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   <ui>1556-276X-5-991</ui>
   <ji>1556-276X</ji>
   <fm>
      <dochead>Nano Express</dochead>
      <bibl>
         <title>
            <p>Cooperative Effects in the Photoluminescence of (In,Ga)As/GaAs Quantum Dot Chain Structures</p>
         </title>
         <aug>
            <au ca="yes" id="A1"><snm>Mazur</snm><mi>I</mi><fnm>Yu</fnm><insr iid="I1"/><email>ymazur@uark.edu</email></au>
            <au id="A2"><snm>Dorogan</snm><fnm>VG</fnm><insr iid="I1"/></au>
            <au id="A3"><snm>Marega</snm><fnm>E</fnm><suf>Jr</suf><insr iid="I1"/></au>
            <au id="A4"><snm>Cesar</snm><fnm>DF</fnm><insr iid="I2"/></au>
            <au id="A5"><snm>Lopez-Richard</snm><fnm>V</fnm><insr iid="I2"/></au>
            <au id="A6"><snm>Marques</snm><fnm>GE</fnm><insr iid="I2"/></au>
            <au id="A7"><snm>Zhuchenko</snm><mnm>Ya.</mnm><fnm>Z</fnm><insr iid="I3"/></au>
            <au id="A8"><snm>Tarasov</snm><fnm>GG</fnm><insr iid="I3"/></au>
            <au id="A9"><snm>Salamo</snm><fnm>GJ</fnm><insr iid="I1"/></au>
         </aug>
         <insg>
            <ins id="I1"><p>Department of Physics, University of Arkansas, 226 Physics Building, Fayetteville, AR, 72701, USA</p></ins>
            <ins id="I2"><p>Departamento de Fisica, Universidade Federal de Sao Carlos, 13565-905, Sao Carlos, Sao Paulo, Brazil</p></ins>
            <ins id="I3"><p>Institute of Semiconductor Physics, National Academy of Sciences of Ukraine, 45 Nauki prospect, Kiev, 03028, Ukraine</p></ins>
         </insg>
         <source>Nanoscale Research Letters</source>
         <publisher>Springer-Verlag, New York</publisher>
         <issn>1556-276X</issn>
         <pubdate>2010</pubdate>
         <volume>5</volume>
         <issue>6</issue>
         <fpage>991</fpage>
         <lpage>1001</lpage>
         <xrefbib><pubidlist><pubid idtype="pmpid">20672035</pubid><pubid idtype="doi">10.1007/s11671-010-9590-5</pubid></pubidlist></xrefbib>
      </bibl>
      <history><rec><date><day>20</day><month>1</month><year>2010</year></date></rec><acc><date><day>27</day><month>3</month><year>2010</year></date></acc><pub><date><day>16</day><month>4</month><year>2010</year></date></pub></history>
      <cpyrt><year>2010</year><collab>The Author(s)</collab></cpyrt>
      <kwdg>
         <kwd>Time-resolved photoluminescence</kwd>
         <kwd>Quantum dot chain</kwd>
         <kwd>Interdot coupling</kwd>
      </kwdg>
      <abs>
         <sec>
            <st>
               <p>Abstract</p>
            </st>
            <p>Multilayer In<sub>0.4</sub>Ga<sub>0.6</sub>As/GaAs quantum dot (QD) chain samples are investigated by means of cw and time-resolved photoluminescence (PL) spectroscopy in order to study the peculiarities of interdot coupling in such nanostructures. The temperature dependence of the PL has revealed details of the confinement. Non-thermal carrier distribution through in-chain, interdot wave function coupling is found. The peculiar dependences of the PL decay time on the excitation and detection energies are ascribed to the electronic interdot coupling and the long-range coupling through the radiation field. It is shown that the dependence of the PL decay time on the excitation wavelength is a result of the superradiance effect.</p>
         </sec>
      </abs>
   </fm>
   <meta>
      <classifications>
         <classification id="springerjournalsubject" type="Primary">Material Science</classification>
         <classification id="springerjournalsubject" type="Secondary">Molecular Medicine </classification>
         <classification id="springerjournalsubject" type="Secondary">Engineering, general</classification>
         <classification id="springerjournalsubject" type="Secondary">Chemistry/Food Science, general </classification>
         <classification id="springerjournalsubject" type="Secondary">Physics, general</classification>
         <classification id="springerjournalsubject" type="Secondary">Materials Science, general</classification>
         <classification id="springerjournalsubject" type="Secondary">Nanotechnology</classification>
      </classifications>
   </meta>
   <bdy>
      <sec>
         <st>
            <p>Introduction</p>
         </st>
         <p>Self-assembled (In,Ga)As/GaAs quantum dots (QDs) demonstrate many favorable physical properties that makes them suitable for numerous device applications <abbrgrp><abbr bid="B1">1</abbr><abbr bid="B2">2</abbr><abbr bid="B3">3</abbr><abbr bid="B4">4</abbr></abbrgrp>. They possess high radiative efficiency and easily controllable areal densities; allow engineering of the energy levels permitting efficient carrier injection from a semiconductor matrix. Typically, (In,Ga)As/GaAs QDs have ~2&#8211;5 nm height and ~20&#8211;50 nm base width. Due to small QD sizes and high confinement potential, the electron and hole states are fully quantized and their wavefunctions are strictly localized within the QD area with a &#948;-like density of states. Therefore, the self-assembled QDs can be treated to some extent as nearly ideal zero-dimensional (0D) systems behaving themselves like a &#8220;frozen ideal gas&#8221;.</p>
         <p>Each individual QD offers several advantages as a source for single photons. It has high oscillator strength and narrow spectral linewidth (~0.01 meV) and does not suffer from photobleaching or shelving. However, these idealizations have to be substantially modified in case of QD densities lying in the range of ~10<sup>10</sup>&#8211;10<sup>11</sup> cm<sup>&#8722;2</sup>. These densities result in mean dot separation of the order of tens to hundreds of nanometers which is comparable with the sizes of the individual QDs. Unavoidable size fluctuations within the QD ensemble lead to an additional inhomogeneous broadening of the optical spectra, frequently making the observation of the intrinsic 0D behavior difficult. Another characteristic of QD ensemble the interdot coupling is usually grouped into two categories with regard to whether it occurs via overlapping wave functions (electronic coupling) of the spatially separated QDs or via long-range electromagnetic interactions.</p>
         <p>Depending on the strength of electronic coupling between neighboring QDs, their individual electronic states and the relaxation of the photo-excited carriers through those states can be significantly altered. In the case of strong coupling, they can form QD molecules <abbrgrp><abbr bid="B5">5</abbr></abbrgrp>, resulting in new physics and a number of applications such as an excitonic qubit system with potential scalability <abbrgrp><abbr bid="B6">6</abbr></abbrgrp>. In the case of intermediate or weak coupling, the energy and carrier transfer between QDs occurs through quantum&#8211;mechanical tunneling that substantially affects recombination, carrier injection, and lasing in the QD system <abbrgrp><abbr bid="B7">7</abbr><abbr bid="B8">8</abbr><abbr bid="B9">9</abbr><abbr bid="B10">10</abbr><abbr bid="B11">11</abbr></abbrgrp>.</p>
