify
the analysis, calculations were carried out on the parent tetrapropargyl zirconium
complex 4 in which the phenyl rings were replaced with hydrogen to provide a
computational model structure. The crystallographically determined structure of 3 was
used for the positions of the non-H atoms of 4. Hydrogen atoms were placed by
geometry optimization and the D2d symmetry of 3 was enforced in 4.
Figure 2-5. Optimized derivative of 3 for DFT calculations.
A molecular orbital diagram (see Appendix D) was generated from the
computational results for 4 and showed a calculated HOMO-LUMO gap of 5.2 eV. This
substantial splitting of the frontier orbitals is consistent with the lack of reactivity of 3
with other species in the reaction mixtures during synthesis. While other D2d Group 4
metal complexes have been reported in the literature,42-44 examples of computational
results are rare. An electronically similar D2d symmetric bispentalene titanium complex
had a calculated HOMO-LUMO gap of 1.93 eV, far smaller than that of 3.42 Tetra(η3-
allyl)zirconium is also a known compound described as a bright red solid, which
decomposes at -20 °C.45,46 The red color and lability of tetra(η3-allyl)zirconium
suggest
23
that its HOMO-LUMO gap must also be smaller than that of 3, which is a colorless solid
that is stable for moderate periods of time at room temperature.
Figure 2-6. Degenerate HOMO (top) and HOMO-2 (bottom) of propargyl complex 4.
The high-lying occupied orbitals of 4 are depicted in Figure 3. The HOMO is
largely comprised of two degenerate orbitals containing the p orbitals of C1 and C3 of
the propargyl ligands. The symmetry dictates that one HOMO orbital includes the dyz of
Zr (20.7%) and the p orbitals in the yz plane of the propargyl ligands, while the other
HOMO orbital utilizes the dxz of Zr (20.7%) and the xz plane of the p orbitals on the
propargyl ligand. The HOMO-2 is comprised mainly of dz2 on Zr (21.3%) and xy plane of the p orbitals on the ligand. Metal-propargyl bonding dominated by interactions of
metal d orbitals with propargyl MO's localized on C1 and C3 is consistent with the
calculated MO diagrams for bonding in [3-CH2C CPh)Pt(PPh3)2].47
The LUMO of 4 (Figure 4) has the strongest p orbital contributions from C2 in the propargyl groups. This is consistent with its derivation from the antibonding C1-C2-C3
24
-orbital, which has its largest coefficient on C2. The largest contributions to the LUMO
from Zr are s (14.2%), and dz2 (11.9%). The LUMO+1 is mainly comprised of the non-
bonding dxy orbital of Zr (86.7%). The LUMO+2 consists of two degenerate orbitals, one
composed primarily of Zr dxz (25.3%) and the other dyz (25.3%).
Figure 2-7. LUMO (top left), LUMO+1 (top right), and degenerate LUMO+2 (bottom) of
propargyl complex 4.
The AO composition of the LUMO provides insight into why this 16 electron early
transition metal complex does not have an open coordination site for addition of another
ligand. The section of the LUMO derived from metal AO's is sterically blocked by the
CH2 groups of the four propargyl ligands. Although complex 3 was recrystallized from
THF with vapor diffusion of pentanes, coordinated THF is not detected in either the
NMR or the crystal structure.
Conclusion
The synthesis of 3 yields, to the best of our knowledge, the first example of a
homoleptic propargyl complex and has been shown by 1H NMR spectroscopy and X-ray
crystallography to have all four phenylpropargyl ligands coordinated to the Zr center in
25
an η3-mode resulting in a complex of D2d symmetry. The π-bonding in 3 was analyzed
by DFT calculations on the model compound 4. The -bonding from the four symmetry
equivalent 3-propargyl ligands and HOMO-LUMO gap of 5.3 eV is consistent with the
stability of the molecule and lack of reactivity toward coordinating solvents.
Experimental Section
General Procedures. All chemicals were purchased in reagent grade purity and
used with no further purification unless otherwise noted. All manipulations were carried
out using standard Schlenk and glove box techniques under an inert atmosphere of
argon or nitrogen. All solvents, unless otherwise noted, were purchased from Fisher
and passed through an M. Braun MB-SP solvent purification system or were distilled
from sodium/benzophenone prior to use. 1H and 13C NMR spectra were obtained on Varian Gemini 300 and VXR 300 and Mercury 300 spectrometers. Infrared spectra
were measured on a Perkin-Elmer 1600 FT-IR.
Phenylpropargyl Bromide. A 50-mL Schlenk flask containing 5.0 mL of ether and 4.8 g (3.7 mmol) phenylpropargyl alcohol and 1.0 g pyridine was cooled to 0 °C and 5.0 g (18 mmol) phosphorus tribromide was added dropwise over a 45 min period with
strong stirring under nitrogen in accordance with literature procedure.30 The resulting
mixture was added to 25 mL of ice to quench the excess PBr3 and extracted with ether
(3x25 mL). The organics were then washed with NaHCO3 and dried over MgSO4,
filtered and the ether was then removed by reduced pressure. Yield 6.0 g, 83%. 1H
NMR (C6D6) δ 4.1 (s, 2H), 7.4 (m, 5H). 13C NMR (CDCl3) δ 15.3, 84.2, 86.6, 121.9,
128.1, 128.7, 131.7.
26
Phenylpropargylmagnesium Bromide. An addition funnel was charged with
12.0 g (61.6 mmol) phenylpropargyl bromide and 30 mL ether and the mixture was
added dropwise to a three-neck flask cooled to 0 °C containing 1.80 g (75.0 mmol)
activated Mg turnings with a few crystals of HgCl2 in ether over a 4 h period in
accordance with literature preparation.31 After the addition, the reaction was refluxed for 1 h. The resulting mixture was filtered through a 1 cm pad of Celite (previously dried
and evacuated) to yield a dark yellow solution. Yield 30 mL of a 1.85 M solution of the
Grignard reagent, 90.1%. 1H NMR (C6D6) δ 2.11 (s, 2H), 6.8 (m, 5H).
