在压力测试时,高分辨率TFT-LCD(Thin Film Transistor-Liquid Crystal Display)液晶面板会发生"斑点不良"。为了预防该不良的发生,本文分析了"斑点不良"的发生机理:压力测试时,隔垫物PS(Photo Spacer)发生滑动,将...在压力测试时,高分辨率TFT-LCD(Thin Film Transistor-Liquid Crystal Display)液晶面板会发生"斑点不良"。为了预防该不良的发生,本文分析了"斑点不良"的发生机理:压力测试时,隔垫物PS(Photo Spacer)发生滑动,将阵列基板上透光区域的配向膜-聚酰亚胺PI(Polyimide)划伤,而失去配向液晶能力,在暗态画面下,划痕处会发生漏光,形成斑点状。本文对不同尺寸及分辨率的液晶面板进行了压力测试,比较隔垫物挡墙、黑矩阵BM(Black Martrix)、隔垫物站位等不同因素对"斑点不良"的影响:隔垫物挡墙能有效阻挡隔垫物的滑动距离的23.6%,能有效降低"斑点不良"的漏光发生;当隔垫物滑动的距离未超出黑矩阵的遮挡范围时,不可见"斑点不良"或很轻微;站在金属块(Pillow)上的隔垫物比没有站在Pillow上的隔垫物滑动距离小约10%。最后以49in超高清UHD(Ultra High Definition)液晶面板为例,提出一种改善"斑点不良"的的设计方案:增加PS上下挡墙设计,降低PS滑动距离;增加BM宽度设计,保证PS边缘到BM边缘的距离大于PS滑动距离;降低PS的个数,增加PS的大小设计降低透过率损失。该方案客户验证无"斑点不良"发生且透过率下降1.2%,说明此设计方案能够有效地改善"斑点不良"。展开更多
Recently,a parametrized Schwarzschild metric(PSM)was proposed,in which n=2 to solve the differences of mass of M87*from different observations.We find the axial gravitational quasinormal modes of this metric are unsta...Recently,a parametrized Schwarzschild metric(PSM)was proposed,in which n=2 to solve the differences of mass of M87*from different observations.We find the axial gravitational quasinormal modes of this metric are unstable for n>1.The decay rate of the quasinormal mode of the case n<1 is much smaller than the case n=1,which can be used to differentiate the PSM from a Schwarzschild one.展开更多
Phononic crystals(PCs) have recently been developed as effective components for vibration suppression and sound absorption. As a typical design of PCs, wave attenuation occurs in the so-called stop-band. However, the ...Phononic crystals(PCs) have recently been developed as effective components for vibration suppression and sound absorption. As a typical design of PCs, wave attenuation occurs in the so-called stop-band. However, the structural response is still significantly large in the pass-band. In this paper, we combine PCs and acoustic black holes(ABHs) in a unique device, achieving a versatile device that can attenuate vibration in the stop-band, while suppress vibration in the pass-band. This approach provides a versatile platform for controlling vibration in a multiband with a simple design.展开更多
We provide a comprehensive survey of possible applications of the matrix method for black hole quasinormal modes. The proposed algorithm can generally be applied to various background metrics, and in particular, it ac...We provide a comprehensive survey of possible applications of the matrix method for black hole quasinormal modes. The proposed algorithm can generally be applied to various background metrics, and in particular, it accommodates both analytic and numerical forms of the tortoise coordinates, as well as black hole spacetimes. We give a detailed account of different types of black hole metrics, master equations, and the corresponding boundary conditions. Besides, we argue that the method can readily be applied to cases where the master equation is a system of coupled equations. By adjusting the number of interpolation points, the present method provides a desirable degree of precision, in reasonable balance with its efficiency. The method is flexible and can easily be adopted to various distinct physical scenarios.展开更多
We utilize the topological-geometrical structure imposed by the Heterotic superstring theory on spacetime in conjunction with the K3 Kähler manifold to explain the mysterious nature of dark matter and its cou...We utilize the topological-geometrical structure imposed by the Heterotic superstring theory on spacetime in conjunction with the K3 Kähler manifold to explain the mysterious nature of dark matter and its coupling to the pure dark energy density of the cosmos. The analogous situations in the case of a Kerr black hole as well as the redundant components of the Riemannian tensor are pointed out and the final result was found to be in complete agreement with all previous theoretical ones as well as all recent accurate measurements and cosmic observations. We conclude by commenting briefly on the Cantorian model of Zitterbewegung and the connection between Olbers’s paradox and dark energy.展开更多