         <p>The long-range radiative coupling between QDs in an ensemble can be interpreted in terms of successive emission and reabsorption of photons resulting in collective modes of several QDs. In this case, the exciton state of a single QD cannot be treated as a stationary state since its excitation in an individual QD will be transferred to other QDs <abbrgrp><abbr bid="B12">12</abbr></abbrgrp>. In addition, energy transfer between dots can be in the form of an electrostatic dipole&#8211;dipole interaction, frequently cited as F&#246;rster energy transfer <abbrgrp><abbr bid="B13">13</abbr></abbrgrp>. In the case of InP QDs with interdot distance of 7 nm, the F&#246;rster time for the excitation transfer between two QDs has been estimated <abbrgrp><abbr bid="B14">14</abbr></abbrgrp> to be in the range of 10<sup>2</sup>&#8211;10<sup>3</sup> ps. This F&#246;rster transfer rate is proportional to the fourth power of the dipole moment matrix element and decays as the sixth power of the interdot distance <abbrgrp><abbr bid="B14">14</abbr></abbrgrp>. Complementary to the F&#246;rster energy transfer, the polariton coupling is also expected to have a long spatial range, of the order of a few photon wavelengths. This mechanism results in the transfer of electron&#8211;hole excitation between distant QDs mediated by the emission and reabsorption of the transverse electromagnetic field <abbrgrp><abbr bid="B12">12</abbr></abbrgrp>. Typical transfer rates attributed to polariton coupling are in the range of 10<sup>&#8722;3</sup>&#8211;10<sup>&#8722;4</sup> ps<sup>&#8722;1</sup>. It is proportional to the square of the dipole moment matrix element and decays as the inverse of the interdot distance, if the transfer is mediated by a propagating field in two dimensions. Thus, in presence of radiative interaction, in fact, even very remote QDs cannot be considered as isolated systems, and the QD ensemble is expected to develop signatures of cooperative radiation or superradiation <abbrgrp><abbr bid="B15">15</abbr></abbrgrp>. In order to strengthen the QD coupling through their radiation field, the use of semiconductor microcavities has been proposed and strong interaction between single QDs and the cavity mode has been already demonstrated <abbrgrp><abbr bid="B16">16</abbr></abbrgrp>.</p>
         <p>In the case of QD ensembles with well-separated QDs, the fingerprint of cooperative effects in radiation is the change of the photoluminescence (PL) decay time with a change in the number of interacting QDs and their respective separation <abbrgrp><abbr bid="B12">12</abbr><abbr bid="B17">17</abbr></abbrgrp>. The number and interdot separation of the dots can be varied using postprocessing of as-grown samples. For example, the dots could be covered by a mask containing small apertures through which the optical excitation as well as the collection of the signal is done. A lateral patterning of the sample surface offers another possibility. In this case, small mesa structures are fabricated which contain only a single QD or a few QDs. In case of CdSe/ZnSe QDs studied in Ref. <abbrgrp><abbr bid="B17">17</abbr></abbrgrp>, mesas of the same size were arranged in a grid-like pattern over an area larger than the size of the laser spot on the sample. Mesas of sizes down to a few tens of nanometers were etched into the QD sample removing the QDs from between the mesas. It has been shown <abbrgrp><abbr bid="B17">17</abbr></abbrgrp> that the radiative interaction between QDs disappears with decreasing mesa size.</p>
         <p>Recently, the new laterally ordered self-assembled (In,Ga)As/GaAs QD stack has been grown by molecular-beam epitaxy (MBE) <abbrgrp><abbr bid="B18">18</abbr></abbrgrp>. QDs align in long rows forming QD chains. It has been found that the dot chains can be substantially increased in length by the introduction of growth interruptions during the initial stages of growth of the GaAs spacer layer. The growth procedure has been also used to create a template to arrange InAs dots into chains with a predictable dot density. The resulting dot chains offer the possibility to engineer interdot coupling for novel physical phenomena and potential devices. Here, the distance between neighboring QD chains can be made sufficiently large as to prevent the immediate electron&#8211;hole wavefunction tunneling as well as the F&#246;rster energy transfer between QDs belonging to different chains. This looks like as a natural mesa between chains. The objective of our research is the study of the peculiarities of interdot coupling in these new laterally ordered self-assembled (In,Ga)As/GaAs QD structures. In this case, we can expect the superradiance effect from the dot-chain ensemble. It is important that in-chain interdot coupling is easily changeable also thus permitting to study the cooperative effects caused by immediate interdot carrier tunneling.</p>
         <p>We use the multilayer (In,Ga)As/GaAs dot-chain structure to reveal various cooperative effects arising both through overlapping wave functions of the spatially separated QDs and through long-range radiative interactions between QDs. &#8220;Experiment&#8221; includes the details of sample growth together with results of AFM analysis of the grown structure. The details of the PL are given. &#8220;Temperature cw PL measurements&#8221; includes the results of the temperature investigation of the cw PL. This results in information about the energy scheme of the system and provides evidence of interdot coupling and carrier transfer in QD chains. &#8220;Time-resolved PL measurements and mechanisms of interdot coupling&#8221; represents the results of the time-resolved PL measurements and contains the theoretical model used for the interpretations of the time-resolved PL data. Last section contains concluding remarks.</p>
      </sec>
      <sec>
         <st>
            <p>Experiment</p>
         </st>
         <p>The multilayer (In,Ga)As/GaAs dot-chain structures were prepared in order to study the actual mechanisms of interdot coupling which lead in part to the appearance of cooperative effects. In<sub><it>x</it></sub>Ga<sub>1&#8722;<it>x</it></sub>As QDs were grown by molecular beam epitaxy (MBE) on semi-insulating GaAs (100) substrates such that dot chains form <abbrgrp><abbr bid="B18">18</abbr></abbrgrp>. Following a 0.3-&#956;m GaAs buffer layer grown at 580&#176;C, the growth of In<sub>0.4</sub>Ga<sub>0.6</sub>As QDs capped by 60 MLs of GaAs, both at 540&#176;C, was repeated for a 15 layer superlattice. The In<sub>0.4</sub>Ga<sub>0.6</sub>As QD layers were grown by the deposition of 8.5 ML of material. A final QD layer was grown and left uncapped for morphology analysis. The atomic force microscopy (AFM) image of the final, uncapped QD layer, Fig. <figr fid="F1">1a</figr>, demonstrates that these InGaAs QDs are formed in chains along the [0-11] direction. Figure <figr fid="F1">1b</figr> shows the Fourier transformed AFM image of an area with sizes 4 &#215; 4 &#956;m<sup>2</sup>. The arrows pointed out the maxima along the directions of the QD alignment, [0-11] and [011]. Figure <figr fid="F1">1c</figr> presents a histogram of the QD aspect ratio. It is seen that the mean aspect ratio is ~0.11. Based on these results, the average spacing between chains is estimated to be 90 nm, while the separation between QDs in the chains is around 45 nm, close to the lateral size of QDs. As a result, it is expected that any observed lateral electronic coupling will be predominantly between the QDs in a single chain and negligible between interchain QDs. However, analysis of the PL reveals a much more complicated system of interaction and coupling between the dots. Note that in our multilayer structures the GaAs spacer between adjacent QD layers was thick enough (approximately 60 MLs thick) to prevent any vertical QD ordering. In this case, adjacent QD layers can be considered as independent QD systems (see e.g. Ref. <abbrgrp><abbr bid="B11">11</abbr></abbrgrp>) and many layers serve predominantly to enhance the total PL gain.</p>
         <fig id="F1"><title><p>Figure 1</p></title><caption><p>a AFM image of the uncapped (In,Ga)As/GaAs QD structure</p></caption><text>
   <p><b>a</b> AFM image of the uncapped (In,Ga)As/GaAs QD structure. <b>b</b> Fourier-transformed AFM image of an area with sizes 4 &#215; 4 &#956;m<sup>2</sup>. The <it>arrows</it> pointed out the maxima along the directions of the QD alignment, [0-11] and [011]; <b>c</b> Histogram of QD distribution by the aspect ratio</p>
</text><graphic file="1556-276X-5-991-1"/></fig>
