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Silicon research of the
Webergroup: Transition-Metal Physics
Transition metals, especially 3d transition metals such as
Fe, Ni and Cu are ubiquitous in IC production lines. It is well
known that 3d transition metals dissolved in silicon introduce
deep energy levels in the band gap and act as generation-recombination
centers, which reduce minority carrier lifetime, degrade the
microchip devices, and give severe reliability problems. The
knowledge of fundamental properties such as diffusivity and
solubility is critical to design the gettering treatment. Recently,
our group is working on the following projects:
1. Intrinsic diffusion coefficient
of interstitial copper in silicon
Probably the most surprising recent discovery associated with
the physics of Cu in Si was the new determination of its diffusion
coefficient [1] by our group. The diffusion coefficient of Cu
in Si was thought to be well established since the work of Hall
and Racette [2] published in 1964. Their expression for Cu diffusivity,
D = 4.7×103×exp(–0.43 eV/kBT)
cm2 s-1, has been widely used for modeling
diffusion of Cu in Si and was included in all major textbooks
(e.g., Ref. [3]). Starting from approximately 1990, a discussion
started in the literature [4-6] that Hall and Racette, who used
p+ -Si ([B] = 5×1020cm-3)
for their diffusion studies, did not take into account the effect
of pairing of positively charged interstitial Cu, Cu, with negatively
charged substitutional boron, B. The consequence of this pairing
is that only a fraction of the total Cu concentration is mobile
at any given moment, while the rest is temporarily trapped.
Following the diffusion theory of Frank and Turbull [7] and
Reiss et al.,[8] it was suggested that Hall and Racette measured
the effective, i.e., decreased by the effect of trapping by
shallow acceptors, diffusion coefficient of Cu in p+-Si,
and that their data should be revised to extract the intrinsic
diffusion coefficients, i.e., the diffusion coefficient in Si
without trapping sites[4-6]. Although in most real-life situations
for p-type Si an effective diffusion coefficient is to be used,
the intrinsic diffusion coefficient is important to know in
order to calculate the effective Cu diffusivity for any p-type
doping level of the substrate. Therefore, the practical significance
of the intrinsic diffusion coefficient is paramount.
Several attempts to calculate the intrinsic
Cu diffusivity by using various assumptions for the interaction
potential between Cu and B from either the data of Hall and
Racette [4] or from data points obtained by the transient ion
drift (TID) technique at room temperature [5][6] were reported.
However, none of these results were reliable since there was
no evidence that the simple electrostatic models used in Ref.
[4-6] to account for the interaction potential between Cu and
B were sufficiently good approximations of the true potential.
Indeed, theoretical calculations indicated that the bonding
in Cu-B pairs has a significant covalent component [9], which
cannot be quantitatively described by a simple model. In 1998,
our group designed an experiment which allowed us to determine
the intrinsic diffusion coefficient of Cu directly from the
experimental data. This was achieved by minimizing Cu-B interactions
to a negligible level by (i) using Si samples with low boron
doping level (1.5×1014 cm -3) and
(ii) performing transient ion drift measurements at elevated
temperatures (up to 110°C). Further details of the experiment
can be found in Ref. [1]. In particular, we found that the intrinsic
diffusion coefficient of interstitial Cu in Si is given by Ref.
[1]

whereas the effective diffusion coefficient
(i.e., the diffusion coefficient which takes into account trapping
of Cu by acceptors) is given by a system of equations, which
for the moderately boron-doped (Na=1017cm-3)
Si can be reduced to the following explicit formula [1]

