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  • 7/29/2019 8- Chun_J. Appl. Phys_1999

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    Dense fully 111-textured TiN diffusion barriers: Enhanced lifetime throughmicrostructure control during layer growthJ.-S. Chun, I. Petrov, and J. E. GreeneCitation: J. Appl. Phys. 86, 3633 (1999); doi: 10.1063/1.371271View online: http://dx.doi.org/10.1063/1.371271View Table of Contents: http://jap.aip.org/resource/1/JAPIAU/v86/i7Published by theAmerican Institute of Physics.Related ArticlesEvaluation and modeling of lanthanum diffusion in TiN/La2O3/HfSiON/SiO2/Si high-k stacks

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    Dense fully 111-textured TiN diffusion barriers: Enhanced lifetime throughmicrostructure control during layer growth

    J.-S. Chun, I. Petrov, and J. E. Greenea)

    Materials Science Department, Materials Research Laboratory, and Coordinated Science Laboratory,University of Illinois, 1101 West Springfield Avenue, Urbana, Illinois 61801

    Received 16 April 1999; accepted for publication 24 June 1999

    Low-temperature deposition of TiN by reactive evaporation or sputter deposition onto amorphoussubstrates leads to highly underdense layers which develop mixed 111/002 orientations through

    competitive growth. In contrast, we demonstrate here the growth of low-temperature 450 C fully

    dense polycrystalline TiN layers with complete 111 texture. This was achieved by reactive

    magnetron sputter deposition using a combination of: 1 highly oriented 25-nm-thick 0002 Ti

    underlayers to provide 111 TiN orientation through texture inheritance local epitaxy and 2 high

    flux (JN2/JTi14), low-energy (EN

    220eV), N2

    ion irradiation in a magnetically unbalanced

    mode to provide enhanced adatom diffusion leading to densification during TiN deposition. The Ti

    underlayers were also grown in a magnetically unbalanced mode, in this case with an incident

    Ar/Ti flux ratio of 2 and EAr11 eV. All TiN films were slightly overstoichiometric with a N/Ti

    ratio of 1.020.03. In order to assess the diffusion-barrier properties of dense 111-textured TiN, Al

    overlayers were deposited without breaking vacuum at 100 C. Al/TiN bilayers were then annealed

    at a constant ramp rate of 3 C s1 to 650 C s1 and the interfacial reaction between Al and TiN

    was monitored by in situ synchrotron x-ray diffraction measurements. As a reference point, we findthat interfacial Al3Ti formation is observed at 450 C in Al/TiN bilayers in which the TiN layer is

    deposited directly on SiO2 in a conventional magnetically balanced mode and, hence, is underdense

    with a mixed 111/002 orientation. However, the onset temperature for interfacial reaction was

    increased to 610 C in bilayers with fully dense TiN exhibiting complete 111 preferred orientation.

    1999 American Institute of Physics. S0021-8979 99 04119-5

    I. INTRODUCTION

    Al-based interconnects with TiN diffusion barriers are

    widely used in multilevel metallization architectures incor-

    porated in submicron ultralarge-scale integrated ULSI de-

    vices. As the dimensions of integrated circuits continue to

    decrease while their packing density increases, interconnec-

    tion reliability issues such as electromigration resistance and

    diffusion barrier lifetime become increasingly important. It is

    well known1 5 that electromigration lifetimes are enhanced

    in Al metal lines having a large average grain size, a small

    grain-size distribution, and strong 111 texture. Shibata et al.6

    found that the dominant factor for Al linewidths below 0.5

    m is the degree of 111 preferred orientation.

    Texture control can also be important for controlling the

    stability of heterointerfaces during high temperature process-

    ing. Both the rate and extent of reaction at metal/diffusionbarrier interfaces have been shown to depend upon film

    texture.7,8 In all previous studies718 of polycrystalline Al/

    TiN interfacial reactions, there were no attempts made to

    control TiN film texture or, except for Refs. 7 and 9, poros-

    ity. In fact, the TiN layers are often uncharacterized. Under

    typical industrial deposition conditions, sputter-deposited

    TiN is underdense with a mixed 111/002 texture.4,7 Al/TiN

    interfacial reactions, the formation of Al3Ti, and barrier fail-

    ure occur during isothermal annealing for 30 min at tempera-

    tures below 400 C.19 Air-exposure leading to oxide forma-

    tion prior to Al deposition has been shown to increase the

    thermal stability of the barrier layer.19 However, the resultsare not reproducible. Moreover, air-exposure reduces the de-

    gree of Al 111 texture and increases the contact resistance.

    Greene et al.20,21 has shown that the preferred orienta-

    tion of polycrystalline TiN films grown by ultrahigh-vacuum

    UHV reactive-magnetron sputter deposition on amorphous

    SiO2 at 350C in pure N2 discharges can be controllably

    varied from essentially complete 111 to purely 002 by vary-

    ing the incident ion/metal flux ratio Ji/JTi from 1 to 5

    while the ion energy EN2 is maintained constant at 20 eV.