         <p>The PL was performed using the 532-nm line from a frequency doubled Nd:YAG (neodymium-doped yttrium aluminum garnet) laser for continuous-wave PL excitation and the 2-ps pulses at &#955;<sub>exc</sub> = 750 nm from a mode-locked Ti:sapphire laser for transient PL measurements. The optical pulse train at 76 MHz and an excitation density that was varied between 10<sup>9</sup> and 2 &#215; 10<sup>14</sup> photons/(pulse &#215; cm<sup>2</sup>) was used. The steady-state PL signal from the sample was dispersed by a 0.5-m single-grating monochromator and detected by a LN-cooled OMA V: InGaAs photodiode detector array. The PL transients were detected with a Hamamatsu synchroscan streak camera C5680 with an infrared enhanced S1 cathode. The overall time resolution of the system used in the time-resolved PL measurements was ~15 ps.</p>
      </sec>
      <sec>
         <st>
            <p>Temperature cw PL Measurements</p>
         </st>
         <p>In order to get the information about both the energy scheme of the InGaAs/GaAs dot chain sample and the channels of the interdot carrier transfer, the temperature-dependent PL spectra are measured (Fig. <figr fid="F2">2</figr>). The low temperature (<it>T</it> = 10 K) and low excitation intensity (<it>I</it><sub>exc</sub> = 0.4 W/cm<sup>2</sup>) cw PL measurements reveal a single peak for the ground state exciton emission with a maximum at <it>E</it><sub>max</sub> = 1.247 eV and full width at half maximum (FWHM) of <it>&#915;</it> ~ 48 meV (Fig. <figr fid="F2">2</figr>). Increasing the temperature from 10 K up to 300 K shifts the PL band to the red by ~67 meV and broadens almost twice, up to ~87 meV. At the temperatures as high as 150 K, the PL is found to broaden asymmetrically, favoring the higher energy. The results of fit with two Gaussians, <inline-formula><graphic file="1556-276X-5-991-i15.gif"/></inline-formula><it>&#915;</it><sub>1</sub> = 49 meV and <inline-formula><graphic file="1556-276X-5-991-i16.gif"/></inline-formula><it>&#915;</it><sub>2</sub> = 60 meV, are shown in the PL spectrum measured for <it>T</it> = 150 K by dashed lines (Fig. <figr fid="F2">2</figr>). Therefore, the high temperature asymmetry is partly a result of thermal population of the higher energy confined states in the dots. More precise behavior of the PL peak maximum and the FWHM versus temperature is shown in Fig. <figr fid="F3">3</figr>. The temperature dependence of the FWHM (Fig. <figr fid="F3">3a</figr>) demonstrates a non-monotonic behavior. It reaches a minimum at ~80 K and then grows significantly with increasing temperature. The PL redshift (~32 meV, see Fig. <figr fid="F3">3b</figr>) is greater than the redshift of InAs (~13 meV, curve 3 in Fig. <figr fid="F3">3b</figr>) or GaAs (~17 meV, not shown here) upon increasing the temperature from 10 K to 100 K.</p>
         <fig id="F2"><title><p>Figure 2</p></title><caption><p>Normalized PL spectra for the multilayer In0</p></caption><text>
   <p>Normalized PL spectra for the multilayer In<sub>0.4</sub>Ga<sub>0.6</sub>As/GaAs QD chain sample measured at different temperatures. For clarity, the spectra are vertically shifted with respect to each other. Two Gaussians best fitting the PL spectrum measured at <it>T</it> = 150 K are shown by <it>dashed lines</it></p>
</text><graphic file="1556-276X-5-991-2"/></fig>
         <fig id="F3"><title><p>Figure 3</p></title><caption><p>Temperature dependences of a FWHM (curve 1), and b PL band maximum Emax (curve 1) measured in the QD sample</p></caption><text>
   <p>Temperature dependences of <b>a</b> FWHM (<it>curve 1</it>), and <b>b</b> PL band maximum <it>E</it><sub>max</sub> (<it>curve 1</it>) measured in the QD sample. The results of fit with the set of parameters &#916; = 15 K and <it>T</it><sub>th</sub> = 60 K to Eqs. (1) and (2) are shown by <it>curve 2</it> in Fig. <figr fid="F3">3a</figr>, <figr fid="F3">3b</figr>. Temperature dependence of InAs energy gap followed the Varshni law <abbrgrp><abbr bid="B22">22</abbr></abbrgrp> is given by <it>curve 3</it> in Fig. <figr fid="F3">3b</figr></p>
</text><graphic file="1556-276X-5-991-3"/></fig>
         <p>The initial PL spectrum narrowing in the temperature range between 10 and 80 K is ascribed to thermally induced carrier transfer between the QDs within each chain. According to a simple thermionic model <abbrgrp><abbr bid="B19">19</abbr><abbr bid="B20">20</abbr></abbrgrp>, at low <it>T</it>, carriers are &#8220;frozen&#8221; randomly into the QD states (after initial partial redistribution) due to the tunneling between QDs within each chain. With increasing <it>T</it>, carriers are expected to be thermally activated outside the dots into the 2D InGaAs wetting layer (WL) or GaAs barrier and/or hopping between dots will favor a drift of carriers toward the dots having lower ground state energies. This results in a narrowing of the PL spectrum and a redshift for the PL peak that is larger than expected from the thermal shrinkage of the InAs band gap under elevating <it>T</it>. In order to describe such a process, one can use either the rate equation model <abbrgrp><abbr bid="B19">19</abbr></abbrgrp> or a simplified quasi-thermodynamic model <abbrgrp><abbr bid="B20">20</abbr></abbrgrp> that introduces a temperature dependent function <it>&#946;</it>(<it>T</it>) allowing to parameterize the degree of thermalization of carriers. This function continuously interpolates between the well-defined low and high-temperature limits of the carrier distribution function and describes the observed peculiarities in the PL spectra with just two fitting parameters. In fact, such a description is equivalent to the assumption that partially thermalized carriers are still described by equilibrium statistics, but with a higher effective temperature <it>T</it><sub>th</sub>. Following to Ref. <abbrgrp><abbr bid="B20">20</abbr></abbrgrp>, the QD PL spectra (<it>I</it>(<it>E</it>)) can be treated using a relation like</p>
         <p>
            <display-formula>
               <graphic file="1556-276X-5-991-i1.gif"/>
            </display-formula>
         </p>
         <p>with <it>I</it><sub>0</sub>(<it>T</it>) being the temperature-dependent scale factor <abbrgrp><abbr bid="B21">21</abbr></abbrgrp> and <it>E</it><sub>g</sub> representing the temperature-dependent energy gap for InAs described, say, by the Varshni formula <abbrgrp><abbr bid="B22">22</abbr></abbrgrp>. Parameter <it>A</it> enters the relationship between the transition energies and the dot sizes <abbrgrp><abbr bid="B23">23</abbr></abbrgrp> and is taken to be equal <it>A</it> = 2.37 eV nm<sup>1/2</sup> for our QDs. The QD ensemble is characterized by a Gaussian size distribution with a variance <it>o</it><sup>2</sup>/2 and mean basal length <it>a</it><sub>0</sub> corresponding to the ground state transition energy <it>E</it><sub>0</sub>. The thermalization function <it>&#946;</it>(<it>T</it>) reflects all the carrier dynamics through the multiple pathways and can be approximated by expression <abbrgrp><abbr bid="B20">20</abbr></abbrgrp></p>
         <p>
            <display-formula>
               <graphic file="1556-276X-5-991-i2.gif"/>
            </display-formula>
         </p>
         <p>with <it>T</it><sub>th</sub> and <it>&#916;</it> being the only two fit parameters of the model. <it>T</it><sub>th</sub> is the temperature when <it>&#946;</it> = 0.5 and <it>&#916;</it> corresponds to the temperature interval over which the transition from a &#8220;glassy&#8221; to a quasi-equilibrium state occurs.</p>
