Localized excitons in cubic Zn1-xCdxS lattice matched to GaAs

Excitonic properties have been studied in cubic Zn0.42Cd0.58S lattice matched to GaAs. At 2 K, the time-integrated photoluminescence spectrum was composed of single emission peaking at 2.863 eV and its LO-phonon replica. The linewidth of the main peak was 18.5 meV, which fairly well agreed with the theoretical value based on the disorder-induced broadening of exciton luminescence in alloys. In order to assess the emission mechanism, the transient luminescence decay was measured at various emission energies. At the high energy tail (2.883 eV), the luminescence showed exponential decay with a time constant of about 72 ps. On the other hand, the decay time increased with decreasing the detected emission energy. It was about 660 ps at the emission peak (2.863 eV). We interpret these features by means of the model of exciton localization

Low-Waterway Variation Due to Change of Water and Sediment Supply Conditions

Source: ICHE Conference Archive - https://mdi-de.baw.de/icheArchiv

Attribute Assignment to Point Cloud Data and Its Usage

In recent years, with the development of laser measurement technology, utilization of point cloud data is progressing. However, since point cloud data does not contain attribute information, the usability of the data is low. It is possible to consider that by assigning attributes to the nonattribute point cloud data, this can lead to the usage of point cloud data in each phase of life cycle of construction: design, construction, and maintenance. Therefore, in this paper, the authors have proposed an attribute assignment method for point cloud data. In addition, the authors proposed the way to use attributed point cloud data, the usage as objects, data linkage, and visualization by using the attribute assignment method. Point cloud data of a dam was used as a case study for the proposed method and the usage

Time-resolved spectroscopy of biexciton luminescence in ZnxCd1-xSe-ZnSySe1-y multiple quantum wells

The radiative lifetime of biexcitons in ZnxCd1-xSe-ZnSySe1-y multiple quantum wells has been studied by means of time-resolved luminescence spectroscopy under high-density excitation. It is shown that the rise of the biexciton luminescence becomes more rapid with increasing excitation energy density and that the biexciton luminescence decays with a double exponential form. It is found that the decay-time constant of the faster-decay component in the double-exponential decay corresponds to the radiative lifetime of the biexciton. Its value is about 6 ps at 2 K and is about one-seventh of that in bulk ZnSe (∼40 ps)

Experimental Study on Flow and Bank Erosion in Steep and Curved Trapezoidal Channels

Source: ICHE Conference Archive - https://mdi-de.baw.de/icheArchiv

Confocal microphotoluminescence of InGaN-based light-emitting diodes

Spatially resolved photoluminescence (PL) of InGaN/GaN/AlGaN-based quantum-well-structured light-emitting diodes (LEDs) with a yellow-green light (530 nm) and an amber light (600 nm) was measured by using confocal microscopy. Submicron-scale spatial inhomogeneities of both PL intensities and spectra were found in confocal micro-PL images. We also found clear correlations between PL intensities and peak wavelength for both LEDs. Such correlations for yellow-green and amber LEDs were different from the reported correlations for blue or green LEDs. This discrepancy should be due to different diffusion, localization, and recombination dynamics of electron-hole pairs generated in InGaN active layers, and should be a very important property for influencing the optical properties of LEDs. In order to explain the results, we proposed a possible carrier dynamics model based on the carrier localization and partial reduction of the quantum confinement Stark effect depending on an indium composition in InGaN active layers. By using this model, we also considered the origin of the reduction of the emission efficiencies with a longer emission wavelength of InGaN LEDs with high indium composition

Pair-density wave signature observed by x-ray scattering in La-based high-TcT_{\rm c} cuprates

Suggestive, but indirect evidence of the existence of pair-density wave (PDW) order in several high-$T_{\rm c}$ cuprates has been reported. As this constitutes a new quantum phase of matter, it is important to {\it establish} its existence at least somewhere in the phase diagram. However, a direct correspondence between experiment and theory has remained elusive. Here, we report the observation of a theoretically predicted PDW {\it bulk} signature in two La-based cuprates, Sr-doped La$_{1.875}$Ba$_{0.125}$CuO$_4$ and Fe-doped La$_{1.87}$Sr$_{0.13}$CuO$_4$, through a comprehensive study that incorporates zero-magnetic field x-ray scattering, neutron scattering, and transport measurements. Specifically, we observe the emergence of so-called "1Q" order, which is to say subharmonic order associated with the charge-density wave (CDW) stripes, in a range of temperatures in which independent evidence suggests the co-existence of PDW long-range order and fluctuating uniform superconducting order. The subharmonic order is most pronounced around a half-integer $l$-vector, where the CDW diffraction peak is also strongest. This is consistent with the theoretical proposal that the cancellation of the Josephson coupling ("layer-decoupling"), is a signature of PDW order and that it is commensurately locked to the density wave stripes that are known to alternate orientation between adjacent layers. Even if the PDW is not the "mother of all state", it is at least a close relative -- possibly a second cousin

Interferometric Observations of the T Tauri Stars in the MBM 12 Cloud

We have carried out a millimeter interferometric continuum survey toward 7 YSOs in the MBM 12 cloud. Thermal emissions associated with 2 YSOs were detected above the 3-$\sigma$ level at 2.1 mm, and one also showed a 1.3 mm thermal emission. Another object was marginally detected at 2.1 mm. Spectral energy distributions of the YSOs are well fitted by a simple power-law disk model. Masses of the circumstellar disks are estimated to be an order of 0.05 M_{\sun}. The circumstellar disks in the MBM 12 cloud have properties in common with the disks in nearby star-forming regions, in terms of disk parameters such as a disk mass, as well as an infrared excess.Comment: 9 pages, 3 figures, accepted by ApJ Letter