Tetra(η3-phenylpropargyl)zirconium (3). An addition funnel was charged with 20.0 mL of 1.85 M phenylpropargylmagnesium bromide (37.0 mmol) and added
dropwise into a three neck flask containing 2.16 g (9.25 mmol) ZrCl4 slurried in 100 mL
ether over a 1 h period and stirred overnight at room temperature. Volatiles were then
removed via reduced pressure to afford a brown solid. The solid was extracted with 150
mL of toluene and filtered through a fine glass frit. The filtrate was concentrated to
afford a solution of 3 from which the compound was then precipitated by the addition of
hexanes. The resulting suspension was filtered through a fine glass frit to collect the
solid precipitate of 3. Yield 3.44 g, 74%. The product was tan in color. Single crystals
could be obtained by repeated vapor diffusion recrystallization using THF and pentanes
until a colorless-to-white solid remained. 1H NMR (THF-d8, -60 °C) δ 3.10 (s, 8H), 6.96 (d, 7.7 Hz, 8H), 7.23 (t, 7.7 Hz, 4H), 7.35 (t, 7.7 Hz, 8H). 13C NMR (THF-d8, -60 °C) δ 38.7, 113.5, 126.7, 127.5, 128.8, 129.1, 129.4.
Crystallographic Structure Determination of 3. X-ray experimental data for 3 were collected at 173 K on a Siemens SMART PLATFORM equipped with a CCD area
27
detector and a graphite monochromator utilizing MoK radiation (l = 0.71073 Å). Cell
parameters were refined using up to 8192 reflections. A full sphere of data (1850
frames) was collected using the ω-scan method (0.3° frame width). The first 50 frames
were re-measured at the end of data collection to monitor instrument and crystal
stability (maximum correction on I was < 1 %). Absorption corrections by integration
were applied based on measured indexed crystal faces.
The structure was solved by the Direct Methods in SHELXTL6,48 and refined using full-matrix least squares. The non-H atoms were treated anisotropically, whereas the
hydrogen atoms were calculated in ideal positions and were riding on their respective
carbon atoms. The complexes are located on 2-fold rotation axes; thus a half complex
occupies the asymmetric unit. A total of 168 parameters were refined in the final cycle
of refinement using 2730 reflections with I > 2s(I) to yield R1 and wR2 of 2.44% and
6.76%, respectively. Refinement was done using F2.
28
CHAPTER 3 COMPOUNDS FOR DEPOSITION OF RU AND FE THIN FILMS
Background
Ruthenium metal is a promising material for the next generation of copper diffusion
barriers. Not only does it posses all the qualities associated with good diffusion
barriers, such as high melting point, hardness, conductivity, and relative inertness but it
also has an affinity for copper adsorption making it a great seed layer.49,50 The ability to
act as a diffusion barrier and a seed layer can eliminate up to two steps from the dual
damascene process which could greatly reduce production cost and save valuable
space in ever shrinking integrated circuits.
There are three main families of CVD precursors for the deposition of ruthenium
thin films. These families are ruthenium β-diketonates, ruthenocene derivatives, and
ruthenium carbonyl complexes. Two examples of the β-diketonates that have been
studied for CVD of ruthenium thin films are Ru(od)3 (od = 2,4-octanedionato) (5) and
Ru(tmhd)3 (tmhd = 2,2,6,6-tetramethyl-3,5-heptanedionato) (6). 51,52
O O
O O O O
Ru Ru O
O O O O O
5 6 Figure 3-1. Ruthenium β-diketonates.
29
Generally compounds 5 and 6 form RuO2 during CVD with O2, however, there is
one example when THF was used as an injecting liquid where Ru metal was formed,
possibly due to the consumption of O2 during the oxidation of THF.53 Triruthenium
dodecacarbonyl, Ru3(CO)12, has been used to deposit ruthenium metal thin films at 150
°C.54
Results and Discussion
In efforts to develop a precursor that will produce high quality ruthenium thin films
and at the same time be optimal for CVD, dicarbonylmethylcyclopentadienyl ruthenium
(7) was targeted.
CO Ru
CO CH3
7 Figure 3-2. Compound 7
Compound 7 is isoelectronic to the ruthenocene compounds that have been
implemented in the past.55 MeRu(CO)2Cp is promising for CVD or ALD because of its
volatility. Complex 7 sublimes at 40 °C (0.1 mmHg).56 The synthesis was adopted from
Davidson et. al. and is shown in Scheme 2.57
30
cyclopentadiene (CpH)
Ru3(CO)12
10
Heptane
Ru2(CO)4(Cp)2
11
3% NaHg THF
MeRu(CO)2Cp
7
MeI
THF
Na+[Ru(CO)2Cp]-
Scheme 3-1. Syntheses of 7
Crystals of 7 were obtained by sublimation. The 1H NMR spectrum of 7 at room
temperature in chloroform-d showed resonances at δ 5.23 ppm and at δ 0.31 ppm.
Crystallographic structure determination (Table 3-1) confirmed the identification of 7; the
geometry of the compound is that of a three-legged piano stool. The Cp occupies three
coordination sites on one face while the two carbonyls and methyl occupy the other
three.