         <p>Using Eqs (1) and (2) with the set of parameters <it>E</it><sub>0</sub> = 1.247 eV and <it>&#916;</it> = 48 meV taken at the lowest temperature (<it>T</it> = 10 K) for a Gaussian describing the low temperature PL spectrum (Fig. <figr fid="F2">2</figr>), we find the best fit of the FWHM (T) (Fig. <figr fid="F3">3a</figr>) and <it>E</it><sub>max</sub>(<it>T</it>) (Fig. <figr fid="F3">3b</figr>) dependences with the parameters <it>&#916;</it> = 15 K and <it>T</it><sub>th</sub> = 60 K in the temperature range from 10 to 125 K. While the theoretical analysis carried out earlier is applied only for the ground state QD transitions our fit is valuable in the temperature range, where the contribution of the excited states is negligible. It follows from Fig. <figr fid="F2">2</figr> that this range spreads from ~10 K up to ~150 K. It is important to note that the narrowing of PL the band width with an increase in temperature from ~10 to 100 K (see Fig. <figr fid="F3">3a</figr>) is not intuitive. One might expect the contrary, i.e., the FWHM increasing due to thermal broadening. Therefore, a good fit of the FWHM (T) dependence in this temperature range supports well the description of data in terms of the quasi-thermodynamic model presented earlier. In turn, the description of the <it>E</it><sub>max</sub>(<it>T</it>) dependence (see Fig. <figr fid="F3">3b</figr>) in the low-temperature range requires more elaborate analysis of the physical processes that determine the band-gap behavior in the QD system with increased temperature, e.g., electron&#8211;phonon coupling. The absence of such analysis can be in part an origin for the absence of a perfect fit for the <it>E</it><sub>max</sub>(<it>T</it>) data shown in Fig. <figr fid="F3">3b</figr> performed using the Varshni formula <abbrgrp><abbr bid="B22">22</abbr></abbrgrp> for the temperature dependence of the energy gap in InAs QDs. For higher temperatures, the contribution of the excited states in the FWHM formation becomes significant leading to a significant deviation of calculated dependences from measured dependences observed in Fig. <figr fid="F3">3</figr> in the temperature range above 150 K. Significantly small <it>T</it><sub>th</sub> value in comparison with that <it>T</it><sub>th</sub> = 127 K found earlier for the InAs/GaAs QDs <abbrgrp><abbr bid="B19">19</abbr><abbr bid="B20">20</abbr></abbrgrp> gives evidence of the existence of non-thermal relaxation mechanism favoring the thermalization of the QD system even at the lowest temperatures. Such a mechanism is the interdot tunneling caused by the electronic coupling between the dots of the same chain. In this case, carriers escape from the smaller QDs with higher ground state energy to the larger QDs with lower ground state energy. Such escape results in the higher population of the lower energy QD states in comparison with the population of the energy states of smaller QDs under the steady-state PL excitation and equal rate of the carrier trap on the small and large QDs. As a result, the PL band of the QD ensemble, which possesses a symmetric QD size distribution described by a Gaussian, has to be asymmetric with a more abrupt high-energy side. Introducing the asymmetry measure as the difference <inline-formula><graphic file="1556-276X-5-991-i17.gif"/></inline-formula><it>&#948;</it> = <it>E</it> &#8722; <it>E</it><sub>max</sub>, one can expect the positive asymmetry in case of low temperatures. Such determined asymmetry of the PL band is shown in Fig. <figr fid="F4">4</figr>. It occurs positive at the T = 10 K evidencing the non-thermal carrier distribution in the QD ensemble at low temperatures. Further temperature increase leads to the subsequent temperature population of the higher energy levels of smaller QDs thus decreasing the PL band asymmetry and finally switches the sign of asymmetry to the negative one. Such a behavior of the PL band asymmetry under the temperature increasing is demonstrated in Fig. <figr fid="F4">4</figr>. As one can see from Fig. <figr fid="F4">4</figr>, the well-pronounced PL band develops at the high-energy side of the dominant PL band. This band in the difference spectrum is shifted by ~38 meV from the PL peak position toward higher energy that quite well correlates with the energy difference <inline-formula><graphic file="1556-276X-5-991-i18.gif"/></inline-formula> found from the PL line shape analysis carried out in Fig. <figr fid="F2">2</figr> for <it>T</it> = 150 K. Our calculations of the QD energy spectrum show that in the In<sub>0.4</sub>Ga<sub>0.6</sub>As/GaAs QD with the aspect ratio ~0.1 only one level <it>e</it><sub>1</sub> is generated in the conduction band and at least two levels of heavy hole states (hh<sub>1</sub> and hh<sub>2</sub>) arise in the valence band. Thus, we ascribe the main PL peak to the <it>e</it><sub>1</sub> &#8594; hh<sub>1</sub> intradot transition, whereas complementary high-energy peak arising at high temperatures is assigned to the <it>e</it><sub>1</sub> &#8594; hh<sub>2</sub> transition developing due to the thermal population of the hh<sub>2</sub> hole state. This additional transition significantly modifies the PL line shape at higher temperatures (Fig. <figr fid="F2">2</figr>) and introduces additional PL band broadening resulting in a significant deviation of the calculated temperature dependences from measured temperature dependences of FWHM and PL <it>E</it><sub>max</sub> within the temperature range 150&#8211;300 K (Fig. <figr fid="F3">3a</figr>, <figr fid="F3">3b</figr>). It is clear that the asymmetry of the PL band, measured directly (Fig. <figr fid="F4">4</figr>), gives information about both the intra- and interdot-chain carrier relaxation. Thus, it provides more information than one can obtain, say, from a Gaussian fit of the PL spectra (Fig. <figr fid="F2">2</figr>).</p>
         <fig id="F4"><title><p>Figure 4</p></title><caption><p>PL band asymmetry measured as difference <inline-formula><graphic file="1556-276X-5-991-i45.gif"/></inline-formula>, &#948; = E &#8722; Emax for various temperatures</p></caption><text>
   <p>PL band asymmetry measured as difference <inline-formula><graphic file="1556-276X-5-991-i45.gif"/></inline-formula>, <it>&#948;</it> = <it>E</it> &#8722; <it>E</it><sub>max</sub> for various temperatures. It is seen that low-temperature (<it>T</it> = 10 K) asymmetry is positive. The change of asymmetry sign evidences the appearance of the <it>e</it><sub>1 </sub>&#8722; hh<sub>2</sub> QD transition and the predominant temperature population of the shallow QD states at high temperatures</p>
</text><graphic file="1556-276X-5-991-4"/></fig>
         <p>Analysis of the temperature dependence of the integrated PL for the multilayer In<sub>0.4</sub>Ga<sub>0.6</sub>As/GaAs QD chain sample gives further verification of the contribution from the <it>e</it><sub>1</sub> &#8594; hh<sub>2</sub> QD transition. Figure <figr fid="F5">5</figr> shows this dependence. At least three Arrhenius-type activation energies can be extracted from the plot in Fig. <figr fid="F5">5</figr>: <inline-formula><graphic file="1556-276X-5-991-i19.gif"/></inline-formula>, <inline-formula><graphic file="1556-276X-5-991-i20.gif"/></inline-formula>, and <inline-formula><graphic file="1556-276X-5-991-i21.gif"/></inline-formula><inline-formula><graphic file="1556-276X-5-991-i22.gif"/></inline-formula> quite satisfactorily agrees with the energy 38 meV extracted from the high temperature difference PL spectra (Fig. <figr fid="F4">4</figr>) for the <it>e</it><sub>1</sub> &#8594; hh<sub>2</sub> transition. The energy <inline-formula><graphic file="1556-276X-5-991-i23.gif"/></inline-formula> we ascribe to the transition from the QD electron ground state (<it>e</it><sub>1</sub>) to the 2D conduction band (<inline-formula><graphic file="1556-276X-5-991-i24.gif"/></inline-formula>) of WL, <inline-formula><graphic file="1556-276X-5-991-i25.gif"/></inline-formula>. Indeed this predicts the 2D WL in our system to be ~1.468 eV which is very close to the energy 1.445 eV that has been observed for the 2D In<sub>0.36</sub>Ga<sub>0.64</sub>As WL in similar QD samples under high optical pumping <abbrgrp><abbr bid="B24">24</abbr></abbrgrp>. We were not able to saturate the QD states to see the WL in our samples due to the large density of dots. The energy <inline-formula><graphic file="1556-276X-5-991-i26.gif"/></inline-formula> we ascribe to the transition from the QD ground states to a 1D WL. Its energy is of about 1.391 eV. The existence of such WL is specific for the dot chain sample and has been proved recently by means of scanning electron, transmission electron, and atomic force microscopies <abbrgrp><abbr bid="B25">25</abbr></abbrgrp> as well as by optical spectroscopy <abbrgrp><abbr bid="B26">26</abbr></abbrgrp>. It has been shown that in addition to the conventional 2D WL involved in the Stranski&#8211;Krastanov growth a 1D-postwetting layer along the [01 &#8722; 1] direction arises that connects the QDs in each chain. Whereas the 2D WL exists before the QD chains form, the 1D-postwetting layer develops during the GaAs capping of already existing dot chains. It arises due to anisotropic surface diffusion of In atoms that accompanies the change in strain profile during capping and therefore produces the steady-state material distribution that includes a 1D-postwetting layer as a result.</p>