    The incident ions are predominantly N2 96.3% ,22 corre-

    sponding to 10 eV per incident N, well below the lattice

    displacement threshold. During low-temperature deposition

    in the absence of significant ion irradiation (Ji/JTi1), TiN

    initially exhibits a mixed texturepredominantly 111, 002,

    and 022and then slowly evolves to a strong 111 texture

    containing a network of both inter- and intracolumnar poros-

    ity due to the combination of low adatom mobilities and

    competitive columnar growth. Increasing Ji/JTi5 results in

    enhanced adatom mobilities giving rise to a dense micro-

    structure. In addition, the low-surface-energy 002 texture

    now dominates even at submonolayer coverage and there isa Electronic mail: [email protected]

    JOURNAL OF APPLIED PHYSICS VOLUME 86, NUMBER 7 1 OCTOBER 1999

    36330021-8979/99/86(7)/3633/9/$15.00 1999 American Institute of Physics

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    no longer any indication of competitive growth as 002 col-

    umns grow essentially straight up.20,21

    Obtaining a dense TiN layer with complete 111 texture

    at low growth temperatures, as required for diffusion barrier

    and many hard-coating applications, is a challenging growth

    kinetics problem. Moving toward higher growth tempera-

    tures favors the development of the 002 texture,23 rather than

    111, since 002 is the low-energy surface for TiN.24 In ad-

    dition, the use of ion irradiation to promote densification of111-textured TiN leads to either 002 preferred orientation as

    noted above for low ion energies with high ion-to-neutral

    ratios20,21 or very high in-plane compressive stress and

    mixed texture with higher energies and low ion-to-neutral

    ratios.23

    In this article, we show, for the first time, that fully

    dense completely 111-textured TiN layers can be achieved at

    low growth temperatures using a combination of 1 highly

    oriented 25-nm-thick 0002 Ti underlayers to provide 111

    orientation through texture inheritance local epitaxy and 2

    high-flux (JN2/JTi14), low-energy (EN

    220eV), N2

    ion

    irradiation to provide enhanced adatom diffusion leading to

    densification. Both the Ti and TiN layers were grown in a

    magnetically unbalanced mode. While interfacial Al3Ti for-

    mation was observed at 450 C in Al/TiN bilayers with un-

    derdense TiN having a mixed texture, the onset temperature

    was increased to 610 C for bilayers with fully dense 111

    TiN. The Al overlayers are dense in both cases, but exhibit

    much stronger 111 texture i.e., texture inheritance on dense

    111 TiN.

    II. EXPERIMENTAL PROCEDURE

    All films were grown in a load-locked multichamber

    UHV stainless-steel dc magnetron sputter deposition systemwhich has been described in detail elsewhere.25 The pressure

    in the sample introduction chamber was reduced to less than

    5108 Torr 7106 Pa) prior to initiating substrate ex-

    change into the deposition chamber which has a base pres-

    sure of 51010 Torr 7108 Pa). For the present experi-

    ments, an additional magnetron-sputtering source with

    separate water cooling lines and shutter was added in the

    viewport flange opposing the original source. The Ti target

    99.999% pure was operated in a magnetically unbalanced

    mode for the growth of both Ti and TiN films while the Al

    target 99.999% pure was sputtered in a magnetically bal-

    anced mode. Target-to-substrate separations were 6.5 cm for

    TiN and 10 cm for Al deposition.A pair of external Helmholtz coils with Fe pole pieces

    were utilized to create a uniform axial magnetic field Bextin the region between the target and the substrate. The posi-

    tive and negative signs refer to geometries in which B ext aids

    and opposes, respectively, the field of the outer pole of the

    magnetron. B ext has a strong effect on the ion flux incident at

    the substrate, with only minor effects on the target atom

    flux.25

    The substrates used in these experiments were thermally

    oxidized 11 cm2 Si 001 wafers with an SiO2 thickness of

    0.6 m. They were cleaned with successive rinses in ultra-

    sonic baths of trichloroethane, acetone, ethanol, and deion-

    ized water and blown dry with dry N2 . The wafers were

    mounted on resistively heated Ta platens using Mo clips and

    inserted into the sample introduction chamber for transport

    to the growth chamber where they were thermally degassed

    at 800 C for 1 h. The substrate temperature Ts was then

    adjusted to 450 C as the Ti target was sputter etched for 5

    min while shielding the substrate and Al target. Reported Tsvalues, which were calibrated using a 0.25-mm-diam

    chromelalumel thermocouple bonded to the surface of asacrificial substrate using Ag paste, include the contribution

    from plasma heating.

    Plasma characteristics in the vicinity of the substrate

    were determined as a function of B ext from electrical mea-

    surements, following the procedures described in Refs. 25

    and 26, obtained using both disk-shaped and cylindrical

    probes. Most of the ions incident at the substrate experience

    the full substrate sheath potential Vs(VbVp), where Vpis the plasma potential and Vb is substrate bias, since the

    mean-free path for charge exchange collisions,27 8 mm, is

    more than an order of magnitude larger than the sheath

    width,

    28

    estimated from the ChildLangmuir equation. In thepresent experiments, Vb is equal to the floating potential Vfand the ion energy Ei at the substrate is e ( VfVp ).

