The T-line    luminescence system is  created in   Si by  annealing at
400-600 
 C. Shifts and splitting of the spectral features with
 
 C and D isotope  substitution  identify the  presence of two  C
atoms and one H atom in the center. Uniaxial stress and magnetic field
measurements show that   the  T-center has monoclinic-I   symmetry and
possesses an acceptor (-/0) level at 0.2 eV below the conduction band.
Ab-initio  cluster calculations lead  to a structure in which an
interstitial   C-H defect  binds with  a  substitutional   C atom. The
calculated  vibrational  modes  are   in  good  agreement  with  those
observed.
	It is  well    established  now  that  hydrogen  is   a common
contaminant                          in                        silicon
[1, 2, 3, 4].   It can   interact
with  both shallow  and  deep   level   centers and  eliminate   their
electrical [1] and  optical     [1, 4]
activity.   However, hydrogen can have a  quite  different effect.  In
this  letter we report the   structure  and properties  of an  optical
center created in silicon    which is stabilized by  the   interaction
between hydrogen and  interstitial carbon.  This  center gives rise to
the T-line (0.9351 eV) luminescence  system which is created in either
float-zone (FZ) or Czochralski (CZ) grown  silicon by radiation damage
and   subsequent   thermal   treatment   in   the  temperature   range
400-600 
 C, or by thermal treatment alone in carbon-rich CZ Si
[2, 3, 4, 5, 6].    It can also
be created in  some [5, 6], but  not all [7],
FZ Si by thermal treatment without  radiation damage.  This center has
been long known to be carbon related, a conclusion originally based on
sample statistics [5], but subsequently confirmed by a shift
in  the    zero-phonon line    with   
 C   isotope   substitution
[6].  However,  recent investigations of silicon deliberately
doped  with hydrogen-deuterium  mixtures have shown   that hydrogen is
also         involved       in            this                  center
[2, 3, 4].  We  present the effects of
isotope substitution on  the local vibrational  mode features observed
in  the luminescence spectra,    the effects of  uniaxial  stress  and
magnetic field  perturbations on the zero  phonon line and temperature
dependence  measurements.   These show  that   the center contains two
inequivalent  carbon  atoms  and one  hydrogen  atom, has monoclinic-I
symmetry and creates an  electron trap at  0.2 eV below the conduction
band.  Within these constraints, we  use ab initio local density
functional cluster theory  to show that  the  structure consists of  a
 
 100 
  oriented pair  of  carbon  atoms which share   a
lattice site, together with  one hydrogen atom attached  to one of the
carbon atoms.  The  calculation   also allows us  to assign   the four
observed local vibrational modes and account for their isotope shifts.
 The material employed in the work reported here was mainly FZ silicon
with  [C]    
 2 
 10 
  cm 
 ;   one   sample had   a
 