Table 3-1. Crystallographic Structural Data for 7.5
Empirical formula C8 H7.25 O2.25 Ru Formula weight 240.46 Temperature 173(2) K Wavelength 0.71073 Å Crystal system Orthorhombic Space group P2(1)2(1)2(1)
5 R1 = å(||Fo| - |Fc||) / å|Fo|
wR2 = [å[w(Fo2 - Fc2)2] / å[w(Fo2)2]]1/2S = [å[w(Fo2 - Fc2)2] / (n-p)]1/2
w= 1/[s2(Fo2)+(m*p)2+n*p], p = [max(Fo2,0)+ 2* Fc2]/3, m & n are constants
31
Table 3-1. Crystallographic Structural Data (Continued) a = 6.8889(7) Å a= 90°.
Unit cell dimensions b = 10.5841(10) Å b= 90°. c = 11.4638(11) Å g = 90°.
Volume 835.86(14) Å3
Z 4 Density (calculated) 1.911 Mg/m3
Absorption coefficient 1.823 mm-1
F(000) 469 Crystal size 0.142 x 0.136 x 0.11 mm3
Theta range for data collection 2.62 to 27.50°. Index ranges -8≤h≤8, -13≤k≤13, -14≤l≤14 Reflections collected 7208 Independent reflections 1917 [R(int) = 0.0182] Completeness to theta = 100.00% 2A7b.s5o0r°ption correction None Refinement method Full-matrix least-squares on F2 Data / restraints / parameters 1917 / 3 / 104 Goodness-of-fit on F2 1.089 Final R indices [I>2sigma(I)] R1 = 0.0195, wR2 = 0.0464 [1886] R indices (all data) R1 = 0.0200, wR2 = 0.0466 Absolute structure parameter 0.50(6) Largest diff. peak and hole 0.687 and -0.533 e.Å-3
Figure 3-3. Thermal ellipsoids drawing of the molecular structure of 7. Thermal
ellipsoids are drawn at 50% probability.
32
To evaluate the effectiveness of compound 7 as a precursor for thin film deposition
of ruthenium films CVD experiments were run. Initial reactions were run with H2 as a
co-reactant and N2 as the carrier gas, based on previous work with growing tungsten nitride (WN) diffusion barrier films. These experiments were unsuccessful, probably
because the CVD conditions for WN thin films were too extreme for these Ru
precursors. Iron may be the solution to fine tuning the CVD parameters.
The iron analogue to 7, dicarbonylmethylcyclopentadienyl iron (8) is an ideal
model compound to optimize conditions for CVD of Ru thin films. Electronically similar
to 7, 8 is approximately one hundred times cheaper to synthesize than its ruthenium
counterpart. One of the most important physical properties regarding CVD precursors is
the volatility. Thermal gravimetric analysis (TGA) indicates that both compounds
sublime around the same temperature at atmospheric pressure.
CO Fe
CO CH3
8 Figure 3-4. Compound 8.
33
80
60
:E ·a;l
40
20
88.42%
40 50 60 70
Temperature (•C) 80 90
Universal V4.5A TA
100
80
60 91. 6
:E Cl Qi
40
20
04--- -- -r-- -- -- -- -- -- -- -r-- --- 20 30 40 so
Temperature (c·) Figure 3-5. TGA data of 7 and B.
60 70 Universal V4.5A TA
34
%
Iron oxide thin films were obtained with the composition of 36.7% Fe and 61.1%
oxygen according to XPS measurements. This is indicative of Fe2O3. In aerobic
conditions higher temperatures often lead to higher oxidation states.58-61 Reducing the
temperature from the initial run of 575 °C led to films with higher Fe concentrations and
at higher oxidation states as expected. Unfortunately the films were contaminated with
carbon.
60
52.0
50
40.2 40.0 40
26.9 38.0
21.1
21.8
32.2 30
27.8 Fe
O 20 C
10
450 400
350
300
250
0 200
Temperature (°C) Figure 3-6. Atomic composition of films from three separate CVD runs.
Recently Kanjolia et. al. have produced some of our targeted precursors and
have successfully used them as precursors for Ru thin films.62-64 The high carbon
contents in the films were a concern. In attempts to identify the carbon source,
dicarbonylethylcyclopentadienyl iron (9) was synthesized as outlined in Scheme 3.
35
O
O
C C O
Fe Fe C
O C
O
NaHg THF
2 Na
Fe C O C
Na Fe C O C
O
Et-I Fe Et
THF C C O O
9 Scheme 3-2. Synthesis of 9 By replacing the methyl with an ethyl it is likely the ethyl will β-hydride eliminate quickly
upon thermal decomposition, thus if carbon content decreased the alkyl most likely is
the carbon source. Compound 9 was identified by 1H NMR δH (CDCl3, p.p.m.): 0.88
(3H, CH3), 1.55 (2H, CH2), 4.72 (5H, Cp). The CVD experiments are summarized in Table 3-2.
Conclusion
Compound 7 was synthesized and characterized. Preliminary data along with
experiments by Kanjolia et. al. indicate that 7 is a viable precursor for CVD of Ru thin
films. The model compound 8 has produced iron oxide thin films with varying iron and
oxygen content trending toward higher percent iron with the increase in deposition
temperatures.
Precursor Temperature
7 8 8 8 8 8 8 8 8
(°C) Reactor 200 200 250 200-400 250-100 250-575 400 300 250
Bubbler 45 RT 50 50 55 60 60 60 60
Heating Tapes 50 RT 60 60 55 60 60 60 60 Pressure (Torr)
Base 2 0.38 1 1 0.91 1.1 0.28 0.32 0.36
Reactor 16 5 5 5-400 2.6 350 350 350 350 Gases (sccm)
Carrier N2 (50) N2 (1000) N2 (100) N2 (30) N2 (1000) N2 (1000) N2 (100) N2 (100) N2 (100)
Co-Reactant H2 (75) NH3(30) NH3(30) NH3 (30) H2 (1000) H2 (1000) H2 (100) H2 (100) H2 (100)
Ambient N2 -- -- -- -- -- -- -- --
Substrate Si(100) Si(100) Si(100) Si(100) Si(100) Si(100)/Si(111) Si(100) Si(100) Si(100)
Composition (%) Ru -- -- -- -- -- -- -- -- --
Fe -- -- -- -- -- 36.7 26.9 38 40 O -- -- -- -- -- 61.1 21.1 21.8 27.8 C -- -- -- -- -- -- 52 40.2 32.2
Fe2O3 Fe-FexOy Fe-FexOy Fe-FexOy
Amorphous Amorphous Amorphous
Table 3-2. Parameters for selected CVD runs with compound 8.