    Two sets of TiN layers were grown with Ts450 C at

    the relatively high sputtering pressure of 20 mTorr

    N2(99.999%), chosen to suppress kinetic energy transfer to

    the growing film by particles backscattered from the target.

    In sample set i, TiN layers, 160 nm thick, were deposited on

    SiO2 with JN2/JTi1 and EN

    220eV (Vp3 V and Vf

    17V). The ion current density at the substrate,

    j N20.12 mA cm2 corresponding to an ion flux

    JN27.51014 cm2 s1), was obtained using an external

    axial magnetic field B ext of20 G. These conditions resultedin a deposition rate R of 6.0 nm min1. The second set of

    TiN layers, series ii, were grown on 25-nm-thick Ti under-

    layers deposited on SiO2 at Ts80 C in 20 mTorr Ar

    99.999% with an incident Ar/Ti flux ratio of 2

    (JAr6.11015 cm2 s1 obtained with Bext200 G), and

    an Ar ion energy EAr11 eV (Vp12.5 V and Vf23.5 V). The TiN overlayers, 140 nm thick, were then

    deposited without breaking vacuum using JN2/JTi14

    (JN21.61016 cm2 s1 achieved with B ext150 G) and

    EN223eV (Vp11V and Vf34 V). The deposition

    rates R of Ti and TiN were 30 and 5.4 nm min1, respec-

    tively.Calculations carried out using the TRIM90 computer

    code,29 combined with Monte Carlo gas transport simula-

    tions based upon energy-dependent scattering cross

    sections,30 show that for the TiN growth conditions de-

    scribed above, a majority of both the sputter-ejected species

    and the energetic neutrals backscattered from the target are

    thermalized during gas-phase transport and contribute little

    to the total kinetic energy transfer to the substrate and grow-

    ing film. The ion flux to the substrate is due, as determined

    by double-modulated mass spectroscopy measurements,22

    primarily to N2(96.3%) with the remainder being

    N(3.5%) and Ti(0.2%).

    3634 J. Appl. Phys., Vol. 86, No. 7, 1 October 1999 Chun, Petrov, and Greene

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    Immediately following TiN deposition, for both series i

    and ii, Ts was decreased to 100 C and 160-nm-thick Al

    overlayers were grown in 5 mTorr Ar discharges without

    breaking vacuum. The Al deposition rate was 71.1 nm min1

    with an incident Ar/Al flux ratio of 0.8 and EAr10 eV.

    The microstructure and microchemistry of as-deposited

    and annealed samples were determined using a combination

    of Rutherford backscattering spectroscopy RBS , x-ray dif-

    fraction XRD , and plan-view and cross-sectional transmis-sion electron microscopy TEM and XTEM . The RBS probe

    beam consisted of 2 MeV He ions incident at an angle of

    22.5 relative to the sample surface normal with the detector

    set at a 150 scattering angle. Backscattered spectra were

    analyzed using the RUMP simulation program.31 The uncer-

    tainty in determining the N/Ti ratio was less than 0.03. TiN

    exhibits a wide single-phase field with a N/Ti ratio extending

    from0.6 to 1.2.32 In the present experiments, all TiN films,

    irrespective of Ji/JTi , were found to be slightly oversto-

    ichiometric with N/Ti1.020.03, as expected for low-

    temperature growth in pure N2 discharges.

    XRD 2 and -rocking curves were obtained using

    Cu K radiation in a system equipped with a double-crystalspectrometer to provide a resolution of 0.01 2 in the pow-

    der diffraction mode 45 kV, 20 mA, 1 divergent slit . The

    TEM and XTEM analyses were carried out using Philips

    CM12 and Hitachi 9000 electron microscopes operated at

    120 and 300 kV, respectively. Sample preparation for TEM/

    XTEM examination followed the procedure outlined in Ref.

    21.

    The surface morphologies of as-deposited TiN films

    were investigated using atomic force microscopy AFM .

    The measurements were carried out in a Digital Nanoscope

    II microscope operated in air in the contact mode with oxide-

    sharpened Si3

    N4

    tips having radii of 540 nm.

    In situ x-ray diffraction XRD measurements during

    sample annealing were performed at the Brookhaven Na-

    tional Synchrotron Light Source, beamline X-20C. As-

    deposited samples were loaded in an annealing chamber

    aligned to the beamline and equipped with an x-ray transpar-

    ent Be window. The chamber was evacuated to 5

    106 Torr, backfilled with purified He, re-evacuated, and

    then backfilled with 1 atm of He. As-deposited samples were

    annealed using linear temperature ramps from 100 to 650 C

    at 3 C s1. A high-intensity monochromator employing

    bandpass multilayer filters provided an energy resolution of

    1.5% at 6.9 keV 0.1797 nm with a typical intensity at the

    sample of 3

    10

    12

    photons s

    1

    . The incident x rays illumi-nated a sample area 15 mm2. Diffraction scans were col-

    lected using a position-sensitive detector with time resolution

    of ms.