文摘在压力测试时,高分辨率TFT-LCD(Thin Film Transistor-Liquid Crystal Display)液晶面板会发生"斑点不良"。为了预防该不良的发生,本文分析了"斑点不良"的发生机理:压力测试时,隔垫物PS(Photo Spacer)发生滑动,将阵列基板上透光区域的配向膜-聚酰亚胺PI(Polyimide)划伤,而失去配向液晶能力,在暗态画面下,划痕处会发生漏光,形成斑点状。本文对不同尺寸及分辨率的液晶面板进行了压力测试,比较隔垫物挡墙、黑矩阵BM(Black Martrix)、隔垫物站位等不同因素对"斑点不良"的影响:隔垫物挡墙能有效阻挡隔垫物的滑动距离的23.6%,能有效降低"斑点不良"的漏光发生;当隔垫物滑动的距离未超出黑矩阵的遮挡范围时,不可见"斑点不良"或很轻微;站在金属块(Pillow)上的隔垫物比没有站在Pillow上的隔垫物滑动距离小约10%。最后以49in超高清UHD(Ultra High Definition)液晶面板为例,提出一种改善"斑点不良"的的设计方案:增加PS上下挡墙设计,降低PS滑动距离;增加BM宽度设计,保证PS边缘到BM边缘的距离大于PS滑动距离;降低PS的个数,增加PS的大小设计降低透过率损失。该方案客户验证无"斑点不良"发生且透过率下降1.2%,说明此设计方案能够有效地改善"斑点不良"。
基金National Natural Science Foundation of China(NNSFC)under contract No.423007the Fundamental Research Funds for the Central Universities,China University of Geosciences(Wuhan)with No.G1323523064supported by the National Natural Science Foundation of China(NNSFC)under contract Nos.127506 and 123519。
文摘Recently,a parametrized Schwarzschild metric(PSM)was proposed,in which n=2 to solve the differences of mass of M87*from different observations.We find the axial gravitational quasinormal modes of this metric are unstable for n>1.The decay rate of the quasinormal mode of the case n<1 is much smaller than the case n=1,which can be used to differentiate the PSM from a Schwarzschild one.
基金Project supported by the National Natural Science Foundation of China(Nos.51575378,11972245,and 11672187)。
文摘Phononic crystals(PCs) have recently been developed as effective components for vibration suppression and sound absorption. As a typical design of PCs, wave attenuation occurs in the so-called stop-band. However, the structural response is still significantly large in the pass-band. In this paper, we combine PCs and acoustic black holes(ABHs) in a unique device, achieving a versatile device that can attenuate vibration in the stop-band, while suppress vibration in the pass-band. This approach provides a versatile platform for controlling vibration in a multiband with a simple design.
基金Support by NNSFC(11805166)Brazilian funding agencies Fundacao de Amparo a Pesquisa do Estado de Sao Paulo(FAPESP)+1 种基金Conselho Nacional de Desenvolvimento Científico e Tecnológico(CNPq)Coordenacao de Aperfeicoamento de Pessoal de Nível Superior(CAPES)
文摘We provide a comprehensive survey of possible applications of the matrix method for black hole quasinormal modes. The proposed algorithm can generally be applied to various background metrics, and in particular, it accommodates both analytic and numerical forms of the tortoise coordinates, as well as black hole spacetimes. We give a detailed account of different types of black hole metrics, master equations, and the corresponding boundary conditions. Besides, we argue that the method can readily be applied to cases where the master equation is a system of coupled equations. By adjusting the number of interpolation points, the present method provides a desirable degree of precision, in reasonable balance with its efficiency. The method is flexible and can easily be adopted to various distinct physical scenarios.
文摘We utilize the topological-geometrical structure imposed by the Heterotic superstring theory on spacetime in conjunction with the K3 Kähler manifold to explain the mysterious nature of dark matter and its coupling to the pure dark energy density of the cosmos. The analogous situations in the case of a Kerr black hole as well as the redundant components of the Riemannian tensor are pointed out and the final result was found to be in complete agreement with all previous theoretical ones as well as all recent accurate measurements and cosmic observations. We conclude by commenting briefly on the Cantorian model of Zitterbewegung and the connection between Olbers’s paradox and dark energy.
