• Title/Summary/Keyword: Red shift

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The Physicochemical Properties on the Organic, Charge Transfer Complexes under High Pressure (고압하의 전하이동착물에 대한 물성론적 연구. 사염화탄소 용액내에서의 헥사메틸벤젠과 1,3,5-트리니트로벤젠과의 전하이동착물 생성에 대한 압력과 온도의 영향)

  • Oh Cheun Kwun;Myong Ja Kim
    • Journal of the Korean Chemical Society
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    • v.32 no.6
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    • pp.513-519
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    • 1988
  • The effect of pressure and temperature on the stabilities of hexamethylbenzene-1,3,5-trinitrobenzene charge transfer complex in carbon tetrachloride has been investigated by spectrophotometric measurements. The absorption spectra of charge transfer complexes were measured at 25, 40, $50^{\circ}C$ under 1, 200, 500, 1000, 1400 bar in this experiments. The equilibrium constants of the complex were increased with pressure and decreased with temperature rising. The absorption coefficients were increased with pressure and temperature. Change of volume, enthalpy, free energy and entropy for the formation of complexes were calculated from the equilibrium constants. The red-shift observed at a higher pressure, the blue-shift at a higher temperature and the relation between pressure and oscillator strength were discussed by means of thermodynamic fuctions.

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The Effect of Pressure and Temperature on the Benzene-Iodine Charge Transfer Complex in n-Hexane (벤젠과 요오드 사이의 전하이동착물에 대한 압력과 온도의 영향)

  • Oh Cheun Kwun;Jeong Rim Kim
    • Journal of the Korean Chemical Society
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    • v.27 no.2
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    • pp.102-110
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    • 1983
  • The effect of pressure and temperature on the stabilities of the benzene-iodine charge transfer complex have been investigated through ultraviolet spectrophotometric measurements in n-hexane. The stabilities of the complexes were measured at temperatures of 25, 40 and $60^{\circ}C$ up to 1600 bars. The equilibrium constant of the complex formation was increased with pressure and decreased with temperature raising. The absorption coefficient was increased with both pressure and temperature. Changes of volume, enthalpy, free energy and entropy for the formation of complexes were obtained from the equilibrium constants. The red-shift at a higher pressure, the blue-shift at a higher temperature and the relation between pressure and oscillator strength were discussed by means of thermodynamic functions.

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The Effect of Pressure and Temperature on the Xylene-Iodine Charge Transfer Complex in n-Hexane (크실렌과 요오드 사이의 전하이동 착물에 대한 압력과 온도의 영향)

  • Oh Cheun Kwon
    • Journal of the Korean Chemical Society
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    • v.22 no.4
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    • pp.245-253
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    • 1978
  • The effect of pressures and temperatures on the stabilities of the p-xylene-iodine charge transfer complex have been investigated through ultraviolet spectrophotometric measurements in n-hexane. The stabilities of complexes were measured at 25, 40 and $60^{\circ}C$ under 1∼1,600 bars. The equilibrium constant of the complex was increased with pressure and decreased with temperature raising. The absorption coefficient was increased with both pressure and temperature. Changes of volume, enthalpy, free energy and entropy for the formation of complexes were obtained from the equilibrium constants. The red-shift observed a higher pressure, the blue-shift at a higher temperature and the relation between pressure and oscillator strength were discussed by means of thermodynamic functions.

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Insight into Rhodopsin Diversity from Viewpoint of Counterion

  • Terakita, Akihisa
    • Journal of Photoscience
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    • v.9 no.2
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    • pp.33-36
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    • 2002
  • In vertebrate rhodopsins the glutamic acid at position 113 serves as a counterion to stabilize the protonated retinylidene Schiff base linkage and to shift the spectrum to the visible region. Invertebrate rhodopsins and retinochrome have the amino acid residue different from glutamic acid or asparatic acid at this position and therefore, these pigments may have a counterion at different position. We first investigated the counterion in retinochrome by site specific mutagenesis. The results showed that the counterion is the glutamic acid at position 181, where almost of all the pigments including vertebrate and invertebrate rhodopsins in the rhodopsin family have a glutamic acid or an aspartic acid. In vertebrate rhodopsins, however, Glu 181 does not act as a counterion, and the red-sensitive cone pigments have a histidine at this position, which serves as a chloride-binding site for red-shift of the absorption spectrum. These findings suggested that the role of Glu181 as a counterion may be weakened by the newly acquired counterion at position 113. Taken together with our recent studies on an invertebrate-type rhodopsin, the rhodopsin diversity was discussed from viewpoint of counterion.

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Solvent effect on the excited state of stilbene dendrimers bearing phenylacetylene groups

  • Nishimura, Yoshinobu;Arai, Tatsuo
    • Rapid Communication in Photoscience
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    • v.3 no.4
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    • pp.85-87
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    • 2014
  • We studied the characteristics of emissive state of the first (p-G1) and second (p-G2) generation of phenylacetylene dendrimers bearing stilbene as a core by using time-resolved fluorescence spectroscopy in cyclohexane (c-Hex) and N, N-dimethylformide (DMF), which are nonpolar and polar solvents, respectively. Time-dependent red-shift of emission spectra p-G2 both in c-Hex and DMF was observed in comparison with p-G1. Besides, the time constant of red-shift of spectra was found to be larger in DMF than in c-Hex. This indicates that the emissive state of p-G2 has a polar character in DMF as a result of charge delocalization from core to peripheral dendrons followed by stabilization of emissive state.