    III. EXPERIMENTAL RESULTS AND DISCUSSION

    Figure 1 a is an XTEM micrograph from a TiN layer

    grown directly on SiO2 with JN2/JTi1 and EN

    220 eV,

    conditions corresponding to TiN sample series i. The micro-

    graph is typical of TiN films grown under weak ion irradia-

    tion conditions at Ts500C (Ts /Tm0.2). The layer is

    underdense due to limited adatom mobilities leading to

    atomic shadowing which, in turn, results in a columnar mi-

    crostructure with both inter- and intracolumnar voids.20,21

    Careful analyses, using nanodiffraction and high-

    resolution XTEM, of the region near the film/substrate inter-

    face show that the layer initially nucleates with islands lead-

    ing to grains which are predominantly broad-based 002 and

    narrow 111. However, the 111 grains eventually overgrow

    the 002 via a competitive growth mechanism. That is, diffu-sion on the low-energy 002 surface24in which there is only

    one adatom backbondis fast, leading to islands spreading

    out relatively rapidly and accounting for the broad-based 002

    columns, compared to the 111 surface where each adatom

    has three backbonds. Thus, the steady-state adatom density

    on 002 islands is low as adatoms quickly move to the edges,

    while 111 grains grow upwards rapidly and intercept ever

    larger fractions of the incoming flux. While the majority of

    the 002 grains are overgrown early in the growth process,

    some survive even in films with thicknesses up to 1 m.21

    The open intercolumnar boundaries observed in low-

    temperature 111-oriented transition-metal nitride layers e.g.,

    TiN,20,21 Ti1xAlxN, 33 and ScN34 is simply a consequenceof the effect of the atomic shadowing process during texture

    evolution via competitive growth combined with the distri-

    bution of particle incidence angles. Figure 1 a also shows

    that the sample surface is rough and faceted, as commonly

    observed for films with voided column boundaries. The layer

    thickness determined from the micrograph is 160 nm, in

    good agreement with the deposition rate calibration.

    Figure 1 b is a -2 XRD scan from the series i layer

    shown in Fig. 1 a . The pattern contains an intense 111 peak

    and a small 002 peak, both at positions corresponding to

    B1-NaCl-structure TiN. The integrated 111 to 002 peak in-

    tensity ratio I111/I002 is 8.8, a factor of 14 higher than that

    FIG. 1. a Bright-field XTEM micrograph and b corresponding -2XRD

    scan from an as-deposited series-i TiN layer grown on SiO 2 at 450 C with

    JN2 /JTi1 and EN

    220 eV.

    3635J. Appl. Phys., Vol. 86, No. 7, 1 October 1999 Chun, Petrov, and Greene

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    obtained from randomly oriented TiN powder. Thus, the

    dominant texture at this film thickness is 111 in agreement

    with the XTEM results discussed above. The 111 interplanar

    spacing d111 is 0.244 nm which is close to the reported bulk

    value of 0.2449 nm and indicates that the layer is nearly fully

    relaxed. The full width at half maximum FWHM intensity

    of the 111 -rocking curve, not shown, is 23.1. The

    large value of is consistent with kinetically limited com-

    petitive texture evolution.

    Low-energy, high-flux, N2 irradiation during growth

    densifies the TiN microstructure leaving no residual ion-

    induced defects detectable by XRD and TEM.20,21 However,

    the layers also exhibit complete 002 preferred orientation.Thus, in an attempt to obtain TiN layers which are both

    dense and have complete 111 texture, we have carried out

    experiments combining intense N2 ion irradiation with the

    use of a dense 0002 oriented hcp Ti underlayer as a crystal-

    lographic template sample series ii . The hcp Ti basal plane

    and the fcc TiN 111 plane the NaCl crystal structure is fcc

    with a two-atom basis have the same two-dimensional sym-

    metry. Moreover, Ti underlayers are often used in multilevel

    interconnections to provide enhanced adhesion between the

    diffusion barrier and SiO235 and lower contact resistance

    with Si.36

    Figure 2 is a schematic view of the atomic arrangement

    at the interface between 0002 Ti and 111 TiN layers. The

    misfit along equivalent close-packed directions in TiN 111

    and Ti 0002 is approximately 1.6% with xTiN0.29995 nm

    and x Ti0.29503 nm. 111 is a polar direction in TiN with

    alternate 111 planes consisting of all Ti and all N atoms.

    Preferred orientation in metal films, as opposed to

    transition-metal nitride layers, typically corresponds to the

    low-energy surface even at low growth temperatures37 due to

    FIG. 2. Schematic view of the atomic arrangement at the interface between

    Ti 0002 and TiN 111 layers.