 C/ 
 C  ratio  of     
 1.4.  All   the   material was
saturated with   
 1.5 
 10 
  cm 
  H, D, or  a H+D
mixture by  heating in flowing gas  for 30 minutes at 1300 
 C,
and  rapidly cooling in  silicone  oil [8].  The material was
then  irradiated with a  flux of  either 10 
  cm 
  neutrons,
with  a  Cd ratio of   25, or  2 
 10 
  cm 
  2 MeV
electrons,  followed by  annealing  for 30 minutes at  450 
 C.
The photoluminescence (PL) was  excited by a  514 nm Ar 
  laser and 
detected with a  Fourier transform   spectrometer fitted with a North
Coast cooled  Ge diode  detector.   Uniaxial stress measurements  were
made with stresses up to 160 MPa. Magnetic fields up to 5T were employed.
 Fig. 1 shows a PL spectrum of the T-line system obtained at 35 K from
a sample saturated with deuterium.  The line at 1.75 meV higher energy
than   the T-line is associated  with  a zero-phonon transition from a
higher excited state.   The  phonon-assisted  region at lower   energy
contains  a  broad  sideband of   perturbed lattice modes,  typical of
carbon-containing defects  [9], together with several local
mode  satellites L 
 -L 
    and  resonance modes   L 
  and L 
 .
Above  10 K,  all the  L mode  features are  doublets mirroring the two
zero-phonon   transitions,  showing  that   these   features  are  all
associated with the same defect.
 We first discuss  the isotopic  shifts of  local mode features  which
reveal the chemical  composition and atomic  structure of the  center.
In   
 C+ 
 C+H    and   
 C+H+D mixed     isotope
materials, the T-line splits into two components establishing that the
center  contains  carbon  and   hydrogen (Fig. 1).  Similar   isotopic
splitting can be  observed  for the zero-phonon transition  associated
with the higher energy excited state.  However, unlike the zero-phonon
line, the  L 
  local mode splits  into four  components in the mixed
carbon  isotope material (Fig. 2) which  unambiguously  shows that the
defect contains two inequivalent  carbon atoms, contrary to a previous
conclusion  [6].  The  splitting   of a  zero-phonon  line is
dependent on the nature  of the electron-phonon coupling [10]
and,    although this   effect    is extensively   used  for  chemical
characterization, it  does   not   unambiguously  reflect the   atomic
structure  of the center.   The modes   and  their isotope shifts  are
listed in  Table  1.   They  give no indication   that  more than  one
hydrogen atom is involved in this center.
  Next we discuss the results of external field perturbation measurements, 
which reveal the symmetry of the center and the origin of the luminescence 
transitions. Both the zero-phonon lines split into 2, 3, and 4 components 
under uniaxial stresses along  
 100 
 ,  
 111 
 , 
and  
 110 
  directions, respectively [7]. 
The  relative amplitudes of  the peaks  do  not depend on temperature,
which strongly suggests that  the splitting of  the line is due to the
lifting  of orientation degeneracy. The   number of components and the
absence of  thermalization suggest that the symmetry  of the center is
monoclinic-I [11]. This is not  in agreement with the results of
earlier study [6], where a smaller number of split components
was observed, probably due to the  lower spectral resolution employed.
Temperature-controlled  measurements  have shown that  with increasing
temperature in the range 20-60 K, the photoluminescence (PL) intensity
decays with an activation energy of 32 meV, which is much smaller than
the  total     binding     energy   of  the    electron-hole     pair,
 
 235 meV.  This is   consistent  with the T-line  luminescence
being related  to the recombination of an  exciton  bound to a neutral
center, where one particle is bound into a  deep level state and other
is weakly  bound in the Coulomb potential  produced by the  first. The
thermal dissociation of the bound exciton and PL  decay, in this case,
is associated with  an excitation of the  weakly bound particle to the
nearest band. A detailed analysis  of the uniaxial stress and magnetic
field   measurements has  shown  that the  shallow effective-mass-like
particle  in the  bound  exciton  is  a hole, contrary  to  a previous
suggestion [6], and  consequently the defect possesses a deep
acceptor  level (-/0)    at    0.2 eV  below  the    conduction   band
[7].  It  has  been found that  the  behavior of  the hole
under  external field perturbations, as well  as the strong anisotropy
of   the   g-tensor,   can   be   successfully   described  by   the
characteristics of the valence band maxima, in agreement with the hole
being bound by the Coulomb potential [7]. In addition, the
analysis of the magnetic data has shown that the defect in its neutral
ground state  has an uncoupled electron  with spin  
  and a
g-factor  close to 2.    Upon photo-excitation,  when an exciton  is
bound to  the defect and an additional  electron occupies the acceptor
level, the two electron are coupled in a singlet state with S =0, so
that the magnetic splitting of the  excited state is determined by the
weakly   bound  hole with  spin  
   and  strong anisotropic
g-factors while the  splitting of the  final state is determined  by
the electron. This fully  accounts for the  observed structure  of the
Zeeman splitting, which corresponds to transitions between states with
spin  
  and  explains the absence of thermalization between
the   two sub-levels  of  the final  ground  state  and the absence of
exchange coupling  between the  bound exciton  particles [6].
Note that the paramagnetic  nature of the center  in its neutral state
is consistent with the presence of one hydrogen atom in the defect.
  Having established the chemistry and symmetry  of the center, we now
describe the results of   ab initio cluster   calculations which
lead  us to a  unique model of the  defect.  Details of the method and
applications to  substitutional   carbon (C 
 ),  interstitial carbon
(C 
 ), and the di-carbon  defect  (C 
 -C 
 ), as well as  defects
containing      hydrogen      have     been           given previously
[12, 13, 14] and will not be repeated here.
A trigonal  88 atom  cluster  C 
 HSi 
 H 
  was used  in all
calculations  presented  here,  all   atoms  were  relaxed  until  the
equilibrium structure was determined.
The second derivatives of the energy  with respect to atomic positions
were calculated for the  C and H atoms, as  well  as their nearest  Si
neighbors.   Energy second derivatives  for  the remaining atoms  were
taken from the  Musgrave-Pople potential found  by a  previous ab
initio  calculation [15],  and  the dynamical matrix  of the
cluster, and hence its vibrational modes, were calculated.
  We first  note that the C-related L 
   mode at 1056 cm 
  lies
within 130 cm 
  of modes due to C 
  and more than 400 cm 
 
