• 제목/요약/키워드: Ge-hong

검색결과 372건 처리시간 0.026초

AsGeSeS/Ag 박막에서 Ag의 두께에 따른 홀로그래픽 회절 효율 특성 (The characteristics of holographic diffraction efficiency depend on thickness of Ag in AsGeSeS/Ag thin film)

  • 이정태;이기남;여철호;이영종;정흉배
    • 한국전기전자재료학회:학술대회논문집
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    • 한국전기전자재료학회 2003년도 추계학술대회 논문집 Vol.16
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    • pp.490-493
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    • 2003
  • We have carried out two-beam interference experiment to form holographic grating on amorphous $As_{40}Ge_{10}Se_{15}S_{35}/Ag$ double-layer. In this study holographic grating formed using He-Ne laser(632.8nm) under non-polarization state and p-polarization state and we confirm that the diffraction efficiency depend on thickness of Ag. The diffraction efficiency was obtained by first order intensity. We got the maximum diffraction efficiency that thickness of Ag was $600{\AA}$. The maximum diffraction efficiency was 13.5% in (P:P) polarization state.

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PRAM용 GST계 박막의 조성에 따른 특성 (Properties of GST Thin Films for PRAM with Composition)

  • 정명훈;장낙원;김홍승;류상욱;이남열;윤성민;박영삼;이승윤;유병곤
    • 한국전기전자재료학회:학술대회논문집
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    • 한국전기전자재료학회 2005년도 하계학술대회 논문집 Vol.6
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    • pp.203-204
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    • 2005
  • PRAM (Phase change Random Access Memory) is one of the most promising candidates for next generation Non-volatile Memories. The Phase change material has been researched in the field of optical data storage media. Among the phase change materials $Ge_2Sb_2Te_5$(GST) is very well known for its high optical contrast in the state of amorphous and crystalline. However, the characteristics required in solid state memory are quite different from optical ones. In this study, the structural properties of GST thin films with composition were investigated for PRAM. The 100-nm thick GeTe and $Sb_2Te_3$ films were deposited on $SiO_2$/Si substrates by RF sputtering system. In order to characterize the crystal structure and morphology of these films, we performed x-ray diffraction (XRD) and atomic force microscopy (AFM).

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비정질 칼코게나이드 박막의 열처리에 따른 회절효율 변화 (The changed diffraction efficiency depend on annealing of amorphous chalcogenide films)

  • 이기남;여철호;신경;정홍배
    • 한국전기전자재료학회:학술대회논문집
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    • 한국전기전자재료학회 2004년도 추계학술대회 논문집 Vol.17
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    • pp.590-593
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    • 2004
  • 본 논문에서는 $As_{40}Ge_{10}Se_{15}S_{35}$ (300nm)박막과 $As_{40}Ge_{10}Se_{15}S_{35}$ (300nm)/Ag(20nm)박막에 홀로그래피 격자를 형성시킨 후 Tg 온도$(240^{\circ}C)$를 기준으로 하여 유리질 천이온도(Tg) 온도 이하 $(190^{\circ}C)$와 이상$(270^{\circ}C)$에서 열처리 시킨 후의 회절효율 변화를 알아보았다. $As_{40}Ge_{10}Se_{15}S_{35}$ (300nm) 박막의 경우 $190^{\circ}C$ : 50%, $240^{\circ}C$ : 약80%, $270^{\circ}C$ : 약 98%의 회절효율 감소가 일어났으며 $As_{40}Ge_{10}Se_{15}S_{35}$(300nm)/Ag(20nm)박막에서는 Tg 온도 이하 즉 $190^{\circ}C$, $240^{\circ}C$ 에서는 회절효율의 변화가 없었으나 Tg온도 이상인 $270^{\circ}C$에서는 약 1.5배 증가한 회절효율을 나타내었다.