    FIG. 3. a -2 XRD scan of an as-deposited Ti layer grown on SiO2 at80 C with an incident Ar/Ti flux ratio of 2 and EAr11 eV. b An 0002

    -rocking curve and c a bright-field plan-view TEM micrograph from the

    same sample.

    3636 J. Appl. Phys., Vol. 86, No. 7, 1 October 1999 Chun, Petrov, and Greene

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    much higher adatom mobilities on metal surfaces. In thepresent experiments, Ti underlayers grown on SiO2 at 80 C

    (Ts /Tm18%) were found to be 0002. However, to enhance

    the degree of orientation, we employed low-energy Ar ir-

    radiation through the use of magnetically unbalanced sputter

    deposition to provide, at the growth surface, an ion-to-metal

    flux ratio JAr/JTi2 with EAr11 eV.

    Figure 3 a is a -2 XRD scan of an as-deposited Ti

    layer. The only peaks observed are 000l ( l2,4,...) whereas

    for Ti powder patterns the strongest peak is 1011 2

    40.17 with an intensity ratio I1011 /I00023.4. We obtain

    an 0002 interplanar spacing d0002 of 0.2342 nm in agreement

    with the reported bulk value, 0.2341.38 The -rocking curve

    shown in Fig. 3 b has a FWHM value 3.3. A bright-

    field plan-view TEM micrograph of the same sample isshown in Fig. 3 c . The absence of Moire fringes is indica-

    tive of a columnar structure. However, the individual grains

    appear fully dense with no evidence of either inter- or intra-

    grain porosity. The average Ti grain size obtained from plan-

    view TEM images using image analysis software39 is 2621

    nm.

    Immediately following growth of the oriented Ti under-

    layers, TiN was deposited at P N220mTorr and Ts

    450 C with JN2/JTi14 and EN

    220 eV. Figure 4 a is

    a typical bright-field XTEM micrograph from an as-

    deposited TiN/Ti bilayer structure. TiN and Ti layer thick-

    nesses determined from the micrographs are 160 and 5 nm,

    FIG. 4. a Bright-field XTEM micrograph from an as-deposited series-ii

    TiN/Ti bilayer structure. The TiN layer was grown at 450 C with

    JN2 /JTi14 and EN

    220 eV. b A -2 XRD scan and c a 111

    -rocking curve from the same sample.

    FIG. 5. High-resolution XTEM micrograph of the TiN/Ti interface from the

    sample corresponding to Fig. 4.

    3637J. Appl. Phys., Vol. 86, No. 7, 1 October 1999 Chun, Petrov, and Greene

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    respectively. The decrease in the Ti thickness from 25 to 5

    nm indicates that 80% of the underlayer has reacted with

    the incident N2 flux, due to the high N2/Ti ratio used in these

    experiments, to form TiN during the initial stages of nitride

    deposition. There are two important points to note in this

    micrograph. The first is that this TiN layer, in contrast to the

    sample in Fig. 1 a , is dense with no detectable inter- or

    intracolumnar porosity. The film appears fully dense even in

    high-resolution micrographs. The second point is that Fig.

    4 a reveals no indication of competitive 111/002 grain

    growth. In fact, all TiN columns are 111 and grow commen-

    surately with the underlying transformed TiN grains as will

    be shown below using high-resolution XTEM HR-XTEM .

    Figure 4 b is a -2XRD scan from the type-ii bilayer

    sample corresponding to Fig. 4 a . Consistent with the

    XTEM results, and in contrast to XRD scans from the type-i

    TiN layer grown with no intentional ion irradiation and with-

    out the oriented Ti underlayer, only the 111 peak is obtainedwith no evidence of a residual 002 feature. The d111 lattice

    spacing is 0.2442 nm in reasonable agreement with the bulk

    value indicating that the layer is relaxed. XRD pole figures

    not shown obtained with 2 set to the 111 Bragg angle for

    TiN confirm that the film texture is azimuthally symmetric

    i.e., it exhibits fiber texture . No other diffraction peaks

    were detected in either pole figures or -2 scans. The lack

    of Ti reflections is due to the fact that most of the underlayer,

    as shown in the XTEM micrograph in Fig. 4 a , was trans-

    formed to TiN. The 111 -rocking curve in Fig. 4 c is ex-

    tremely narrow, 1.9, compared to the FWHM obtained

    from the type-i layer, 23.1. Thus, the mosaicity is

    greatly reduced giving rise to a factor of16 increase in thein-plane coherence length.

    A HR-XTEM bright-field image of the TiN/Ti interface

    in Fig. 4 a is presented in Fig. 5. It shows clearly, together

    with high and lower-magnification images obtained from dif-

    ferent regions of the same sample, that cubic 111 TiN grains

    grow with a local epitaxial relationship to hexagonal 0002 Ti

    grains: TiN111Ti0002 . The TiN/Ti interface is locally coher-

    ent with TiN and Ti exhibiting equal in-plane grain sizes.

    The micrograph also shows that the Ti/SiO2 interface re-

    mains abrupt.

