Article

Carbon-related centres in irradiated SiGe alloys

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Abstract

We report measurements on the Ci–Oi ‘C-centre’ in Czochralski-grown Si1−xGex (x⩽0.06), using the complementary techniques of photoluminescence (PL) and deep-level transient spectroscopy (DLTS). Both techniques show that the donor level of the C-centre in SiGe alloys shifts towards the valence band with increasing x. Unexpectedly, the shift rate of d(ΔHn)/dx=+550meV detected using DLTS is found to be 1.6 times greater than that from PL measurements. Alloy broadening of the PL line and the DLTS signal are similar, and suggest that the C-centre is preferentially found in a Ge-rich environment.

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... This alloy usually becomes polycrystalline for the other range of Ge content [6,7]. The radiation damage of the Si 1−x Ge x devices related with introduction of radiation defects [3,[8][9][10][11] can be healed by the atomic reconfiguration of the crystal structure during material anneal [12][13][14]. The particle detector degradation [15][16][17][18] usually appears through decrease of carrier recombination lifetime. ...
Article
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The particle detector degradation mainly appears through decrease of carrier recombination lifetime and manifestation of carrier trapping effects related to introduction of carrier capture and emission centers. In this work, the carrier trap spectroscopy in Si1−xGex structures, containing either 1 or 5% of Ge, has been performed by combining the microwave probed photoconductivity, pulsed barrier capacitance transients and spectra of steady-state photo-ionization. These characteristics were examined in pristine, 5.5 MeV electron and 1.6 MeV proton irradiated Si and SiGe diodes with n+p structure.
... The influence of the Ge content on the properties of a few point defects known for pure Si has been understood [33][34][35][36][37][38][39]. An example is given in Fig. 2. The conclusions drawn from these studies with respect to the defect level position in the gap are as follows [40,41]: (i) The observed level displacement towards the valence band with increasing Ge is characteristic of (almost) all defect levels. ...
Article
The article is dedicated to the review and analysis of the effects and processes occurring in Si-Ge quantum size semiconductor structures upon particle irradiation including ion implantation. Comparisons to bulk materials are drawn. The reasons of the enhanced radiation hardness of superlattices and quantum dots are elucidated. Some technological applications of the radiation treatment are reviewed.
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In this work, electrically active defects of pristine and 5.5 MeV electron irradiated p-type silicon–germanium (Si1−xGex)-based diodes were examined by combining regular capacitance deep-level transient spectroscopy (C-DLTS) and Laplace DLTS (L-DLTS) techniques. The p-type SiGe alloys with slightly different Ge contents were examined. It was deduced from C-DLTS and L-DLTS spectra that the carbon/oxygen-associated complexes prevailed in the pristine Si0.949Ge0.051 alloys. Irradiation with 5.5 MeV electrons led to a considerable change in the DLT spectrum containing up to seven spectral peaks due to the introduction of radiation defects. These defects were identified using activation energy values reported in the literature. The double interstitial and oxygen complexes and the vacancy, di-vacancy and tri-vacancy ascribed traps were revealed in the irradiated samples. The interstitial carbon and the metastable as well as stable forms of carbon–oxygen (CiOi* and CiOi) complexes were also identified for the electron-irradiated SiGe alloys. It was found that the unstable form of the carbon–oxygen complex became a stable complex in the irradiated and the subsequently annealed (at 125 °C) SiGe samples. The activation energy shifts in the radiation-induced deep traps to lower values were defined when increasing Ge content in the SiGe alloy.
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The equilibrium geometries, phonon spectra, electronic structures and optical properties of the CiOi defect in bulk Si and Si1−xGex systems are calculated using the ab initio plane wave density-functional method. We find that in a Ge-doped Si crystal it is more energetically favourable for the defect to stabilize in a configuration with no Ge atoms in the first sphere. Our calculations show that the vibrational properties of the defect in the Si1−xGex alloy are similar to those in the pure Si bulk crystal and only one local vibrational mode is sensitive to the presence of the Ge substitutions. The effect of C, O, Si and Ge isotopes on the phonon spectra are also investigated and found to be in good agreement with available experimental data. It also follows from our calculations of the singlet–triplet splitting and a position of the gap state of the defect with respect to the top of the valence band that the optical energies of the CiOi defect are expected to increase due to Ge doping, which is in agreement with available experimental data.
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The microscopic behavior of iron in relaxed Si1-xGex alloy is addressed in the present work where various new aspects are highlighted. In p-type materials two types of defects involving iron may coexist under equilibrium; the isolated form, Fei, and the iron-acceptor pair, Fei-As. The latter complex is favored over the former because it is thermodynamically more stable. In each case the iron atom stabilizes at the interstitial tetrahedral site. When boron is the acceptor impurity, both the isolated and the paired forms introduce donor-like levels, distant from each other by 0.28 eV. In the relaxed Si1-xGex bulk alloy, these levels are shown to remain separated by the same amount. However, they shift toward the valence band much faster than the shrinkage of the band gap when the Ge content is increased. The consequence is that the pair-related donor level merges with the valence band at a fairly low alloy composition (x>=7%) while the iron donor level is predicted to disappear from the gap for x>=25%. We also show that neither the entropy nor the enthalpy of migration of free iron, whose experimental determination requires one to take into account the above-mentioned shift, are affected by alloying. Therefore, the fast diffusing character, attributed to iron in silicon, still holds in the alloy. The origin of spectral broadening, related to the chemical disorder, is discussed. Finally, the major technological implication emerging from our new findings is addressed. In particular, we show that both the gettering by segregation, routinely used in silicon, and the field-induced outdiffusion, established in n-type silicon ten years ago, are totally inefficient in the Si1-xGex alloy.