         <fig id="F5"><title><p>Figure 5</p></title><caption><p>Semi-logarithmic plot of the integrated PL versus inverse temperature for the multilayer In0</p></caption><text>
   <p>Semi-logarithmic plot of the integrated PL versus inverse temperature for the multilayer In<sub>0.4</sub>Ga<sub>0.6</sub>As/GaAs QD chain sample. Three Arrhenius-type activation energies are extracted from the plot: <inline-formula><graphic file="1556-276X-5-991-i46.gif"/></inline-formula><inline-formula><graphic file="1556-276X-5-991-i47.gif"/></inline-formula> and <inline-formula><graphic file="1556-276X-5-991-i48.gif"/></inline-formula></p>
</text><graphic file="1556-276X-5-991-5"/></fig>
         <p>Thus, the existence of various discrete and continuous states in the multilayer In<sub>0.4</sub>Ga<sub>0.6</sub>As/GaAs QD chain sample substantially complicates the real picture of relaxation and coupling of the QDs. Based on the temperature dependence of the PL spectra, we can distinguish the low temperature effects caused by the in-chain interdot coupling and high temperature effects related to the QD coupling through the WL and GaAs barrier states. To go further, we focus on the low-temperature interdot coupling. We have demonstrated the cooperative effects caused by in-chain, interdot electronic coupling that becomes transformed into a change of the low temperature PL band and its line-shape. The features related to the interdot-chain, long-range radiative coupling are explored by means of time-resolved PL spectroscopy.</p>
      </sec>
      <sec>
         <st>
            <p>Time-Resolved PL Measurements and Mechanisms of Interdot Coupling</p>
         </st>
         <p>The low temperature PL transients for the multilayer In<sub>0.4</sub>Ga<sub>0.6</sub>As/GaAs(001) QD chain sample are shown in Fig. <figr fid="F6">6</figr>. The excitation density is chosen to be comparatively low in order to provide the mono-exponential PL decay following the law <inline-formula><graphic file="1556-276X-5-991-i27.gif"/></inline-formula> under excitation with different wavelengths. Here, the time <it>t</it><sub>0</sub> corresponds to the beginning of declining part of the <it>I</it><sub><it>PL</it></sub>(<it>t</it>) dependence and is set to be 0 in further analysis. The rate of decay is characterized with time <it>&#964;</it><sub>d</sub>. The characteristic rise time for all PL transients is found to not exceed ~20 ps indicating that the carriers are trapped quickly by all QDs. Figure <figr fid="F6">6a</figr> shows the transients measured with the excitation wavelength <it>&#955;</it><sub>exc</sub> = 750 nm and the detection wavelengths <it>&#955;</it><sub>det</sub> = 930 nm, 950 nm, 995 nm, and 1030 nm covering the region of the QD ground state emission. For comparison the laser pulse is also shown indicating that the observed PL decay is related to the QD system response only. Figure <figr fid="F6">6b</figr> shows the transients measured at the peak of the ground state emission, <it>&#955;</it><sub>det</sub> = 995 nm, with pulsed laser excitation varied between &#955;<sub>exc</sub> = 720 nm (above the GaAs bandgap) and &#955;<sub>exc</sub> = 870 nm (below the GaAs bandgap and the InGaAs WL as shown in &#8220;Temperature cw PL measurements&#8221;). The observed exponential PL decay is well characterized by a single <it>&#964;</it><sub>d</sub> value depending nevertheless both on the <it>&#955;</it><sub>exc</sub> and <it>&#955;</it><sub>det</sub>. Figure <figr fid="F7">7</figr> summarizes the <it>&#964;</it><sub>d</sub>(<it>E</it><sub>det</sub>) data measured for various excitation energies <it>E</it><sub>exc</sub>. The <inline-formula><graphic file="1556-276X-5-991-i28.gif"/></inline-formula> dependences are plotted versus the difference<inline-formula><graphic file="1556-276X-5-991-i29.gif"/></inline-formula>. Qualitative analysis of all <inline-formula><graphic file="1556-276X-5-991-i30.gif"/></inline-formula> dependences allows four items to be explained: i) rapid increasing of <inline-formula><graphic file="1556-276X-5-991-i31.gif"/></inline-formula> with decreasing <it>E</it><sub>det</sub> throughout the QD PL spectrum; ii) reaching the maximal <inline-formula><graphic file="1556-276X-5-991-i32.gif"/></inline-formula> when <it>E</it><sub>det</sub> reaches the PL maximum; iii) decreasing the maximal <inline-formula><graphic file="1556-276X-5-991-i33.gif"/></inline-formula> values with decreasing the excitation energy <it>E</it><sub>exc</sub>; and iv) appearance of the dip on the <inline-formula><graphic file="1556-276X-5-991-i34.gif"/></inline-formula> dependences for the detection energies lower than <it>E</it><sub>0</sub>. In order to address these four points we involve two different mechanisms of interdot coupling and the mechanisms of QD coupling with the host material and inherent defects finally affecting the <it>&#964;</it><sub>d</sub> value.</p>
         <fig id="F6"><title><p>Figure 6</p></title><caption><p>a Low-temperature PL transients measured at various &#955;det for a constant excitation wavelength &#955;exc = 750 nm in the multilayer In0</p></caption><text>
   <p><b>a</b> Low-temperature PL transients measured at various <it>&#955;</it><sub>det</sub> for a constant excitation wavelength <it>&#955;</it><sub>exc</sub> = 750 nm in the multilayer In<sub>0.4</sub>Ga<sub>0.6</sub>As/GaAs QD chain sample. <it>&#955;</it><sub>det</sub> = 995 nm corresponds to the PL maximum. Laser pulse presents the response of the detecting system. <b>b</b> PL transients measured under two different <it>&#955;</it><sub>exc</sub> at the position of the PL maximum, <it>&#955;</it><sub>det</sub> = 995 nm</p>
</text><graphic file="1556-276X-5-991-6"/></fig>
         <fig id="F7"><title><p>Figure 7</p></title><caption><p>The <inline-formula><graphic file="1556-276X-5-991-i49.gif"/></inline-formula> data measured for various excitation energies Eexc</p></caption><text>
   <p>The <inline-formula><graphic file="1556-276X-5-991-i49.gif"/></inline-formula> data measured for various excitation energies <it>E</it><sub>exc</sub>. The <inline-formula><graphic file="1556-276X-5-991-i50.gif"/></inline-formula> dependences are plotted versus the difference <inline-formula><graphic file="1556-276X-5-991-i51.gif"/></inline-formula>. <it>E</it><sub>0</sub> = 1.246 eV presents the position of the low temperature PL maximum</p>
</text><graphic file="1556-276X-5-991-7"/></fig>
         <sec>
            <st>
               <p>Electronic Wave Function Interdot Coupling</p>
            </st>
            <p>Figure <figr fid="F8">8</figr> shows <it>&#964;</it><sub>d</sub>(<it>E</it><sub>det</sub>) dependences measured at <it>E</it><sub>exc</sub> = 1.722 eV and <it>E</it><sub>exc</sub> = 1.477 eV together with the normalized low temperature PL spectrum. We find these dependences resembling the typical <it>&#964;</it><sub>d</sub>(<it>E</it><sub>det</sub>) dependences observed earlier in dense QD arrays <abbrgrp><abbr bid="B27">27</abbr><abbr bid="B28">28</abbr></abbrgrp>, which were described using lateral interdot transfer. Taking into account our finding of &#8220;Temperature cw PL measurements&#8221; concerning the in-chain interdot coupling, we first apply this description to our dot chain sample. The carrier dynamics in the QD system under excitation with a weak electromagnetic field can be treated with a system of rate equations. The lateral coupling is introduced through tunneling along the (In,Ga)As/GaAs QD chains as has been revealed recently <abbrgrp><abbr bid="B29">29</abbr></abbrgrp>. In this case, the change of the population, <it>n</it> = <it>n</it>(<it>E</it>), of the QD ground state <it>E</it> for QD ensemble excited by the <it>E</it><sub><it>exc</it></sub> photon is given by the equation <abbrgrp><abbr bid="B10">10</abbr></abbrgrp></p>