    Figures 6 a and 6 b are plan-view TEM micrographs

    showing a direct comparison of the microstructure of type-i

    FIG. 6. Bright-field plan-view TEM micrographs of a series-i and b

    series-ii TiN/Ti bilayers.

    FIG. 7. AFM images of the samples shown in a Fig. 6 a and b Fig. 6 b .

    3638 J. Appl. Phys., Vol. 86, No. 7, 1 October 1999 Chun, Petrov, and Greene

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    TiN films grown by conventional reactive magnetron sput-

    tering and type-ii TiN layers grown under intense low-

    energy N2 irradiation and with an oriented Ti underlayer.

    Both TiN films were deposited at Ts450 C with

    EN220 eV. However, the series-i film in Fig. 6 a grown

    with JN2/JTi1 exhibits an underdense structure consistent

    with the XTEM micrograph in Fig. 1 a with a mixed tex-

    ture which is predominantly 111. The intercolumn voids

    have widths of up to 2 nm. In contrast, the series-ii layer in

    Fig. 6 b is fully dense with a complete 111 texture. Averagegrain sizes d measured near the top of the underdense anddense TiN films are 2014 and 4330 nm, respectively.

    Since the average grain size of the as-deposited Ti under-

    layer is 2621 nm, d in the 111 TiN overlayer grainsincreases with layer thickness. This can be also seen in the

    XTEM micrograph in Fig. 4 a .

    Figures 7 a and 7 b are AFM images of the TiN films

    corresponding to Figs. 6 a and 6 b . The 160-nm-thick un-

    derdense series-i TiN layer in Fig. 7 a is extremely rough

    with a root-mean-square surface width w 8.5 nm and anin-plane surface coherence length 78 nm. The same

    thickness dense series-ii 111-oriented TiN layer Fig. 7 b

    grown on the 0002 Ti template is much smoother with w

    3.3 nm and 49 nm.In order to examine the effects of texture, microstruc-

    ture, and surface roughness on the diffusion barrier proper-

    ties of TiN, 160-nm-thick Al overlayers grown with

    JAr/JAl0.8 and EAr10 eV were deposited at

    PAr5 mTorr and Ts100 C on both series-i and series-ii

    TiN layers without breaking vacuum. Figures 8 a and 8 b

    are typical XTEM micrographs from Al/TiN diffusion-

    barrier test structures. Both Al overlayers were fully dense

    with average grain sizes, obtained from plan-view images, of

    210 nm. They exhibited quite different degrees of pre-

    ferred orientation, however, and the surface of the Al film

    grown on the type-i TiN layer is much rougher with an in-

    FIG. 8. Bright-field XTEM micrographs from a series-i Al/TiN and b

    series-ii Al/TiN bilayers.

    FIG. 9. -2 XRD scans from as-deposited a series i and b series-ii

    Al/TiN bilayers. c Al 111 -rocking curve from the sample corresponding

    to b .

    3639J. Appl. Phys., Vol. 86, No. 7, 1 October 1999 Chun, Petrov, and Greene

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    plane wavelength of the order of the grain size.

    -2 XRD scans from the Al/TiN bilayers in Figs. 8 a

    and 8 b are shown in Figs. 9 a and 9 b . The patterns dem-

    onstrate that the Al film grown on TiN with mixed 111/002

    texture also exhibits a mixed orientation Fig. 9 a while the

    Al layer grown on the TiN film with a complete 111 pre-

    ferred orientation also has a pure 111 texture note the scale

    change by a factor of 102 in the inset of Fig. 9 b . Both Al

    layers are relaxed with a 111 interplanar spacing equal to thebulk value of 0.2338 nm.40 In addition, the 111 Al and TiN

    integrated peak intensities obtained from bilayer ii are two

    orders of magnitude higher than those of bilayer i at equal

    layer thicknesses. for Al layers grown on both series i

    and ii TiN are 13.5 and 0.82, respectively.

    The above results show that the stronger 111 orientation

    in the TiN film in bilayer-ii results in a corresponding en-

    hancement in the 111 texture of the Al overlayer. This occurs

    through texture inheritance as metal islands nucleate and, at

    least initially, grow with a local epitaxial relationship with

    underlying TiN grains. However, the final Al grain size is

    more than five times larger than that of TiN indicating the

    presence of recrystallization which is known to occur at tem-peratures Tr as low as Tr /Tm0.24 in high purity Al.

    41

    While this further reduces grain misorientation in both Al

    overlayers, the mosaicity of the layers grown on purely 111-

    oriented TiN is still more than an order of magnitude lower,

    as indicated by the measurements, than for Al grown on

    mixed 111/002-oriented TiN.