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Hole 구조 상변화 메모리의 전기 및 열 특성 (Electro-Thermal Characteristics of Hole-type Phase Change Memory)

  • 최홍규;장낙원;김홍승;이성환;이동영
    • Journal of Advanced Marine Engineering and Technology
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    • 제33권1호
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    • pp.131-137
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    • 2009
  • In this paper, we have manufactured hole type PRAM unit cell using phase change material $Ge_2Sb_2Te_5$. The phase change material $Ge_2Sb_2Te_5$ was deposited on hole of 500 nm size using sputtering method. Reset current of PRAM unit cell was confirmed by measuring R-V characteristic curve. Reset current of manufactured hole type PRAM unit cell is 15 mA, 100 ns. And electro and thermal characteristics of hole type PRAM unit cell were analyzed by 3-D finite element analysis. From simulation temperature of PRAM unit cell was $705^{\circ}C$.

Theoretical Study of Gamma-ray Pulsars

  • Song, Yuzhe;Cheng, Kwong Sang;Takata, Jumpei
    • Journal of Astronomy and Space Sciences
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    • 제33권2호
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    • pp.69-73
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    • 2016
  • We use the non-stationary three dimensional two-layer outer gap model to explain gamma-ray emissions from a pulsar magnetosphere. We found out that for some pulsars like the Geminga pulsar, it was hard to explain emissions above a level of around 1 GeV. We then developed the model into a non-stationary model. In this model we assigned a power-law distribution to one or more of the spectral parameters proposed in the previous model and calculated the weighted phase-averaged spectrum. Though this model is suitable for some pulsars, it still cannot explain the high energy emission of the Geminga pulsar. An Inverse-Compton Scattering component between the primary particles and the radio photons in the outer magnetosphere was introduced into the model, and this component produced a sufficient number of GeV photons in the spectrum of the Geminga pulsar.

두께에 따른 비정질 칼코게나이드 $Ag/As_{40}Ge_{10}Se_{15}S_{35}$ 박막의 홀로그래피 데이터 격자형성 (The Formation of Holographic Data Grating on Amorphous Chalcogenide $Ag/As_{40}Ge_{10}Se_{15}S_{35}$ Thin Films with Various Thickness)

  • 여철호;정홍배
    • 대한전기학회논문지:전기물성ㆍ응용부문C
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    • 제55권8호
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    • pp.387-391
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    • 2006
  • The Ag photodoping effect in amorphous $As_{40}Ge_{10}Se_{15}S_{35}$ chalcogenide thin films for holographic recording has been investigated using a He-Ne laser (${\lambda}$=632.8 nm). The chalcogenide films thickness prepared in the present work were thinner in comparison with the penetration depth of recording light ($d_p=1.66{\mu}m$). It exhibits a tendency of the variation of the diffraction efficiency (${\eta}$) in amorphous chalcogende films, independently of the Ag photodoping. That is, ${\eta}$ increases rapidly at the beginning of the recording process and reaches the maximum (${\eta}_{max}$) and slowly decreases slowly with the exposed time. In addition, the value of ${\eta}_{max}$ depends strongly on chalcogenide film thickness(d) and its maximum peak among the films with d = 40, 80, 150, 300, and 633 nm is observed 0.083% at d = 150 nm (approximately 1/2 ${\Delta}n$), where ${\Delta}$n is the refractive index of chalcogenide thin film (${\Delta}n=2.0$). The ${\eta}$ is largely enhanced by Ag photodoping into the chakogenides. In particular, the value of ${\eta}_{max}$ in a bilayer of 10-nm-thick Ag/150-nm-thick $As_{40}Ge_{10}Se_{15}S_{35}$ film is about 1.6%, which corresponds to ${\sim}20$ times larger than that of the single-layer $As_{40}Ge_{10}Se_{15}S_{35}$ thin film (without Ag). And we obtained the diffraction pattern according to the formation of (P:P) polarization holographic grating using Mask pattern and SLM.