            <p>
               <display-formula>
                  <graphic file="1556-276X-5-991-i3.gif"/>
               </display-formula>
            </p>
            <p/>
            <fig id="F8"><title><p>Figure 8</p></title><caption><p>The &#964;d(Edet) data measured for two different excitation energies (symbols) and simulated &#964;d(Edet) dependence (curve 1) using the rate Eqs</p></caption><text>
   <p>The <it>&#964;</it><sub>d</sub>(<it>E</it><sub>det</sub>) data measured for two different excitation energies (<it>symbols</it>) and simulated <it>&#964;</it><sub>d</sub>(<it>E</it><sub>det</sub>) dependence (<it>curve 1</it>) using the rate Eqs. (3), (5), and (6) with <it>&#964;</it><sub>op</sub> = 1 and <it>&#964;</it><sub><it>T</it></sub> = 1.4 ns (<it>solid line</it>). Normalized PL spectrum (<it>curve 2</it>) is given for <it>T</it> = 10 K</p>
</text><graphic file="1556-276X-5-991-8"/></fig>
            <p>Here, 1/<it>&#964;</it><sub><it>op</it></sub>(<it>E</it>, <it>E</it><sub>exc</sub>) represents the rate of the radiative recombination, <it>R</it><sub>1</sub>(<it>E</it>, <it>t</it>) represents the rate at which the QD population decreases through tunneling processes, and <it>R</it><sub>2</sub>(<it>E</it>, <it>E</it><sub>exc</sub>, <it>t</it>) represents the QD capture rate from the reservoir of photo-excited electrons. Taking into account that the PL intensity <it>I</it><sub>PL</sub>(<it>t</it>) &#8733; <it>n</it>(<it>t</it>), one can introduce the PL decay time like a formula</p>
            <p>
               <display-formula>
                  <graphic file="1556-276X-5-991-i4.gif"/>
               </display-formula>
            </p>
            <p>The explicit form of the relaxation terms introducing the tunneling time <it>&#964;</it><sub><it>T</it></sub> for the lateral carrier transfer is given by</p>
            <p>
               <display-formula>
                  <graphic file="1556-276X-5-991-i5.gif"/>
               </display-formula>
            </p>
            <p/>
            <p>
               <display-formula>
                  <graphic file="1556-276X-5-991-i6.gif"/>
               </display-formula>
            </p>
            <p/>
            <p>
               <display-formula>
                  <graphic file="1556-276X-5-991-i7.gif"/>
               </display-formula>
            </p>
            <p>Here, <it>N</it>(<it>E</it>) is the number of QDs with the ground state emission energy <it>E</it>; <it>D</it>(<it>E</it>) is the density of states function; <it>&#964;</it><sub><it>T</it></sub>(<it>E</it>, <it>E</it>&#8242;) is the tunneling time from the state <it>E</it> to the state <it>E</it>&#8242;, and <it>G</it>(<it>E</it>, <it>E</it><sub>exc</sub>) is the carrier generation rate in the state <it>E</it> by light with energy <it>E</it><sub>exc</sub>. For the QD ensemble, the <it>D</it>(<it>E</it>) is taken as a Gaussian, <inline-formula><graphic file="1556-276X-5-991-i35.gif"/></inline-formula> (see &#8220;Temperature cw PL measurements&#8221;). In fact Eq. (3) with the relaxation terms (5) and (6) describes carrier dynamics with a cascade-like carrier transfer from upper states to the lower QD states defined by the tunneling rate <inline-formula><graphic file="1556-276X-5-991-i36.gif"/></inline-formula> This equation allows for consideration of non-linear effects as well because the inequality (7) must hold strictly.</p>
            <p>For the sake of simplicity, we define a single tunneling time for all QDs, <it>&#964;</it><sub><it>T</it></sub>(<it>E</it>, <it>E</it>&#8242;) = <it>&#964;</it><sub><it>T</it></sub>, and independent of <it>E</it> and <it>E</it><sub>exc</sub> set the optical recombination time as <it>&#964;</it><sub>op</sub>(<it>E</it>, <it>E</it><sub>exc</sub>) = <it>&#964;</it><sub>op</sub> = 1 ns. Then, considering the case of a weak electromagnetic field and comparatively slow interdot transfer, <it>&#964;</it><sub><it>T</it></sub> = 1.4 ns <abbrgrp><abbr bid="B10">10</abbr><abbr bid="B27">27</abbr><abbr bid="B28">28</abbr></abbrgrp>, we also assume that <it>N</it>(<it>E</it>) &gt; &gt;<it>n</it>(<it>E</it><it>t</it>). This allows us to linearize Eqs. (3), (5), and (6) and solve them numerically. The result of such simulation is shown in Fig. <figr fid="F8">8</figr> by solid line. This demonstrates that the mechanism of interdot carrier tunneling allows us to qualitatively reproduce the observed rise of <it>&#964;</it><sub>d</sub>(<it>E</it><sub>det</sub>) with decreasing <it>E</it><sub>det</sub> through the range of the QD PL spectrum. The difference between experimental and calculated dependences can be reduced significantly if the saturation of the QD ground states is taken into account. This would allow us to shift the energies at which the calculated <it>&#964;</it><sub>d</sub>(<it>&#955;</it><sub>det</sub>) function saturates closer to the PL maximum as it is observed for the measured <it>&#964;</it><sub>d</sub>(<it>&#955;</it><sub>det</sub>) dependence. Thus, this mechanism of in-chain interdot tunneling is consistent with two items mentioned earlier: rapid increasing the <it>&#964;</it><sub>d</sub>(<it>E</it><sub>det</sub>) value within the QD PL spectrum and reaching the maximal <it>&#964;</it><sub>d</sub>(<it>E</it><sub>det</sub>) values at the energy corresponding to the energy of PL maximum. However, this simplified model cannot reproduce in principle two experimental facts: decreasing the maximal <it>&#964;</it><sub>d</sub>(<it>E</it><sub>det</sub>) values with decreasing the excitation energy <it>E</it><sub>exc</sub> and appearance of the dip on the <it>&#964;</it><sub>d</sub>(<it>E</it><sub>det</sub>) dependences for the detection energies lower than <it>E</it><sub>0</sub>. These two features are formed by complementary mechanisms: interdot coupling through radiation field and QD coupling with the host materials and inherent defects.</p>
         </sec>
         <sec>
            <st>
               <p>Radiation Field Interdot Coupling</p>
            </st>
            <p>In analyzing the <it>&#964;</it><sub>d</sub>(<it>E</it><sub>det</sub>) dependence in terms of Eqs. (3), (5) and (6), we assumed that <it>&#964;</it><sub>op</sub>(<it>E</it>, <it>E</it><sub>exc</sub>) = <it>&#964;</it><sub>op</sub> = const. However, it has been shown <abbrgrp><abbr bid="B30">30</abbr><abbr bid="B31">31</abbr><abbr bid="B32">32</abbr></abbrgrp> that <it>&#964;</it><sub>op</sub> depends on <it>E</it> in QD systems and can be written as</p>
            <p>
               <display-formula>
                  <graphic file="1556-276X-5-991-i8.gif"/>
               </display-formula>
            </p>
