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解变系数偏微分方程的任意差分精细积分法 总被引:2,自引:0,他引:2
本文提出用任意差分精细积分法来求解变系数偏微分方程,它既保留了差分法的优点,又具备有限元法易于处理各种边界条件的特点,同时还是高精度是式差分格式。了后,用一算例来验证了本文方法的正确性和精确性。 相似文献
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The China Spallation Neutron Source/Rapid Cycling Synchrotron (CSNS/RCS) accelerates a high-intensity proton beam from 80 MeV to 1.6 GeV. Since the beam current and beam power is high, the beam loading is a severe problem for the stability of the circulating beam in the RCS. To study the beam loading effect in the CSNS/RCS theoretically, the RLC circuit model of the rf cavity, the method of Fast Fourier Transform and the method of Laplace transform have been employed to obtain the impedance of the rf system, the beam spectrum and the beam-induced voltage, respectively. Based on these physical models, the beam dynamics equations have been revised and a beam loading model has been constructed in the simulation code ORIENT. By using the code, the beam loading effect on the rf system of the CSNS/RCS has been investigated. Some simulation results have been obtained and conclusions have been drawn. 相似文献
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Both longitudinal and transverse coupling impedance for some critical components need to be measured for accelerator design. The twin wires method is widely used to measure longitudinal and transverse impedance on the bench. A mode error is induced when the twin wires method is used with a two-port network analyzer. Here, the mode error is analyzed theoretically and an example analysis is given. Moreover, the mode error in the measurement is a few percent when a hybrid with no less than 25 dB isolation and a splitter with no less than 20 dB magnitude error are used. 相似文献
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The state of super-dense matter is essential for us to understand the nature of pulsars; however, non- perturbative quantum chromodynamics makes it very difficult to make direct calculations of the state of cold matter at realistic baryon number densities inside compact stars. Nevertheless, from an observational point of view, it is conjectured that pulsars could be made up of quark clusters since the strong coupling between quarks might render the quarks to be grouped in clusters. In this paper, we attempt to find an equation of state of condensed quark-cluster matter in a phenomenological way. Supposing that the quark-clusters could be analogized to inert gases, we apply here the corresponding-state approach to derive the equation of state of quark-cluster matter, as was similarly demonstrated for nuclear and neutron-star matter in the 1970s. According to the calculations that we have presented, the quark-cluster stars, which are composed of quark-cluster matter, could have a high maximum mass that is consistent with observations and, in turn, further observations of pulsar mass could also place a constraint on the properties of quark-cluster matter. We will also briefly discuss the melting heat during the solid-liquid phase conversion and its related astrophysical consequences. 相似文献
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为了使气浮支承的承载力动态可调,设计了一种可变节流高度气浮支承. 通过建立气浮支承计算流体动力学(Computational Fluid Dynamics,CFD)模型,利用CFD动网格技术来模拟小孔节流器的运动,研究小孔节流器的结构参数、运动参数及气浮支承的工作参数对可变节流高度气浮支承动态性能的影响. 结果表明:通过调节小孔节流器的节流高度可以明显改变气浮支承的承载力;在只考虑单一变量的前提下,气浮支承承载力的波动量随着小孔节流器的运动幅值、运动频率、节流高度、直径和气浮支承供气压强的增加而增加,但随着气膜厚度的增大而减小;当小孔节流器直径较小时,随着小孔节流器运动频率的增加,气浮支承动刚度的增幅很小,但当小孔节流器直径增大时,随着小孔节流器运动频率的增加,气浮支承动刚度的增幅会明显变大. 相似文献
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