WF –SiH mixture, the impact of H is almost negligible
6
4
2
and the main solid products will always be TiF and W. All
3
these seem to be supported by the results of Figs. 1 and 2.
Apparently, more oxidation takes place on the TiN surface of
the low-T TiN, because this TiN has substantially more grain
boundaries per unit surface area as compared to the high-T
TiN.13 The grains of the low-T TiN extend right through the
whole TiN layer down to the underlying Ti layer. If sufficient
F reaches the Ti underlayer, delamination can occur due to
the interaction of F with Ti. The nonstoichiometric TiN layer
also seems to promote the interaction between WF and TiN.
6
Therefore, to reduce the impurity level at the W–TiN inter-
face, a stoichiometric TiN layer is preferred and a large
amount of H should be introduced to the WF –SiH gas
2
6
4
mixture during the deposition of W nucleation layers. The
slight W penetration into the underlying TiN is ascribed to
FIG. 3. RBS spectra for the W nucleation layers of 40 nm thickness depict-
ing a small difference in the low-energy edge of the W peaks among the
three wafers presented.
the inhomogeneous interaction between WF and the par-
6
tially oxidized TiN surface. The latter is formed because of
nonuniform surface oxidation of TiN in air at room tempera-
ture.
concentration decays rapidly from the peak values of 1.0–2.5
at. % at the W–TiN interface to about 0.1 at. % at the W
surface ͑depthϭ0 nm͒ only about 40 nm apart. Presumably,
most of the O impurities are also found in the similar depth
range.
Tailing of F into the TiN layer is closely associated with
the W penetration into the underlying TiN. The Rutherford
backscattering spectrometry ͑RBS͒ results of Fig. 3 depict
that the degree of extension of the low-energy edge of the W
peaks towards lower energies follows the same trend as the
degree of F tailing shown in Fig. 2. Since both the W surface
and the W–TiN interface for the W nucleation layer depos-
ited on the low-T TiN are smoother than those of the W
nucleation layer deposited on the high-T TiN,13 the W pen-
etration into the underlying TiN is concluded to be the main
cause for the extension of the low-energy edge of the W
peaks observed in Fig. 3. Thus, depositing W on the high-T
The W films are all under tensile stress, and the ampli-
tude of the stress is not only strongly influenced by the type
of adhesion TiN/Ti bilayers,13 but also affected by H addi-
2
tion to the reactants during W nucleation layer deposition
͑see Table I͒. According to x-ray diffraction ͑XRD͒ analysis,
the W films deposited are all preferentially oriented to the W
͗110͘, and the strong impact of the underlying TiN on the
film texture of W has been reported elsewhere.13 The inte-
grated intensities of the W-͑110͒ peak given in Table I are
normalized values. The W films are less textured for the W
deposited with H addition to the reactants during the depo-
2
sition of W nucleation layers. Thus, the difference in stress is
attributed to the difference in the texture of the W films and
possibly to the interfacial impurities as well.
The authors wish to thank J. Cardenas for SIMS and N.
Lundberg for RBS. This work was financially supported by
the Swedish Board for Technical Development ͑Nutek͒ and
by the Flemish Institute for the Advancement of Scientific-
Technological Research in Industry ͑IWT͒.
TiN or adding H to the reactants during W deposition leads
2
to reduced W penetration. It should, however, be noted that
the depth of W extending into the underlying TiN is much
shallower than the depth of F tailing into the same TiN. This
is interpreted as a consequence of the much more rapid F
penetration along the grain boundaries of TiN, as compared
to W into TiN.
1
M. L. Green and R. A. Levy, J. Electrochem. Soc. 132, 1243 ͑1985͒.
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1992, edited by T. S. Cale and F. S. Pintchovski ͑Materials Research
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E. K. Broadbent and C. L. Ramiller, J. Electrochem. Soc. 131, 1427
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The interfacial O found at the W–TiN interface origi-
nates from native oxide on the TiN surface formed before W
͑
1984͒.
4
5
6
7
1
3
K. Y. Tsao and H. H. Busta, J. Electrochem. Soc. 131, 2702 ͑1984͒.
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deposition. Fluorine atoms pile up at the same interface
because of the presence of O there. Large amounts of F
atoms are incorporated at the W–TiN interface also due to
the formation of nonvolatile TiF , a product of the chemical
3
8
9
0
interaction between WF and TiN under the deposition con-
6
ditions used. Thermodynamic calculations predict that when
a TiO surface is exposed to the WF –SiH mixture with a
141, 2192 ͑1994͒.
2
6
4
1
¨
H. Norstr o¨ m, S. Nygren, P. Wiklund, M. Ostling, R. Buchta, and C. S.
SiH -to-WF ratio of about 0.5 and without H addition, the
4
6
2
Petersson, Vacuum 35, 547 ͑1985͒.
S. Sivaram, M. L. A. Dass, C. S. Wei, B. Tracy, and R. Shukla, J. Vac. Sci.
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main solid products will be WO , TiF , and W. H addition to
11
2
3
2
the same WF –SiH mixture reduces the amount of solid
6
4
12
oxide phase͑s͒ by enhancing the formation of gaseous H O.
2
The formation of TiF will also be considerably reduced by
3
13
14
S.-L. Zhang, R. Palmans, S. Petersson, and K. Maex ͑unpublished͒.
H as a result of increased amount of gaseous phase HF. On
2
¨
H. J. Whitlow, Th. Ericsson, M. Ostling, C. S. Petersson, J. Keinonen, and
the other hand, when a TiN surface is exposed to the same
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3000
Appl. Phys. Lett., Vol. 67, No. 20, 13 November 1995
Zhang et al.
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