(200)
Compounds
C C C
36
37
Experimental Section
General Procedures. All chemicals were purchased in reagent grade purity and
used with no further purification unless otherwise noted. All manipulations were carried
out using standard Schlenk and glove box techniques under an inert atmosphere of
argon or nitrogen. All solvents, unless otherwise noted, were purchased from Fisher
and passed through an M. Braun MB-SP solvent purification system or were distilled
from sodium/benzophenone prior to use. 1H and 13C NMR spectra were obtained on
Varian Gemini 300 and VXR 300 and Mercury 300 spectrometers. Infrared spectra
were measured on a Perkin-Elmer 1600 FT-IR.
CVD Experiments. The thin films were deposited using a custom-built vertical
quartz cold wall CVD reactor. A representative sample of parameters used is displayed
in Table 5. Film composition was determined by Auger electron spectroscopy (AES) or
XPS with a Perkin Elmer 5100 XPS System nominally at 15.0 kV and 300 W for the X-
ray source (monochromated Al X-rays). The sputtering ion was Ar with an accelerating
voltage of 4 KeV.
Bis(η5-cyclopentadienyldicarbonyl ruthenium)(10). Ru3(CO)12 (1.912 g, 2.991
mmol) was charged to a three neck round bottom flask outfitted with air inlet, a reflux
condenser, and a rubber septum. Next 3.0 mL of freshly distilled cyclopentadiene (12:1
molar ratio), and 40 mL dry heptane were added. The mixture was heated to reflux for
1 hr. The septum was removed to allow the heptane to evaporate to ~ 5 mL at which
time untreated (“wet” and oxygenated) heptane was added to the flask to restore initial
volume. The flask was once again sealed and allowed to reflux for an additional 3
hours. The solution was cooled and filtered. The solid collected from filtration was
38
washed with hexanes and then dried. The compound was identified by comparison to
literature data.65
1H NMR (CDCl3) δ 5.26 (s, 5H) and by IR with frequencies at 1774, 1933, 1952, 1995 cm-1
Sodium η5-cyclopentadienyldicarbonyl ruthenate (11). The dimer Ru2(CO)4Cp2
(1.252 g, 2.250 mmol) was dissolved in THF and cannula transferred into 3 wt% Na
amalgam in a 5:1 Na to Ru molar ratio. After 5 hours of stirring, the solution turned dark
red. The solution was separated from the mercury by cannula transfer and then
reserved in solution for the next step.
Dicarbonylmethylcyclopentadienyl ruthenium (7). To the THF solution
containing the anion of 11, 0.589 mL (11.250 mmol) of methyl iodide was added and
allowed to stir overnight. The THF was removed by trap to trap distillation and then final
product was isolated by sublimation at 40 °C (0.1 mmHg). The compound was identified
by 1H NMR (CDCl3) δ 5.23 (s, 5H), δ 0.31 (s, 3H).
Dicarbonylmethylcyclopentadienyl iron (8). MeLi (3.1 mL, 1.5 : 1 molar ratio of alkyl lithium : starting material) was added to CpFe(CO)2I (1.000 g, 3.290 mmol) in 30
mL Et2O and allowed to react for 1 h at -78 °C. Product was isolated in vacuo and
sublimed at 50°C (0.1 mmHg). The compound was identified by 1H NMR (CDCl3) δ 4.76
(s, 5H), δ 0.17 (s, 3H).66
Dicarbonylethylcyclopentadienyl iron (9). A 2 wt% NaHg amalgam was
prepared by slowly adding Hg (2.1 mL) to small pieces of Na (0.593 g), and stirring
vigorously. The dimer Cp2Fe2(CO)4 (3.02g, 8.35 mmol) was dissolved in THF (20 mL)
and added to the amalgam to reduce overnight. 3 equivalents of EtI (2.0 mL) were
39
added, and again reacted overnight. Upon completion, stirring was ceased, allowing the
NaI salt to settle to the bottom. The brown liquid layer at the top was cannula
transferred, through Celite, into a clean flask. Trap-to-trap distillation was performed to
remove solvent. The remaining solid was transferred to a small Schlenk flask, and ether
was evaporated over 2 days under strong flow of Ar. Compound 9 was dried under
vacuum to afford 15% yield.
40
CHAPTER 4 PRECURSORS FOR TUNGSTEN NITRIDE THIN FILMS
Background
Tungsten nitride is a promising refractory nitride for thin film diffusion barriers in
integrated circuits. Along with the beneficial properties associated with the refractory
nitrides, tungsten nitride has the lowest electrical resistivity making it an ideal candidate
in electronics. In addition there are no known reactions of WN with copper therefore
making it a good barrier material to prevent the diffusion of copper interconnects into the
silicon and/or silicon substrate.
Some examples of single-source precursors are bis(tert-butylamino)bis(tert-
butylimino)tungsten (12),67 bis(tert-butylimino)(guanidinato)tungsten hydride (13),68
bis(tert-butylimino)(di-tert-butyl pyrazolato)tungsten (14).69
tBu
NtBu H N N W
tBuN N N W
tBu
W NHtBu N N
tBuN N
tBuN NHtBu
N
N tBu
tBu
12 13 14 Figure 4-1. Single-source precursors for WN thin films.