In this equation, temperature, T, is measured
in kelvin and the boron doping level, Na, in cm-3.
Note that in the case of heavily doped samples (Na>1017
cm-3) or in the case of Al or Ga-doped wafers one
should solve a system of equations given in Ref. [1] rather
than use Eq. 2
The intrinsic diffusion coefficient was defined
in Ref. [1] as the diffusion coefficient of Cu in intrinsic
float zone with low levels of oxygen and carbon. The impact
of oxygen and carbon on Cu diffusivity is unclear, but there
are indications that it is very small [6]. Since there is no
experimental data on the pairing of Cu with positively charged
shallow donors such as phosphorus, we think that the intrinsic
diffusion coefficient may also be applied to moderately doped
n-type Si at high temperatures. At low temperatures, the diffusivity
of Cu in n-type Si may be impaired by the high likelihood of
the formation of clusters and precipitates of Cu in n-Si (see
the section on Defect reactions of Cu). The diffusivity of Cu
in n+-Si requires a separate investigation since
it was suggested [2][10] that a significant fraction of Cu becomes
substitutional in n+ -Si, thus changing its diffusion
mechanism and making feasible a pairing of negatively charged
substitutional Cu with shallow donors [11].
The fact that the intrinsic diffusion coefficient
of Cu in Si at room temperature, 2.8×10-7 cm2/s
(Eq. 1), is three orders of magnitude greater than extrapolated
from the data of Hall and Racette [2], implies that Cu diffusivity
is sufficiently high to enable Cu to diffuse significant distances
in a wafer even at room temperature. For instance, Cu can diffuse
at room temperature through a standard 4 in. p-type boron-doped
10 cm Si wafer in about 15 h.
It is important to point out that despite a
difference of three orders of magnitude between our data for
the intrinsic diffusion coefficient of Cu at room temperature
and the expression suggested for Cu diffusivity by Hall and
Racette, our results do not contradict the old Cu diffusivity
data. This is illustrated in Fig. 1, which summarizes all published
data on the Cu diffusivity in boron-doped Si with different
boron concentrations (symbols), the intrinsic Cu diffusivity
(curve 1), and the calculated diffusivities for different doping
levels (curves 2-5), including that used by Hall and Racette
(curve 5). Besides four data points of Hall and Racette [2],
a data point obtained by Struthers for intrinsic Si22
is also shown. The data point of Struthers lies indeed on the
intrinsic diffusivity line (curve 1). It is seen from Fig. 1
that the effective diffusion coefficient of Cu calculated for
the boron doping level of 5×1020 cm-3
is in perfect agreement with the data of Hall and Racette [2],
see curve 5 in Fig. 1. This indicates that their data were correct,
but unfortunately applicable only to p+-Si with a
doping level of 5×1020 cm-3, and
only in the temperature range where their data points were taken.

Fig.
1. Effective diffusion coefficient of Cu in Si calculated for
different boron doping levels (lines) and experimental data
obtained by Istratov et al.[1] (circles) Na = 1.5×1014
cm-3 and (diamonds) Na = 2×1015
cm-3, by Hall and Racette; [2] (triangles) Na = 5×1020cm-3,
by Struthers [12] (gray triangle, intrinsic silicon). Curve
1, intrinsic silicon (corresponds to the intrinsic diffusivity).
Curve 2, Na = 1.5×1014 cm-3. Curve
3, Na = 2×1015 cm-3. Curve 4, Na
= 1×1017 cm-3. Curve 5, Na = 5×1020
cm-3.
The diffusion barrier of 0.18 eV is by far
lower than that of any other impurity in Si. This low value
is due primarily to the small ionic radius of Cu in Si and the
weakness of covalent interactions of Cu with the crystal lattice.
It is known that the diffusion barrier of any impurity consists
of two major components, determined by the elastic and electronic
interactions with the lattice atoms [13]. Utzig [14] estimated
the elastic component of the diffusion coefficient of 3d metals
in Si and obtained results surprisingly close to the experimental
data for the majority of transition metals, with the exception
of the ionized copper Cu, whose ionic radius was so small that
Utzig's model predicted a zero diffusion barrier for it. Woon
et al. [15] predicted the electronic component of the Cu diffusion
coefficient at 0.24 eV, in good agreement with our experimental
data.
[1] A. A. Istratov, C. Flink, H. Hieslmair, E.
R. Weber, and T. Heiser, Phys. Rev. Lett., 81, 1243 (1998)
[2] R. N. Hall and J. H. Racette, J. Appl. Phys., 35, 379 (1964
[3] K. Graff, Metal Impurities in Silicon-Device Fabrication,
Springer, Berlin (1995
[4] R. Keller, M. Deicher, W. Pfeiffer, H. Skudlik, D. Steiner,
and T. Wichert, Phys. Rev. Lett., 65, 2023 (1990
[5] A. Mesli and T. Heiser, Phys. Rev. B, 45, 11632 (1992)
[6] A. Mesli, T. Heiser, and E. Mulheim, Mater. Sci. Eng., B,
25, 141 (1994)
[7] F. C. Frank and D. Turnbull, Phys. Rev., 104, 617 (1956)
[8] H. Reiss, C. S. Fuller, and F. J. Morin, Bell Syst. Tech.
J., 35, 535 (1956)
[9] S. K. Estreicher, Phys. Rev. B, 60, 5375 (1999); S. K. Estreicher,
Phys. Rev. B, 41, 5447 (1990)
[10] U. Wahl, A. Vantomme, G. Langouche et al, Appl.
Phys. Lett., 77, 2142 (2000)
[11] R. L. Meek and T. E. Seidel, J. Phys. Chem. Solids, 36, 731
(1975
[12] J. D. Struthers, J. Appl. Phys., 27, 1560 (1956
[13] O. L. Anderson and D. A. Stuart, J. Am. Ceram. Soc., 37,
573 (1954)
[14] J. Utzig, J. Appl. Phys., 65, 3868 (1989)
[15] D. E. Woon, D. S. Marynick, and S. K. Estreicher, Phys. Rev.
B, 45, 13383 (1992)
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