UV VISIBILITY OF MODERATE-REDSHIFT GIANT ELLIPTICAL GALAXIES

  • Rhee, Myung-Hyun;Lee, Young-Wook;Byun, Yong-Ik;Sohn, Young-Jong
    • Journal of Astronomy and Space Sciences
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    • v.15 no.1
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    • pp.49-52
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    • 1998
  • We show quantitatively whether giant elliptical galaxies would be visible at for UV wavelenghts if they were placed at moderate red shift of 0.4-0.5. On the basis of simple cosmological tests, we conclude that giant elliptical galaxies can be detectable up to the red shift of 0.4-0.5 in the proposed GALEX(Galaxy Evolution Explorer) Deep Imaging Survey. We also show that obtaining UV color index such as $m_{1550}$ - V from upcoming GALEX and SDSS (Sloan Digital Sky Survey) observations should be feasible.

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Optical Excitation and Emission Spectra of YNbO4 : Eu3+

  • Lee, Eun-Young;Kim, Young-Jin
    • Journal of the Korean Electrochemical Society
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    • v.12 no.3
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    • pp.234-238
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    • 2009
  • In the excitation spectra of $YNbO_4$ : $Eu^{3+}$, the charge transfer (CT) band around 270 nm due to $[NbO_4]^{3-}$$-Eu^{3+}$ interaction and sharp excitation peaks by f-f transition of $Eu^{3+}$ strongly appeared simultaneously. CT band depended on the structural properties of powders, showing the red-shift with increasing the crystallinity, while the f-f transition peaks were independent of the crystallinity. For $YNb_{1-x}Ta_xO_4$ : $Eu^{3+}$ (x = 0.05.0.2), $[TaO_4]^{3-}$. configuration was locally constructed, leading to the blue-shift in CT band and the decrease in the red emission intensity with increasing the Ta content.

Tuning Photoluminescence of Biological Light Emitters via Silk Protein Based Resonators

  • Arif, Sara;Umar, Muhammad;Kim, Sunghwan
    • Current Optics and Photonics
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    • v.3 no.1
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    • pp.40-45
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    • 2019
  • Adding tunability to biological light emitters offers an unprecedented technique in biological sensing and imaging. Here, we report a tunable, lithographic-free, planar, and ultrathin metal-insulator-metal (MIM) resonator capable of tuning the optical properties solely by a silk/sodium fluorescein hydrogel layer, a biocompatible light emitter. In water, the volume of the resonator was expanded by swelling, and then the resonant mode could be shifted. Simulations predicted the red-shifted resonance peak in transmission when the MIM was swollen in water. The red-shift could be attributed to the increase in the thickness of the silk hydrogel layer due to the absorbed water. The shift of the resonance could affect the fluorescence of the dye in the silk hydrogel layer.

Enhancement of Thermal Stability in Photoluminescence by Carbonization of Porous silicon (다공성실리콘의 탄화를 이용한 PL의 열적안정성 증진)

  • 최두진;서영제;전희준;박홍이;이덕희
    • Journal of the Korean Ceramic Society
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    • v.34 no.5
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    • pp.467-472
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    • 1997
  • Porous silicon was prepared by an anodic etching. The pore size was about 10 nm at an etching time of 20 sec and a current density of 20 mA/$\textrm{cm}^2$. The porous layer was composed of an micro-porous layer (0.6 ${\mu}{\textrm}{m}$) and a macro-porous layer (10 ${\mu}{\textrm}{m}$). Room temperature PL with maximum peak 6700$\AA$ appeared. The peak disappeared by an oxidation reaction when the porous silicon was heated to 100~20$0^{\circ}C$ in atmosphere. In order to avoid the oxidation a heat treatment was done in H2 atmosphere. The micro-pore and Si column, which formed quantum well, were collapsed by the high temperature. The PL maximum peak of heated sample was gradually red-shifted and showed about 300$\AA$ red-shift at 50$0^{\circ}C$. The intensity of PL was maintained to high temperatures in lower pressures. The porous Si was carbonized in C2H2+H2 gas in order to increase thermal stability. The carbonization of the porous Si prevented red-shift of the maximum PL peak caused by sintering effect at high temperatures, and the carbonized porous Si showed Pl signal at higher temperatures by above 20$0^{\circ}C$ than the sample in H2 atmosphere.

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On the study of two luminescence band structfue from ambient air aged porous silicon (대기중에서 aged된 다공성 실리콘의 2가지 발광 band에 관한 연구)

  • Sung-Sik Chang;Akira Sakai
    • Journal of the Korean Crystal Growth and Crystal Technology
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    • v.6 no.4
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    • pp.564-570
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    • 1996
  • We have observed the red and blue luminescence from porous silicon (PS) without any rapid thermal oxidation. Aged porous silicon specimens prepared in dilute HF concentration, especially for the short duration of etching, display the increase of the blue band. The measured luminescence decay time at room temperature exhibits a decay time of about 100 ps and shows appreciably faster decay time than that of 20 K. No photoluminescence (PL) peak maximum shift is observed for the blue PL band at 77 K. However, the red PL band shows the blue shift and displays yellow luminescence at 77 K. The origin of red luminescence has some properties related to Si crystallites, whereas blue luminescence seems to be associated other than Si crystallites.

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