Our group has reported WNx and WNxCy thin film deposition from two families of CVD precursors, tungsten imido and tungsten hydrazido complexes.70-75
The hydrazido compounds yielded a higher maximum nitrogen content (24 at %)
compared to their imido analogues (14 at %).76 The increased N incorporation into the
thin films with the hydrazido complexes could be due to the weaker N-N bond compared
41
to the N-C bond connecting the nitrido fragment with the rest of the ligand. NMR kinetic
studies of ligand exchange of the coordinated acetonitrile on the dimethyl hydrazido
complex concluded a low Gibbs free energy of activation, 14.4 kcal/mol.77 This
indicates the W-N bond between the metal center and the hydrazido nitrogen is weak
and is most likely the first bond to be broken in CVD conditions. After loss of the nitrile,
mass spectrometry data from the isopropyl and allyl imido compounds suggests the
cleavage of the N-C bond in the imido ligand while DFT calculations and in-situ Raman
spectroscopy suggest cleavage of the N-N bond in the hydrazido compounds.77,78
Further weakening of the bond between the nitrido fragment and the remainder of the complex and incorporating more nitrogen into the ligands could lead to thin films with
higher concentrations of nitrogen.
Results and Discussion
A new class of WNx and WNxCy compounds containing the general formula of
W(NNCR2)Cl4, where R = various alkyl and aromatic compounds (Figure 9) were the
next target precursors. The initial synthetic scheme to develop these novel compounds
was to first create the diazo ligand and then attach it to WCl4.
R R C
N
N
Cl W Cl
R = phenyl 15
tolyl 16 isobutyl 17
Cl Cl
N
C
CH3
Figure 4-2. Diazo-tungsten complex 15-17.
42
(Diphenylmethylene)hydrazine 18 was reacted with mercury oxide in petroleum
ether to afford the diphenyldiazo ligand 19. 1H NMR spectrum of 19 at room
temperature in chloroform-d3 showed aromatic peaks at δ 7.30 and 7.30 along with
some residual peaks from the starting material. Compound 19 was then reacted with
WCl4 in THF in attempts to make 15. The 1H NMR was inconclusive, however it did
show an increased amount of aromatic peaks shifted from that of the starting material.
Attempts at crystallization were unsuccessful leading to the exploration of the tolyl
derivative, which from past experience of ligand substitutions have yielded single
crystals more readily. To make compound 16, first (ditolylmethylene)hydrazine (20) was
synthesized from the reaction of ditolylketone with hydrazine in n-butanol. The 1H NMR
spectrum of 20 at room temperature in chloroform-d3 showed peaks at δ 7.14, 7.16,
7.33, and 7.36 for the aromatic hydrogens and at δ 2.40 for the methyl hydrogens and 5.35 for the ones on the amine.
Experimental Section
General Procedures. All chemicals were purchased in reagent grade purity and
used with no further purification unless otherwise noted. All manipulations were carried
out using standard Schlenk and glove box techniques under an inert atmosphere of
argon or nitrogen. All solvents, unless otherwise noted, were purchased from Fisher
and passed through an M. Braun MB-SP solvent purification system or were distilled
from sodium/benzophenone prior to use. 1H spectra were obtained on Varian Gemini
300 and VXR 300 and Mercury 300 spectrometers.
(Diazomethylene)dibenzene (19). Diphenyl hydrazine, (1.96 grams, 10.0 mmol)
was weighed out and added to 2.21 grams (10.2 mmol) of mercury oxide in a round
bottom flask containing ~20 mL of petroleum ether. The flask was put under argon and
43
a condenser was attached. The contents were heated to 50 °C for approximately 2
hours with a mineral oil bath. Afterwards the reaction was cooled to room temperature
and filtered through a fine glass frit via cannula transfer. The resulting liquid was purple;
the solvent was then pulled off in vacuo. 1H NMR (CDCl3): δ 7.15, 6.96 ppm.
4,4'-(Diazomethylene)bis(methylbenzene) (20). Di-tolyl ketone, 4.0 grams (0.019 mol) was charged to a Schlenk flask. Approximately 20 mL of absolute ethanol
was then added. In a 4:1 ratio hydrazine:ketone 5.6 mL, (0.095 mol) of hydrazine was
added via syringe. The mixture was left to reflux overnight at 120 C. It was then was
cooled to room temperature, filtered through a medium frit yielding a clear colorless
solution. This solution was cooled to ~-25C with a dry ice and a dichlorobenzene bath
for 2 hours. The precipitate was then filtered and dried in vacuo. 1H NMR (CDCl3): δ 7.11, 6.95, 2.09.
(Di-p-tolylmethylene)hydrazine (16). To a round bottom flask 0.276 grams (1.23
mmol) of 20 was added along with 0.268 grams (1.23 mmol) of HgO. The flask was then
charged with ~20 mL of petroleum ether and put under an argon flow. The contents
were heated to 50°C for 2 hours with an oil bath. Afterwards the reaction was cooled to
room temperature then filtered through a glass frit via cannula transfer The resulting
liquid was purple. The solvent was then pulled off in vacuo. 1H NMR (CDCl3): δ 7.37,
7.30, 7.18, 7.10 , 2.42, 2.32.
44
APPENDIX A NMR DATA
Ph
Zr 4
Figure A-1. 1H NMR spectrum of 3 in THF-d8 at -60 °C.
45
Ph
Zr 4
Figure A-2. 1H-13C gHMBC spectrum of 3 in THF-d8 at -60 °C.
46
Ph
Zr 4
Figure A-3. Expansion of the 1H-13C gHMBC spectrum of 3.
47
CO Ru
CO CH3
7
Figure A-4. 1H NMR of 7 in chloroform-d.