above  those of C 
   [16].   This suggests that the  T-center
contains C 
 .   We now argue that  the  observed C-isotope shifts of
the  L 
  mode suggest the presence  of a C-C  bond.  This follows as
the  reduced  mass of  an isolated  C-C unit implies  that its stretch
frequency would   shift downwards by   20,  20  and 41 cm 
   for
 
 C- 
 C,    
 C- 
 C,     and       
 C- 
 C
respectively.  These shifts roughly agree with  the observed values of
18,  27  and 45 cm 
   for  the H case,   and  16.5, 20.5  and 
38 cm 
  for  D.  The different  shifts  in the  two mixed  C-isotope
cases imply that the C atoms are inequivalent, and the distinct shifts
in the H and D cases suggest that H is bonded with one of the C atoms.
Thus we  look for models with   
  symmetry containing  C 
  and
C-C-H units.
Several models were examined [17] 
and the ground state structure was found to be one shown in Fig. 3 where 
a  
 100 
  oriented C-C pair share a substitutional site. 
The H atom is attached to one of the carbon atoms, denoted C 
 , and 
the second undercoordinated carbon atom is labeled C 
 .
The calculations show   that the C 
 -C 
 , C 
 -H,  C 
 -Si  and
C 
 -Si bond lengths are 1.46, 1.11, 1.91 (2) and 2.05 (2) Å , respectively.
The calculated vibrational modes and their isotope shifts 
are given in Table 1.   Now, PL only detects
modes of A-symmetry and we concentrate on those at 2913, 1180, 1098,
744, 558   and   542 cm 
 .   The   first  four   modes correspond
predominantly to C 
 -H stretch, C 
 -H wag, C 
 -C 
  stretch and
C 
 -Si stretch  respectively.  The  last  two modes at 558   and 
542 cm 
  are close to the  Raman frequency, and involve predominantly
the  motion of  C 
   and C 
 , respectively,   as  well as  their Si
neighbors. There is close agreement between the modes L 
  to L 
  