            <p>with <it>E</it> being the emitted photon energy and <inline-formula><graphic file="1556-276X-5-991-i37.gif"/></inline-formula> being the optical matrix element for the conduction-valence band transition. According to Eq. (8), the <it>&#964;</it><sub>op</sub> value inversely depends on the emission energy (<it>&#964;</it><sub>op</sub>(<it>E</it>) &#8733; 1/<it>E</it>). This monotonic behavior of <it>&#964;</it><sub>op</sub> can explain neither the dependence of <it>&#964;</it><sub>d</sub> on the <it>E</it><sub>exc</sub> nor the saturation of <it>&#964;</it><sub>d</sub> function observed experimentally. Because the strongest change of <it>&#964;</it><sub>d</sub> takes place near the QD PL maximum, which is related to the emission of the most numerous QDs, we might attribute the change to a cooperative effect. The cooperative emission from optically coupled oscillators <abbrgrp><abbr bid="B12">12</abbr></abbrgrp> has been revealed recently in a single layer of self-assembled CdSe/ZnSe QDs <abbrgrp><abbr bid="B17">17</abbr></abbrgrp> and in the (In,Ga)As/GaAs dot-chain superlattices <abbrgrp><abbr bid="B33">33</abbr></abbrgrp>. With optical collective interaction, the conventional radiation of <it>N</it> identical oscillators transforms into two different radiant modes: a superradiant mode with a shorter lifetime <it>&#964;</it><sub>spr</sub> &#8776; <it>&#964;</it><sub>op</sub>/<it>N</it> and a subradiant mode with lifetime <it>&#964;</it><sub>sbr</sub> &#8811; <it>&#964;</it><sub>op</sub><it>.</it> Thus, the effective radiation rate is given by</p>
            <p>
               <display-formula>
                  <graphic file="1556-276X-5-991-i9.gif"/>
               </display-formula>
            </p>
            <p/>
            <p>Since <it>&#964;</it><sub>sbr</sub> &#8811; <it>&#964;</it><sub>op</sub> &gt;<it>&#964;</it><sub>spr</sub>, only the superradiant modes contribute significantly along with the radiative recombination time to the effective decay time. In our case, this description has to be extended to the cooperative emission of a certain number, <it>&#916;N</it>(<it>E</it>), of optical modes corresponding to QDs emitting light with the same frequency. Then, the optical decay time will be given by</p>
            <p>
               <display-formula>
                  <graphic file="1556-276X-5-991-i10.gif"/>
               </display-formula>
            </p>
            <p/>
            <p>In a simplified description of continuous distribution of optical modes by energy, their density can be considered as a Lorenzian. Thus, the number of modes within a range &#916;<it>E</it> will be</p>
            <p>
               <display-formula>
                  <graphic file="1556-276X-5-991-i11.gif"/>
               </display-formula>
            </p>
            <p>where 2 stands for the double degeneracy of each QD ground state, and <it>n</it><sub><it>T</it></sub> is the total number of dots. The dispersion width of optical modes, <it>&#915;</it><sub>op</sub>, can be calculated by considering a total number of the excited optical modes, <it>N</it><sub><it>T</it></sub>, that depends on the excitation energy, <it>E</it><sub>exc</sub>, through</p>
            <p>
               <display-formula>
                  <graphic file="1556-276X-5-991-i12.gif"/>
               </display-formula>
            </p>
            <p/>
            <p>This yield</p>
            <p>
               <display-formula>
                  <graphic file="1556-276X-5-991-i13.gif"/>
               </display-formula>
            </p>
            <p>where <inline-formula><graphic file="1556-276X-5-991-i38.gif"/></inline-formula></p>
            <p>The important parameter characterizing the collective emission is the decay time at the PL maximum energy, <it>&#964;</it><sub>eff</sub>(<it>E</it><sub>0</sub>). According to Eqs. (10, 11), this parameter is reduced to</p>
            <p>
               <display-formula>
                  <graphic file="1556-276X-5-991-i14.gif"/>
               </display-formula>
            </p>
            <p>It can be immediately compared with the measured data. Taking <it>&#964;</it><sub>op</sub>(<it>E</it>) in the form <it>&#964;</it><sub>op</sub>(<it>E</it>) = <it>C</it><sub>1</sub>/<it>E</it> as in Eq. (8), we fit Eq. (14) to the measured <it>&#964;</it><sub>d</sub>(<it>E</it><sub>0</sub>) with the set of parameters: <it>C</it><sub>1</sub> = 1.3 ns &#215; eV, <it>&#945;</it> = 0.025 eV, and <it>N</it><sub><it>T</it></sub>/<it>n</it><sub><it>T</it></sub> = 1.113. The result of best fit is shown in Fig. <figr fid="F9">9</figr> by solid line together with measured <it>&#964;</it><sub>d</sub>(<it>E</it><sub>0</sub>) (open circles). The quantitative agreement of the <inline-formula><graphic file="1556-276X-5-991-i39.gif"/></inline-formula> growth with the difference <inline-formula><graphic file="1556-276X-5-991-i40.gif"/></inline-formula> increasing between the theory and experiment gives strong support of the cooperative nature of the QD emission near the PL maximum.</p>
            <fig id="F9"><title><p>Figure 9</p></title><caption><p>The measured (open circles) and calculated data from Eq</p></caption><text>
   <p>The measured (<it>open circles</it>) and calculated data from Eq. (14) with the set of parameters: <it>C</it><sub>1</sub> = 1.3 ns &#215; eV, <it>&#945;</it> = 0.025 eV, and <it>N</it><sub><it>T</it></sub>/<it>n</it><sub><it>T</it></sub> = 1.113 (<it>solid line</it>) <inline-formula><graphic file="1556-276X-5-991-i52.gif"/></inline-formula> dependences versus the difference <inline-formula><graphic file="1556-276X-5-991-i53.gif"/></inline-formula></p>
</text><graphic file="1556-276X-5-991-9"/></fig>
            <p>Further evidence of the superradiance effect in our QD system arises from comparison of the <it>&#964;</it><sub>d</sub>(<it>&#955;</it><sub>det</sub>) dependence under excitation both with <it>&#955;</it> close to the PL maximum (quasi-resonant case) and far from the PL maximum (non-resonant case). It has been shown <abbrgrp><abbr bid="B17">17</abbr></abbrgrp> that for the non-resonant condition <it>&#964;</it><sub>d</sub>(<it>&#955;</it><sub>det</sub>) is mainly a result of the optical emission lifetime <it>&#964;</it><sub>op</sub>, whereas for the quasi-resonant condition it equals <it>&#964;</it><sub>eff</sub>. From Fig. <figr fid="F7">7</figr>, the <it>&#964;</it><sub>d</sub>(<it>&#955;</it><sub>det</sub>) dependences can be seen to be different under non-resonant (<it>nr</it>) excitation condition and quasi-resonant (<it>qr</it>) conditions. Figure <figr fid="F10">10a</figr> displays the relative change in decay rate given by taking the ratio of the PL decay times under quasi-resonant excitation (<it>&#955;</it><sub>exc</sub> = 870 nm) and non-resonant (<it>&#955;</it><sub>exc</sub> = 720 nm) excitation. The ratio <it>&#964;</it><sub>870</sub>/<it>&#964;</it><sub>720</sub> reveals the strongest change just in the vicinity of the maximum of the PL spectrum. Such a behavior of the <it>&#964;</it><sub>870</sub>/<it>&#964;</it><sub>720</sub> ratio <abbrgrp><abbr bid="B33">33</abbr></abbrgrp> serves as a fingerprint of the cooperative QD emission. Indeed, the continuous wave PL spectrum represents the distribution of the ground-state energies of excitons in the QD ensemble which is in turn due to the QD size distribution. While the QD density is the highest in the center of the QD size distribution, the radiation field of the QDs is the strongest at a specific exciton ground-state energy corresponding to the maximum of the PL signal. Consequently, a radiative interaction has to be strongest between the QDs belonging to the central part of the QD size distribution, thus the change in radiation rate has to be strongest in the PL spectral maximum. This is what is observed experimentally in our QD sample. It is also shown in Ref. <abbrgrp><abbr bid="B10">10</abbr></abbrgrp> that the change of the radiation rate (<inline-formula><graphic file="1556-276X-5-991-i41.gif"/></inline-formula>) caused by a radiative coupling between QDs has to be properly scaled because it depends linearly on the number of QDs, <it>N(&#955;)</it>, emitting with the wavelength <it>&#955;,</it> and decreases inversely with the distance between QDs, <it>R(&#955;)</it>. This leads to the change in the radiation rate as <it>&#916;</it>(<it>N</it>(<it>&#955;</it>), <it>R</it>(<it>&#955;</it>))&#8733; <it>I</it><sup>3/2</sup>(<it>&#955;</it>). We compared this dependence with the measured change in the PL decay time (Fig. <figr fid="F10">10b</figr>) presented in the form <inline-formula><graphic file="1556-276X-5-991-i42.gif"/></inline-formula> and found a good correlation, which indicates radiative coupling between QDs. We assume that this radiative coupling is dominant for the QDs belonging to different chains, whereas immediate electronic coupling dominates between the in-chain dots.</p>