48
CO Fe
CO CH3
8
Figure A-5. 1H NMR of 8 in chloroform-d.
49
Et Fe
C C O O
9
Figure A-6. 1H NMR of 9 in chloroform-d.
50
Figure B-1. IR of 7.
APPENDIX B IR SPECTRUM
51
APPENDIX C X-RAY CRYSTALLOGRAPHY TABLES
Table C-1. Atomic coordinates ( x 104) and equivalent isotropic displacement
parameters (Å2 x 103) for 3.6
x y z U(eq) Zr 5000 2439(1) 2500 23(1) C1 4441(1) 3688(2) 1066(1) 34(1) C2 4154(1) 4303(2) 1576(1) 31(1) C3 4088(1) 4430(2) 2250(1) 30(1) C4 3747(1) 5176(2) 2721(1) 28(1) C5 3979(1) 6629(2) 3098(1) 42(1) C6 3656(1) 7319(2) 3556(2) 51(1) C7 3100(1) 6602(2) 3638(1) 45(1) C8 2858(1) 5173(2) 3258(1) 41(1) C9 3184(1) 4457(2) 2810(1) 34(1) C11 4471(1) 1185(2) 3377(1) 35(1) C12 4162(1) 580(2) 2567(1) 32(1) C13 4071(1) 458(2) 1814(1) 30(1) C14 3699(1) -244(2) 978(1) 29(1) C15 3905(1) -1675(2) 791(1) 45(1) C16 3543(1) -2318(2) -15(1) 54(1) C17 2971(1) -1548(2) -638(1) 45(1)
6 U(eq) is defined as one third of the trace of the orthogonalized Uij tensor.
52
Table C-2.
Bond lengths [Å] and angles [°] for 3.7
Zr-C12#1 2.4043(15) Zr-C12 2.4043(15) Zr-C2 2.4043(14) Zr-C2#1 2.4044(14) Zr-C3#1 2.4474(15) Zr-C3 2.4474(15) Zr-C13#1 2.4573(15) Zr-C13 2.4573(15) Zr-C11#1 2.4884(16) Zr-C11 2.4884(16) Zr-C1 2.4955(15) Zr-C1#1 2.4955(15) C1-C2 1.376(2) C1-H1A 0.99 C1-H1B 0.99 C2-C3 1.249(2) C3-C4 1.450(2) C4-C9 1.392(2) C4-C5 1.398(2) C5-C6 1.383(3) C5-H5A 0.95 C6-C7 1.371(3) C6-H6A 0.95 C7-C8 1.385(3) C7-H7A 0.95 C8-C9 1.383(2) C8-H8A 0.95 C9-H9A 0.95 C11-C12 1.374(2) C11-H11A 0.99 C11-H11B 0.99 C12-C13 1.247(2) C13-C14 1.452(2) C14-C19 1.390(2) C14-C15 1.391(2) C15-C16 1.387(3)
7 Symmetry transformations used to generate equivalent atoms:
#1 -x+1,y,-z+1/2
53
Table C-2. Continued
C15-H15A 0.95 C16-C17 1.378(3) C16-H16A 0.95 C17-C18 1.374(2) C17-H17A 0.95
C18-C19
1.383(2) C18-H18A 0.95 C19-H19A 0.95 C12#1-Zr-C12 96.41(8) C12#1-Zr-C2 138.02(6) C12-Zr-C2 98.49(5) C12#1-Zr-C2#1 98.49(5) C12-Zr-C2#1 138.01(6) C2-Zr-C2#1 96.11(7) C12#1-Zr-C3#1 87.54(6) C12-Zr-C3#1 167.81(5) C2-Zr-C3#1 86.01(5) C2#1-Zr-C3#1 29.81(5) C12#1-Zr-C3 167.81(5) C12-Zr-C3 87.54(6) C2-Zr-C3 29.81(5) C2#1-Zr-C3 86.01(5) C3#1-Zr-C3 90.96(7) C12#1-Zr-C13#1 29.70(5) C12-Zr-C13#1 86.70(5) C2-Zr-C13#1 167.66(5) C2#1-Zr-C13#1 87.24(5) C3#1-Zr-C13#1 91.19(5) C3-Zr-C13#1 162.49(5) C12#1-Zr-C13 86.71(5) C12-Zr-C13 29.70(5) C2-Zr-C13 87.24(5) C2#1-Zr-C13 167.66(5) C3#1-Zr-C13 162.49(5) C3-Zr-C13 91.18(5) C13#1-Zr-C13 91.97(7) C12#1-Zr-C11#1 32.56(5) C12-Zr-C11#1 105.29(6) C2-Zr-C11#1 105.46(5) C2#1-Zr-C11#1 108.32(5) C3#1-Zr-C11#1 84.21(5)
54
Table C-2. Continued
C3-Zr-C11#1 135.25(5) C13#1-Zr-C11#1 62.26(5) C13-Zr-C11#1 82.04(6) C12#1-Zr-C11 105.29(6) C12-Zr-C11 32.56(5) C2-Zr-C11 108.31(6) C2#1-Zr-C11 105.46(5) C3#1-Zr-C11 135.25(5) C3-Zr-C11 84.21(5) C13#1-Zr-C11 82.04(6) C13-Zr-C11 62.26(5) C11#1-Zr-C11 128.49(8) C12#1-Zr-C1 105.47(5) C12-Zr-C1 107.96(5) C2-Zr-C1 32.55(5) C2#1-Zr-C1 105.44(5) C3#1-Zr-C1 81.89(5) C3-Zr-C1 62.35(6) C13#1-Zr-C1 135.14(5) C13-Zr-C1 83.73(5) C11#1-Zr-C1 72.93(5) C11-Zr-C1 131.95(5) C12#1-Zr-C1#1 107.96(5) C12-Zr-C1#1 105.47(5) C2-Zr-C1#1 105.44(5) C2#1-Zr-C1#1 32.54(5) C3#1-Zr-C1#1 62.35(6) C3-Zr-C1#1 81.89(5) C13#1-Zr-C1#1 83.73(5) C13-Zr-C1#1 35.14(5) C11#1-Zr-C1#1 131.95(5) C11-Zr-C1#1 72.93(5) C1-Zr-C1#1 128.88(8) C2-C1-Zr 70.08(9) C2-C1-H1A 116.6 Zr-C1-H1A 116.6 C2-C1-H1B 116.6 Zr-C1-H1B 116.6 H1A-C1-H1B 113.6 C3-C2-C1 154.38(16) C3-C2-Zr 77.01(10) C1-C2-Zr 77.37(9)