    Figures 10 a and 10 b are typical contour plots of the

    logarithm of the diffracted synchrotron x-ray intensity as a

    function of the diffraction angle 2 and temperature Ta dur-

    ing thermal ramping of underdense series-i TiN and dense

    111 series-ii TiN samples to 650 C at a rate of 3 C s1. The

    intensity is indicated by gray scale. White corresponds to an

    intensity of 1.9104 in Fig. 10 a and 9.2104 in Fig. 10 b

    while black is 102 counts s1. The angular range of the

    position sensitive detector was chosen based upon ex situ

    XRD results following isothermal anneals showing, in addi-

    tion to the strong TiN and Al 111 peaks, the emergence of

    the 112 tetragonal-structure Al3Ti peak also observed by

    TEM and XTEM at 39.132. 112 was the only XRD peak

    observed, indicating that the product phase is highly tex-

    tured. Grains of the intermetallic compound Al3Ti, whichhas the DO22 structure with lattice constants a0b 00.385 37 nm and c0.858 39 nm,42 are aligned with their

    112 plane perpendicular to the Al film growth direction.

    112 is the closest-packed Al3Ti plane and exhibits an in-

    plane misfit with Al 111 of only 1%.

    Figure 10 a shows that for type-i samples, the intensity

    of the 111 Al peak at 45.2 0.1797 nm 2decreases with

    increasing annealing temperature Ta and is completely lost at

    Ta620 C. This is well below the Al melting point

    660 C and indicates that the Al layer has been completely

    consumed. Al3Ti starts to form at 450 C and reaches its

    maximum intensity at the same temperature at which the Al

    intensity disappears. In contrast, Al3Ti formation in type-iisamples is suppressed up to 610 C and significant unre-

    acted Al still remains even at 650 C as shown in Fig. 10 b .

    We attribute the enhanced interfacial stability of series

    ii, compared to series i, Al/TiN samples to the densification

    of TiN grain boundaries with high-flux (JN2/JTi14), low-

    energy (EN220eV), N2

    ion irradiation during TiN depo-

    sition, the larger TiN grain size by a factor of two , and the

    flatter surface. It has been reported previously8,9 that TiN

    barrier failure is initiated at the Al/TiN interface by the for-

    mation of Al3Ti in the Al layer. In type-i samples, massive

    diffusion of Al into the open TiN inter- and intracolumnar

    voids is expected to occur rapidly at relatively low annealingtemperatures leading to an enormous increase in the actual

    area of the Al/TiN interface.

    IV. CONCLUSION

    We have demonstrated, for the first time, the low-

    temperature growth of fully dense polycrystalline TiN with

    complete 111 preferred orientation. This was achieved using

    a combination of highly oriented thin 0002 Ti underlayers to

    provide orientation through texture inheritance local epi-

    taxy and high-flux, low-energy, N2

    ion irradiation(JN

    2/JTi14, EN

    2 20 eV) to provide enhanced adatom

    diffusion leading to densification. The preferred orientation

    of Al overlayers grown on dense fully 111-oriented TiN was

    also greatly enhanced due to texture inheritance, thus reduc-

    ing the FWHM of the 111 -rocking curve from 13.5 for Al layers grown on TiN deposited by conven-

    tional reactive magnetron sputter deposition to 0.82.

    This corresponds to an enhancement in the average mosaic

    coherence length by more than a factor of 15. Finally, we

    show that the thermal stability of Al/TiN bilayers to interfa-

    cial breakdown is increased from 450 to 610 C through the

    use of fully dense TiN layers with complete 111 texture.

    FIG. 10. XRD diffracted intensity contour maps plotted as a function of

    temperature during thermal ramping of a series i and b series-ii Al/TiN

    bilayers from 100 to 650 C at 3 C s1.

    3640 J. Appl. Phys., Vol. 86, No. 7, 1 October 1999 Chun, Petrov, and Greene

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    ACKNOWLEDGMENTS

    The authors gratefully acknowledge the financial support

    of the NSF/DARPA VIP Program and the Department of

    Energy under Contract No. DEAC0276ER01198 during the

    course of this research. We also appreciate the use of the

    Brookhaven National Synchrotron Light Source beamline

    X-20C together with the expert technical assistance of Dr.

    C. Lavoie and Dr. C. Cabral, Jr. of the IBM T.J. Watson

    Research Center, and the facilities in the Center for Mi-

    croanalysis, which is partially supported by DOE, at the Uni-

    versity of Illinois.

    1 M. Kageyama, K. Hashimoto, and H. Onoda, in Proceedings of the 29th

    International Reliability Physics Symposium, 1991 unpublished , p. 97.2 S. Vaidya and A. K. Sinha, Thin Solid Films 75, 253 1981 .3 M. Tsukada and S. Ohfuji, J. Vac. Sci. Technol. B 11, 326 1983 .4 K. Hashimoto and H. Onoda, Appl. Phys. Lett. 10, 120 1989 .5 H. Onoda, M. Kageyama, and K. Hashimoto, J. Appl. Phys. 32, 4479

    1993 .6 H. Shibata, M. Murota, and K. Hashimoto, Jpn. J. Appl. Phys., Part 1 32,

    4479 1993 .7 Q. Z. Hong, S. P. Jeng, R. H. Havemann, H. L. Tsai, and H. Y. Liu, J.

    Appl. Phys. 78, 7419

    1995

    .8 J.-S. Chun, J. R. A. Carlsson, D. B. Bergstrom, I. Petrov, J. E. Greene, C.