            <fig id="F10"><title><p>Figure 10</p></title><caption><p>a The ratio &#964;870/&#964;720 (symbols) of the &#964;d(&#955;det) measured under quasi-resonant (&#955;exc = 870 nm) and non-resonant (&#955;exc = 720 nm) excitations</p></caption><text>
   <p><b>a</b> The ratio <it>&#964;</it><sub>870</sub>/<it>&#964;</it><sub>720</sub> (<it>symbols</it>) of the <it>&#964;</it><sub>d</sub>(<it>&#955;</it><sub>det</sub>) measured under quasi-resonant (<it>&#955;</it><sub>exc</sub> = 870 nm) and non-resonant (<it>&#955;</it><sub>exc</sub> = 720 nm) excitations. The strongest change is seen just in the vicinity of the maximum of the normalized PL spectrum (<it>solid line</it>). <b>b</b> Normalized <inline-formula><graphic file="1556-276X-5-991-i54.gif"/></inline-formula> dependence (<it>symbols</it>) and normalized <it>I</it><sup>3/2</sup>(<it>&#955;</it>) spectrum (<it>solid line</it>). Such a behavior of the measured <it>&#964;</it><sub>d</sub>(<it>&#955;</it><sub>det</sub>) under non-resonant and quasi-resonant conditions evidences the cooperative radiative QD coupling</p>
</text><graphic file="1556-276X-5-991-10"/></fig>
            <p>Independently, the superradiance contribution to the radiation rate in our system is revealed from the analysis of the <it>&#964;</it><sub>d</sub>(<it>&#955;</it><sub>det</sub>) dependence measured at the PL band maximum for various excitation intensities. It is expected <abbrgrp><abbr bid="B33">33</abbr></abbrgrp> that the <it>&#964;</it><sub>d</sub>(<it>&#955;</it><sub>det</sub>) value must depend non-monotonicly on <it>I</it><sub>exc</sub>. Indeed, for the case of extremely low excitation intensity only a very small number of QDs are optically excited, and therefore the radiative cooperative effects should be negligible. Under increased excitation density, the superradiance mode becomes more significant, coupling the QDs of the ensemble and leading to a decrease of the <it>&#964;</it><sub>d</sub>(<it>&#955;</it><sub>det</sub>) value. Such a result is shown in Fig. <figr fid="F11">11</figr> for the In<sub>0.4</sub>Ga<sub>0.6</sub>As/GaAs QD chain sample. Here, the dependence of <it>&#964;</it><sub>d</sub> measured at the QD PL maximum on the excitation density is clearly demonstrated for various excitation wavelengths. One can see that at the lowest excitation densities (~10<sup>10</sup> photons/(pulse &#215; cm<sup>2</sup>)) the <it>&#964;</it><sub>d</sub> value is practically invariable due to the absence of interdot radiative coupling. However, let us note that the experimental accuracy of the <it>&#964;</it><sub>d</sub> determination is rather low due to the noisy PL signal in case of lowest excitation densities. As a result, for <it>&#955;</it><sub>exc</sub> = 870 nm and <it>&#955;</it><sub>exc</sub> = 900 nm (see Fig. <figr fid="F11">11</figr>), we cannot reliably investigate the region of the lowest excitation densities. If the excitation intensity is raised the superradiance mode turns on strongly, coupling the QDs within the ensemble. Such a coupling tends to reduce the <it>&#964;</it><sub>d</sub> value, which is seen in Fig. <figr fid="F11">11</figr> for the excitation wavelengths <it>&#955;</it><sub>exc</sub> = 720 nm and <it>&#955;</it><sub>exc</sub> = 810 nm. Further increase in the excitation density leads to a saturation of the QD ground states resulting in a progressive increase in the <it>&#964;</it><sub>d</sub> value. The appearance of a dip in the <it>&#964;</it><sub>d</sub> dependence on the excitation density in the range of very low excitation densities serves as a specific fingerprint of superradiance in our QD samples.</p>
            <fig id="F11"><title><p>Figure 11</p></title><caption><p>The &#964;d dependence measured at the QD PL maximum in In0</p></caption><text>
   <p>The <it>&#964;</it><sub>d</sub> dependence measured at the QD PL maximum in In<sub>0.4</sub>Ga<sub>0.6</sub>As/GaAs QD chain sample versus excitation density for different excitation wavelengths. <it>Vertical bars</it> show experimental accuracy</p>
</text><graphic file="1556-276X-5-991-11"/></fig>
            <p>The appearance of the dip on the <inline-formula><graphic file="1556-276X-5-991-i43.gif"/></inline-formula> dependences for the detection energies lower than <it>E</it><sub>0</sub> (see Fig. <figr fid="F7">7</figr>) can be attributed to the coupling of longitudinal optical phonons with confined electrons and holes in QDs and to the presence of deep levels allowing the holes tunnel to these states even at low temperatures <abbrgrp><abbr bid="B34">34</abbr></abbrgrp>. The states of deep levels are closer to the states of larger QDs. Therefore, the hole tunneling is more effective for larger QDs that form the low energy side of the PL spectrum thus reducing the <inline-formula><graphic file="1556-276X-5-991-i44.gif"/></inline-formula> value observed experimentally in the spectral range below the QD PL maximum.</p>
         </sec>
      </sec>
      <sec>
         <st>
            <p>Conclusions</p>
         </st>
         <p>Finally, peculiar dependences of the PL decay time on the excitation and detection energies are revealed in the multilayer In<sub>0.4</sub>Ga<sub>0.6</sub>As/GaAs QD chain sample and ascribed to the peculiarities of the carrier and energy relaxation caused by both immediate electronic interdot coupling and long-range coupling through the radiation field. Summarizing, we have established: i) appearance of low temperature asymmetry of the PL band caused by the non-thermal carrier distribution through in-chain interdot wave function coupling. The energy scheme of the In<sub>0.4</sub>Ga<sub>0.6</sub>As/GaAs QD chain sample is specified and 1D WL, 2D InGaAs WL, and the heavy hole excited states are identified from the temperature cw PL measurements: ii) the in-chain interdot carrier transfer forms the swing of the decay time <it>&#964;</it><sub>d</sub> versus detection energy dependence and can lead to the state saturation effect shifting the maximal <it>&#964;</it><sub>d</sub> value close to QD PL maximum; iii) superradiant mode of the emission field couples the QDs of different dot chains and leads to a significant change of the decay time value just in the vicinity of the QD PL maximum. This radiant interdot coupling defines the dependence of the <it>&#964;</it><sub>d</sub> value on the excitation wavelength. Coexistence of various mechanisms of interdot coupling is determined here by special design of the QD samples providing effective interdot in-chain electronic coupling and effective radiative interchain coupling due to superradiance. This latter type of coupling could play a significant role in ultrafast applications.</p>
      </sec>
      <sec>
         <st>
            <p>Misc</p>
         </st>
         <p>E. Marega Jr: On leave from Departamento de F&#237;sica e Ci&#234;ncia dos Materiais, Instituto de F&#237;sica de S&#227;o Carlos-USP S&#227;o Carlos SP 13560-970, Brazil.</p>
      </sec>
   </bdy>
   <bm>
      <ack>
         <sec>
            <st>
               <p>Acknowledgments</p>
            </st>
            <p>The authors acknowledge the financial support of the National Science Foundation of the U.S. through Grant # DMR-0520550.</p>
            <sec>
               <st>
                  <p>Open Access</p>
               </st>
               <p>This article is distributed under the terms of the Creative Commons Attribution Noncommercial License which permits any noncommercial use, distribution, and reproduction in any medium, provided the original author(s) and source are credited.</p>
            </sec>
         </sec>
      </ack>
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