Relaxation mechanism of Ge islands/Si(001) at low temperature
F. K. LeGoues, J. Tersoff, M. C. Reuter, M. Hammar, and R. Tromp
IBM Research Division, Thomas J. Watson Research Center, Yorktown Heights, New York 10598
͑Received 31 March 1995; accepted for publication 14 August 1995͒
Strained layers generally relax by dislocation glide. Here, using UHV-TEM, we study growth of Ge
islands on Si͑001͒ at Շ350 °C. We find that, although conventional relaxation ͑i.e., via glide of 60°
dislocations͒ is suppressed, the islands grow relaxed from the outset, by direct incorporation of
sessile 90° dislocations into the edge of the growing island. Paradoxically, the low-temperature
islands are more fully relaxed than those grown at higher temperature. © 1995 American Institute
of Physics.
Enormous effort has been devoted to understanding the
growth and relaxation of strained epitaxial layers. The SiGe
system has received particular attention in recent years be-
cause of its technological importance. The maximum mis-
match between Si and SiGe alloys is 4% ͑for pure Ge͒, and
in this regime, it is generally agreed that relaxation always
occurs by nucleation and glide of dislocations. However, as
the growth temperature is lowered, glide becomes more slug-
gish, and one may wonder whether, and by which mecha-
nism, relaxation can then occur at all.
Here, we study the growth of Ge on Si͑100͒ at low tem-
perature in situ and in real time. We find that the Ge grows
from the outset as strain-relaxed islands. It does this by di-
rectly incorporating sessile 90° dislocations into the edge of
the growing island. Previously, direct formation of 90° dis-
locations in SiGe was thought so unlikely that, whenever
they were observed, they were attributed to the reaction of
two 60° dislocations.1–4 Paradoxically, islands grown at low
temperature are more fully relaxed than those grown at
higher temperatures, where relaxation should be much easier.
Our ultrahigh vacuum transmission electron microscope
͑UHV-TEM͒ and experimental procedures have been de-
scribed previously.5 A Si͑001͒ wafer is chemically thinned to
electron transparency, and then heated to above 1300 °C in-
side the UHV-TEM. Oxygen is leaked into the TEM to etch
the sample at 950 °C, giving thinner viewing areas. For Ge
deposition, a 10:1 helium/germane mixed is leaked into the
TEM column to a pressure of about 10Ϫ5 Torr. The sample
temperature is measured by pyrometry. The growth is ob-
served in real time, and recorded on video tape. All images
are obtained in weak-beam dark-field conditions using the
͗200͘ reflection.
cated islands is also quite intriguing, and plays an important
role in the relaxation. We speculate that where the corners of
diagonally adjoining huts meets, they can act as pre-existing
dislocations, similar to the ‘‘coreless’’ dislocations discussed
for other systems.7,8 A somewhat related relaxation mecha-
nism, the nucleation of ‘‘V-shaped defects,’’ where two huts
coalesce, has been discussed by Sakai and Tatsumi,9 al-
though in our in situ studies we have never observed such
defects.
Returning to the central question of how the island re-
laxes, we show in Fig. 1͑c͒ the same island as in 1͑b͒ after
further growth. Two additional dislocations are evident.
There are also dislocations in the orthogonal direction, but
they are not visible under our imaging conditions ͑cf. Fig. 2͒.
Figure 2 shows weak-beam dark field images of a much
larger island with an extensive network of dislocations. In
Fig. 2͑a͒, only dislocations perpendicular to ͓220͔ are visible
͑thin vertical lines͒. In Fig. 2͑b͒, only dislocations parallel to
͓220͔ appear as thin horizontal lines. The g–b analysis shows
that there are two perpendicular sets of dislocations, whose
¯
Burgers’ vectors are perpendicular to ͓220͔ and ͓220͔, re-
spectively. This is consistent with the dislocation being 90°
Lomer dislocations, bϭ(a/2) 110 . This g–b is not complete
͓
͔
enough to rule out other 90° dislocations. However, the
Lomer dislocation is the only likely possibility, since other
90° dislocations that exist in this system are partials of the
͓112͔ type, which would generate stacking faults. While 90°
dislocations have been seen before in SiGe,1 because they
are immobile and cannot glide to the interface they have
invariably been attributed to the reaction of two 60°
dislocations.1–4 However, we see in the real-time video that
these 90° dislocations are formed directly at the edge of the
island, and not by the reaction of two 60° dislocations. We
suspect this was also the case in previous studies where net-
works of 90° dislocations were seen.1 Direct formation of
90° dislocations has been previously suggested only in sys-
tems with extremely high misfit ͑Շ8%͒.10–12
Figure 1 shows the evolution of the microstructure dur-
ing growth of Ge on Si͑001͒ at a nominal sample tempera-
ture of 350 °C. Initially, Ge forms an array of ‘‘huts’’,6 ͓Fig.
1͑a͔͒. Unlike the larger coherent islands that form at high
temperature,5 we never see these huts form dislocations. In-
stead, once the entire surface is covered with huts, another
kind of island nucleates, Fig. 1͑b͒. This island is quite small,
no larger than a hut, yet it already contains a dislocation
͑arrow͒. Because it is partially relaxed, this island is a pref-
erential site for incorporation of Ge, and subsequent growth
takes place only at such relaxed islands.
The degree of relaxation at low temperature is also quite
surprising. The dislocation spacing is approximately 115 Å,
close enough to relieve about 90% of the strain. This spacing
is much smaller than the hut size, and so is unrelated to the
presence of huts. In contrast, at higher temperature,5 al-
though introduction of dislocations is much easier, the island
remained far more strained, with only 25% relaxation.
As the growth temperature decreases, dislocation glide
While our principal concern here is how the Ge islands
relax as they grow larger, the initial formation of the dislo-
Appl. Phys. Lett. 67 (16), 16 October 1995
0003-6951/95/67(16)/2317/3/$6.00
© 1995 American Institute of Physics
2317
132.174.255.116 On: Sun, 30 Nov 2014 13:12:42