    Lavoie, C. Cabral, Jr., and L. Hultman unpublished .9 L. Hultman, S. Benhenda, G. Radnoczi, J.-E. Sundgren, J. E. Greene, and

    I. Petrov, Thin Solid Films 215, 152 1992 .10 M. Wittmer, J. Appl. Phys. 53, 1007 1982 .11 H. Norstrom, T. Donchev, M. Ostling, and C. S. Petersson, Phys. Scr. 28,

    33 1983 .12 C. Y. Ting, J. Vac. Sci. Technol. 21, 14 1982 .13 N. Kumar, K. Pourrezaei, B. Lee, and E. C. Douglas, Thin Solid Films

    164, 417 1998 .14 H. P. Kattelus, J. L. Tandon, C. Sala, and M. A. Nicolet, J. Vac. Sci.

    Technol. A 4, 1850 1986 .15 R. Beyer, R. Sinclair, and M. E. Thomas, J. Vac. Sci. Technol. B 2, 781

    1984 .16 R. C. Elwanger and J. M. Towner, Thin Solid Films 161, 289 1988 .17 K.-H. Bather and H. Schreibe, Thin Solid Films 200, 93 1991 .18 A. Kohlhase, M. Mandle, and W. Pamler, J. Appl. Phys. 65, 2464 1989 .19 W. Sinke, G. P. A. Frijlink, and F. W. Saris, Appl. Phys. Lett. 47, 471

    1985 .

    20 J. E. Greene, J.-E. Sundgren, L. Hultman, I. Petrov, and D. B. Bergstrom,

    Appl. Phys. Lett. 67, 2928 1996 .21 L. Hultman, J.-E. Sundgren, J. E. Greene, D. B. Bergstrom, and I. Petrov,

    J. Appl. Phys. 78, 5395 1995 .22 I. Petrov, A. M. Myers, J. E. Greene, and J. Abelson, J. Vac. Sci. Technol.

    A 12, 2846 1994 .23 I. Petrov, L. Hultman, U. Helmersson, J.-E. Sundgren, and J. E. Greene,

    Thin Solid Films 169, 299 1989 .24 L. Hultman, J.-E. Sundgren, and J. E. Greene, J. Appl. Phys. 66, 536

    1989 .25 I. Petrov, F. Adibi, J. E. Greene, W. D. Sproul, and W.-D. Munz, J. Vac.

    Sci. Technol. A 10, 3283 1992 .26 J. A. Thornton, J. Vac. Sci. Technol. 15, 188 1978 .27 R. F. Stebbing, B. R. Turner, and A. C. H. Smith, J. Chem. Phys. 38, 2277

    1963 .28 B. Chapman, Glow Discharge Processes Wiley, New York, 1980 , p.

    108.29 J. A. Biersack and L. G. Haggmark, Nucl. Instrum. Methods 174, 257

    1980 .30 A. V. Phelps, J. Phys. Chem. Ref. Data 20, 557 1991 .31 R. L. Doolittle, Nucl. Instrum. Methods Phys. Res. B 15, 344 1985 .32 J.-E. Sundgren, B.-O. Johansson, A. Rockett, S. A. Barnett, and J. E.

    Greene, in Physics and Chemistry of Protective Coatings, edited by J. E.

    Greene, W. D. Sproul, and J. A. Thornton American Institute of Physics,

    New York, 1986 , Ser. 149, p. 95.33

    F. Adibi, I. Petrov, J. E. Greene, L. Hultman, and J.-E. Sundgren, J. Appl.Phys. 73, 8580 1993 .

    34 D. Gall, I. Petrov, L. D. Madsen, J.-E. Sundgren, and J. E. Greene, J. Vac.

    Sci. Technol. A 16, 2411 1998 .35 C. Y. Ting and M. Wittmer, Thin Solid Films 96, 327 1982 .36 R. W. Bower, Appl. Phys. Lett. 23, 99 1973 .37 J. E. Greene, in Handbook of Crystal Growth, Volume 1: Fundamentals,

    edited by D. T. J. Hurle Elsevier, Amsterdam, 1993 , p. 639.38Inorganic Index to Powder Diffraction File Joint Committee on Powder

    Diffraction Standards, Pennsylvania, 1996 .39

    IMAGE software V. 1.55, from the National Institute of Health, obtainable

    from public program site with access address zippy.nimh.nih.gov un-

    der the directory/pub/nih-image.40Inorganic Index to Powder Diffraction File Joint Committee on Powder

    Diffraction Standards, Pennsylvania, 1996 .41 E. C. W. Perryman, ASM Seminar, Creep and Recovery, 1957 American

    Society for Metals, Cleveland, Ohio, 1957 , p. 111.42Inorganic Index to Powder Diffraction File Joint Committee on Powder

    Diffraction Standards, Pennsylvania, 1996 .

    3641J. Appl. Phys., Vol. 86, No. 7, 1 October 1999 Chun, Petrov, and Greene