observed by PL and the calculated vibrational modes which enables them 
to be identified (Table 1).  
The two highest energy  modes at 2913 and 1180 cm 
  are undetected 
by PL. However, the intensities of the phonon-assisted transitions are
critically  dependent   on   the exciton-phonon   coupling,   and  not
necessarily all local modes can be detected by PL.  In addition, there
is an experimental problem in observing  the highest energy local mode
since the Ge detector is insensitive in  the region where the position
of the corresponding luminescence line is expected.  
The  C 
 -C 
   stretch mode lies  close to
L 
  and has carbon isotope shifts 19, 21, 41 cm 
  in the H case
and  17, 24, 42 cm 
   in  the D case.   These  shifts are in good
agreement with the experimental values  18, 27, 45 cm 
  and 16.5,
20.5,  38 cm 
 , respectively, observed   for  L 
 .  We therefore
identify the  L 
    mode  with C 
 -C 
  stretch.     The C 
 -Si
stretch mode at 744 cm 
  involves the movement  of H as well, but
has little amplitude on C 
 .   As a consequence, this mode  displays
large isotope shifts with both  
 C and D --  23 cm 
  and 
30 cm 
  respectively -- but  essentially no additional modes appear
in the mixed C-isotopic cases.  These results allow us to identify the
mode   with L 
   at  796 cm 
 , which decreases   by  25 and 
37 cm 
  for  
 C and D, respectively, and  involves the motion of
only one of the C atoms.  Finally, the two  lower A modes at 558 and
542 cm 
  (H) are in good agreement with L 
  and L 
 , at 567.5
and  531.5 cm 
 , respectively.    These modes are more delocalized
and have only small shifts with D and  the various combinations of the
C-isotopes.
The neutral defect has a deep mid-gap donor   level  occupied by one electron,
although 
the theory is unable to  locate it exactly. This donor level has not
been reported so far. 
The acceptor level at  
  eV would then  be explained by a 
large Hubbard-U term of   at least  0.4 eV.
The structure and  electronic properties of the center are similar to 
the stable form of the  P-C 
  defect which possesses  acceptor and donor levels at
 
  eV and  
  eV respectively [18].
The wavefunction for the singly occupied level   is 
localized on a  non-bonding p-orbital on the  C 
 
atom and has spin  
  in agreement with the
Zeeman measurements described above.   Only small isotropic  hyperfine
couplings with   C 
  and  H    are, however,  to   be  expected. The
saturation of  the dangling bond related  to C 
  by  a second H atom
would eliminate the optical activity of the center, which might  account 
for the
observed loss of the  PL intensity when the  H concentration is  large
[3, 4].
  The calculations   presented here  favor the   
 100 
 
oriented  C 
 -C 
 -H  split-interstitial  as a   candidate  for the
T-center, although additional support would arise from observations of
the C-H stretch and wag modes at 2914 cm 
  and 1180 cm 
 , as
well as the   mode of B-symmetry.  The  presence  of a  C-C  bond is
surprising  as  the C 
 -C 
  defect,  which is  stable to about 300
 
 C, only contains  C-Si bonds  [19].  We suggest  that
the T-center  is formed  when C 
  traps  H  in the BC  sited defect.
This in turn diffuses to C 
  where conversion  to the T-center takes
place.  A calculation shows the trapping of  C 
 -H by C 
  leads to
an energy reduction of  1.4 eV [17].  This formation mechanism
is more likely than the  trapping of H  by the di-carbon defect as the
latter is not stable at 400-600  
 C.
The identification  of this defect  is important  for several reasons.
It is commonly produced in FZ and CZ silicon samples by irradiation
and/or thermal treatment, showing that H is present as an unintentional
impurity    in   silicon  [2, 3].     The defect
structure   and the mechanisms  of  formation provide further evidence
that thermal treatment of CZ Si leads to a generation of Si 
 , which
can be subsequently trapped by C 
  to produce mobile C 
 .  
The stability of the T-center over  an important temperature range 
(400-600 
 C)  where thermal donors are generated may enable 
it to be used to monitor Si 
  production. The results reported in this 
paper show that the presence of hydrogen can lead to the formation of 
unusually stable electrically and optically active defects.
In conclusion, a combination of high resolution photoluminescence experiments, Zeeman and uniaxial stress studies, and ab initio theory have successfully elucidated the structure and properties of an interstitial carbon-hydrogen defect in silicon.
This work was carried out with funding from the Engineering and Physical Sciences Research Council. R.J and P. L. thank the HPCI for computer time on the T3D at Edinburgh. S. Öberg thanks the Swedish National Scientific Research Council for financial support as well as the PDC for computer time on the SP2 at Stockholm.