55
Table C-2. Continued
C2-C3-C4 148.94(15) C2-C3-Zr 73.19(10) C4-C3-Zr 137.87(11) C9-C4-C5 118.64(15) C9-C4-C3 120.59(14) C5-C4-C3 120.77(15) C6-C5-C4 120.24(17) C6-C5-H5A 119.9 C4-C5-H5A 119.9 C7-C6-C5 120.65(17) C7-C6-H6A 119.7 C5-C6-H6A 119.7 C6-C7-C8 119.72(17) C6-C7-H7A 120.1 C8-C7-H7A 120.1 C9-C8-C7 120.26(17) C9-C8-H8A 119.9 C7-C8-H8A 119.9 C8-C9-C4 120.47(15) C8-C9-H9A 119.8 C4-C9-H9A 119.8 C12-C11-Zr 70.35(9) C12-C11-H11A 116.6 Zr-C11-H11A 116.6 C12-C11-H11B 116.6 Zr-C11-H11B 116.6 H11A-C11-H11B 113.6 C13-C12-C11 154.59(16) C13-C12-Zr 77.50(10) C11-C12-Zr 77.09(9) C12-C13-C14 149.68(16) C12-C13-Zr 72.80(10) C14-C13-Zr 137.51(11) C19-C14-C15 118.51(14) C19-C14-C13 119.95(14) C15-C14-C13 121.54(14) C16-C15-C14 120.47(16) C16-C15-H15A 119.8 C14-C15-H15A 119.8 C17-C16-C15 120.25(16) C17-C16-H16A 119.9 C15-C16-H16A 119.9
56
Table C-2. Continued
C18-C17-C16 119.74(16) C18-C17-H17A 120.1 C16-C17-H17A 120.1 C17-C18-C19 120.37(15) C17-C18-H18A 119.8 C19-C18-H18A 119.8 C18-C19-C14 120.65(14) C18-C19-H19A 119.7 C14-C19-H19A 119.7
Table C-3. Anisotropic displacement parameters (Å2 x 103) for 3.8
U11 U22 U33 U23 U13 U12 Zr 24(1) 25(1) 21(1) 0 9(1) 0 C1 36(1) 39(1) 26(1) 4(1) 12(1) 2(1) C2 28(1) 30(1) 29(1) 7(1) 8(1) 3(1) C3 26(1) 29(1) 32(1) 2(1) 10(1) 0(1) C4 27(1) 29(1) 26(1) 4(1) 9(1) 6(1) C5 44(1) 34(1) 53(1) -4(1) 27(1) -5(1) C6 67(1) 34(1) 61(1) -11(1) 35(1) -2(1) C7 59(1) 41(1) 47(1) 5(1) 34(1) 15(1) C8 38(1) 41(1) 49(1) 11(1) 26(1) 8(1) C9 32(1) 32(1) 38(1) 2(1) 15(1) 1(1) C11 36(1) 39(1) 32(1) 4(1) 17(1) -2(1) C12 29(1) 30(1) 38(1) 4(1) 15(1) -5(1) C13 27(1) 29(1) 32(1) 2(1) 10(1) 0(1) C14 28(1) 28(1) 30(1) 1(1) 12(1) -5(1) C15 45(1) 34(1) 39(1) -1(1) 4(1) 8(1) C16 64(1) 35(1) 48(1) -10(1) 12(1) 8(1) C17 52(1) 41(1) 32(1) -6(1) 9(1) -6(1) C18 34(1) 40(1) 34(1) 3(1) 6(1) -1(1) C19 31(1) 33(1) 36(1) 0(1) 11(1) 4(1)
8 The anisotropic displacement factor exponent takes the form: -2p2[ h2 a*2U11 + ... + 2 h k a* b* U12 ]
57
Table C-4. Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Å2x 103) for 7.9
Ru1
x 897(1)
y 4939(1)
z 8267(1)
U(eq) 20(1)
O1 -1576(5) 6976(3) 9352(3) 56(1) O2 -1375(5) 3063(3) 9705(3) 54(1)
O3 - 2285(17) 4763(11) 6344(10) 53(3)
C1 3359(5) 5832(4) 7268(4) 34(1) C2 3871(5) 5843(3) 8457(3) 36(1) C3 4001(6) 4585(3) 8845(3) 33(1) C4 3589(5) 3788(3) 7878(3) 29(1) C5 3221(5) 4549(3) 6911(3) 29(1) C6 -611(5) 6232(3) 8945(3) 29(1) C7 -513(5) 3746(3) 9163(3) 28(1) C8 -1246(6) 4841(5) 6971(4) 26(1) C8' -970(20) 4521(18) 7103(12) 44(5)
9 . U(eq) is defined as one third of the trace of the orthogonalized Uij tensor.