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Room-temperature irradiation of silicon with 2 MeV electrons can create many defects that give rise to optical absorption lines. The authors describe a simple procedure for calculating the strengths of the more important absorption features and the concentrations of the corresponding defect centres as functions of the radiation dose and of the carbon and oxygen concentrations in the silicon. The following absorption features and centres are considered: the 969 meV line (two-carbon-atom centre), the 865 cm-1 line (C+O centre), the 1020 cm-1 line (C+O+self-interstitial), the 835 cm-1 line (vacancy+O'A centre'), the 1.7 mu m band (di-vacancy) and the 488 meV line (C+O+vacancy centre).
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Low-dose proton- and helium-implanted silicon was studied by deep-level transient spectroscopy. By comparing the spectra as well as the defect level concentration profiles, five electron traps and one hole trap (after proton implantation at room temperature) and one dominant electron trap (after proton implantation at 80K) were identified to be hydrogen-related. Two of the hydrogen-related defect levels produced at room temperature represent different charge states of the same defect with a structure probably containing two hydrogen atoms. The electron trap produced by proton implantation at 80K is a donor level located at about Ec-0.2 eV. The defect is tentatively identified as a vacancy-hydrogen complex or a hydrogen atom in a single interstitial site and anneals out before reaching room temperature.
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The paper is concerned with carbon interstitial (Ci), Ev+0.28 eV, and a carbon-related centre, Ev+0.37 eV, growing almost simultaneously with the removal of the Ci atoms in electron-irradiated p-type Cz-grown Si. An observed inverse annealing stage of the former defect at approximately 275 K most likely indicates the existence of internal processes taking place below room temperature which liberate Ci as a final product. These processes are in accord with other experimental findings showing that the concentration of the Ev+0.37 eV defect is larger than that of the Ci. The identity of the two centres found to contribute to the creation of the Ev+0.37 eV defect state is discussed.
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Highly excited states of the 0.79 eV luminescent defect observed in photoluminescence excitation (PLE) measurements are interpreted as effective-mass (EMT) states of a pseudo-donor with Ei=38.3 meV. The interpretation implies that the 1s ground state of the donor electron is fivefold split in the C1h symmetric strain field of the defect. Modelling of the internal deformation around the defect by a compressive uniaxial field of 80 MPa along (001) allows the authors to explain the ground state splitting quantitatively and gives rise to a re-interpretation of published uniaxial stress data. Transient decay data suggest that the lowest excited defect state is a split singlet-triplet bound exciton, the 0.79 eV line being emitted by the higher-energy singlet.
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The activation energy of phosphorus substituted into Si1−xGex alloys (0 ≦ x ≦ 0.27) is investigated by IR absorption. A weak shift of the activation energy with germanium content is found: E(A1) = (45.5 − 26x) meV. This can be explained by multivalley effective mass theory with a phenomenological central cell potential which does not depend on alloy composition within the investigated range. The experiments show that P atoms are distributed at random in the alloy and that their positions are uncorrelated to those of the Ge atoms. Die Aktivierungsenergie des Phosphorgrundzustandes in Si1−xGex-Mischkristallen im Bereich 0 ≦ x ≦ 0,27 wird mit IR-Absorptionsmessungen untersucht. Mit zunehmendem Germaniumgehalt verringert sich diese Energie um 26x meV. Dies kann mit der Effektiv-Massen-Näherung erklärt werden, wenn ein im untersuchten Bereich von der Zusammensetzung des Kristalls unabhängiges „Zentral-Zellen-Potential” angenommen wird. P- und Ge-Atome sind statistisch im Mischkristall eingebaut.
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The photoluminescence spectra of crystalline silicon samples are measured for temperatures below 1000 K. The optical transitions are analyzed in terms of excitonic and band‐to‐band transitions. From the modeling of the line shape we are able to determine the fundamental indirect band gap for temperatures up to 750 K. The temperature dependence follows the Varshni equation with E g (0)=1.1692 eV, α=(4.9±0.2)×10<sup>-4</sup> eV/K and β=(655±40) K. © 1996 American Institute of Physics.
Article
Over one hundred independent photoluminescence transitions are now known in crystalline silicon. This paper begins by outlining those properties of silicon which are relevant to understanding the photoluminescence. The advantages of, and problems with, the different optical techniques are outlined. Topics discussed in detail include the quantitative understanding of the optical effects of radiation damage, and the vibroni c bandshapes of the photoluminescence, including local and resonant modes, the vibronic coupling of nearly degenerate excited states and isotope effects. The link is described between the excited states of some of the centres and the band states of the silicon host lattice. Relationships within groups of similar optical centres, and the widths of the zero-phonon transitions are also discussed. Tables include a list of published photoluminescence transitions indicating their key properties.
Article
Isoelectronic substitutional carbon atoms, present as an impurity in crystalline silicon, are shown to split the no-phonon luminescence line produced by the decay of excitons bound to phosphorus donors. The centroid of the doublet moves to lower photon energy in proportion to the carbon concentration. The splitting and shift can be explained quantitatively as a perturbation of the transition by the strain produced by the carbon. © 1996 The American Physical Society.
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