58
Table C-5. Bond lengths [Å] and angles [°] for 7. Ru1-C6 1.886(3) Ru1-C7 1.894(3) Ru1-C8' 1.904(5) Ru1-C8 2.098(4) Ru1-C1 2.255(3) Ru1-C4 2.263(3) Ru1-C5 2.270(3) Ru1-C3 2.270(4) Ru1-C2 2.272(4) O1-C6 1.131(4) O2-C7 1.124(4) O3-C8' 1.283(14) C1-C2 1.408(5) C1-C5 1.421(5) C1-H1A 0.95 C2-C3 1.407(5) C2-H2A 0.95 C3-C4 1.422(5) C3-H3A 0.95 C4-C5 1.394(4) C4-H4A 0.95 C5-H5A 0.95 C8-H8A 0.98 C8-H8B 0.98 C8-H8C 0.98 C6-Ru1-C7 88.74(12) C6-Ru1-C8' 94.9(6) C7-Ru1-C8' 83.1(6) C6-Ru1-C8 86.53(17) C7-Ru1-C8 89.46(17) C8'-Ru1-C8 10.6(6) C6-Ru1-C1 108.61(15) C7-Ru1-C1 160.10(15) C8'-Ru1-C1 104.4(6) C8-Ru1-C1 100.95(16) C6-Ru1-C4 157.41(15) C7-Ru1-C4 99.71(14) C8'-Ru1-C4 106.8(6) C8-Ru1-C4 114.25(16) C1-Ru1-C4 60.59(13)
59
Table C-5. Continued
C6-Ru1-C5 143.35(13) C7-Ru1-C5 127.74(14) C8'-Ru1-C5 87.3(6) C8-Ru1-C5 90.12(14) C1-Ru1-C5 36.60(14) C4-Ru1-C5 35.82(11) C6-Ru1-C3 121.24(15) C7-Ru1-C3 102.41(14) C8'-Ru1-C3 143.3(6) C8-Ru1-C3 149.53(15) C1-Ru1-C3 60.58(12) C4-Ru1-C3 36.56(12) C5-Ru1-C3 60.37(11) C6-Ru1-C2 98.71(15) C7-Ru1-C2 133.71(15) C8'-Ru1-C2 140.6(6) C8-Ru1-C2 136.33(16) C1-Ru1-C2 36.25(14) C4-Ru1-C2 60.44(13) C5-Ru1-C2 60.40(12) C3-Ru1-C2 36.10(13) C2-C1-C5 107.7(3) C2-C1-Ru1 72.5(2) C5-C1-Ru1 72.3(2) C2-C1-H1A 126.2 C5-C1-H1A 126.2 Ru1-C1-H1A 120.8 C3-C2-C1 108.3(3) C3-C2-Ru1 71.9(2) C1-C2-Ru1 71.2(2) C3-C2-H2A 125.8 C1-C2-H2A 125.8 Ru1-C2-H2A 122.7 C2-C3-C4 107.6(3) C2-C3-Ru1 72.0(2) C4-C3-Ru1 71.5(2) C2-C3-H3A 126.2 C4-C3-H3A 126.2 Ru1-C3-H3A 122 C5-C4-C3 108.3(3) C5-C4-Ru1 72.3(2) C3-C4-Ru1 72.0(2)
60
Table C-5. Continued
C5-C4-H4A 125.9 C3-C4-H4A 125.9 Ru1-C4-H4A 121.5 C4-C5-C1 108.1(3) C4-C5-Ru1 71.84(19) C1-C5-Ru1 71.1(2) C4-C5-H5A 125.9 C1-C5-H5A 125.9 Ru1-C5-H5A 122.7 O1-C6-Ru1 177.3(4) O2-C7-Ru1 178.3(3) Ru1-C8-H8A 109.5 Ru1-C8-H8B 109.5 H8A-C8-H8B 109.5 Ru1-C8-H8C 109.5 H8A-C8-H8C 109.5 H8B-C8-H8C 109.5 O3-C8'-Ru1 155.0(15)
Table C-6. Anisotropic displacement parameters for 7.
Ru1
U11 15(1)
U22 21(1)
U33 24(1)
U23 1(1)
U13 1(1)
U12 1(1)
O1 52(2) 45(2) 72(2) - 8(2) 13(1) 12(2)
O2
56(2)
46(2)
60(2)
12(1)
11(2) - 11(1)
C1 20(2) 41(2) 42(2) 16(2) 5(2) -2(1)
C2 19(2) 44(2) 44(2) - 16(2) 4(2) -
10(1) C3 19(2) 54(2) 25(1) 0(1) -2(1) 1(2) C4 18(2) 35(2) 32(2) 3(1) 3(1) 7(1) C5 18(2) 53(2) 17(1) -1(1) 2(1) -4(1) C6 25(2) 33(2) 31(2) 2(1) 3(1) 3(2) C7 26(2) 29(2) 28(2) 2(1) 1(1) -3(1)
61
APPENDIXD MOLECULAR ORBITAL DIAGRAM OF 4
The molecular orbital diagram of 4 was generated using Microsoft Excel.
eV 0.5 Orbital Energy
-0.5
-1.5
-2.5
LUFO
-3.5
HOFO
-4.5
·5.5
·6.5
-7.5
-8.5
Zr
Zr(CH2CCH)4 4L
HOFO
-+-•1
--bl
"""*""b2
62
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BIOGRAPHICAL SKETCH
Dan Denomme was born in 1981, in Redford, MI. Science was an interest as
early as age 7 when he wanted to be a paleontologist. This desire lasted for almost a
full year before he realized it required digging in dirt. While attending Central Michigan
University Dan worked for Dow Chemical in Midland, MI as a technical co-op in the
water-soluble polymer research laboratories. In 2007, he received his B.S. in chemistry
from CMU and enrolled in graduate school and joined the research group of Prof. Lisa
McElwee-White. He received his Master of Science degree from the University of
Florida in the fall of 2012.