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大型光学望远镜副镜位姿精调机构的优化设计 被引量:13
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作者 徐刚 杨世模 龚雨兵 《光学精密工程》 EI CAS CSCD 北大核心 2008年第7期1181-1189,共9页
分析了大型光学望远镜副镜位姿精调机构的性能要求,提出了基于Gough-Stewart平台机构的副镜位姿精调机构的2个设计准则:运动精度准则和刚度准则。选取Gough-Stewart平台机构的2个角度尺寸参数和3个无量纲化的线性尺寸参数作为设计变量,... 分析了大型光学望远镜副镜位姿精调机构的性能要求,提出了基于Gough-Stewart平台机构的副镜位姿精调机构的2个设计准则:运动精度准则和刚度准则。选取Gough-Stewart平台机构的2个角度尺寸参数和3个无量纲化的线性尺寸参数作为设计变量,分析了各设计变量对机构性能的影响规律;提出了与设计准则相对应的2个全条件性指标:运动传递精度指标和刚度指标,按照统一目标法的乘除法构造统一目标函数,建立有约束单目标优化问题数学模型。针对机构性能比较的实际需要,以普适空间替代全条件性指标中的可达工作空间。针对选定的设计变量定义域,以改进的遗传算法计算得到机构参数的Pareto最优解。结果表明,当动定平台的半径比为1.095时,机构性能最优,相对于动定平台的半径比≤1时的最优解,运动传递精度指标提高了0.7%,刚度指标减少了4.0%。本文的优化设计方法及最优解为位姿精调机构的优化设计提供了参考。 展开更多
关键词 望远镜副镜 位姿精调机构 Gough-Stewart平台机构 无量纲化参数 遗传算法 设计
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Diagnosing ΛHDE model with statefinder hierarchy and fractional growth parameter
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作者 LanJun Zhou Shuang Wang 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS CSCD 2016年第7期14-19,共6页
Recently, a new dark energy model called AHDE was proposed. In this model, dark energy consists of two parts: cosmological constant A and holographic dark energy (HDE). Two key parameters of this model are the frac... Recently, a new dark energy model called AHDE was proposed. In this model, dark energy consists of two parts: cosmological constant A and holographic dark energy (HDE). Two key parameters of this model are the fractional density of cosmological constant Ω2A0, and the dimensionless HDE parameter c. Since these two parameters determine the dynamical properties of DE and the destiny of universe, it is important to study the impacts of different values of ΩA0 and c on the AHDE model. In this paper, we apply various DE diagnostic tools to diagnose AHDE models with different values of ΩA0 and c; these tools include statefinder hierarchy {S3^(1) ,S4(1)fractional growth parameter E, and composite null diagnostic (CND), which is a combination of{S3(1),S4(1)} and E. We find that: (1) adopting different values of ΩA0 only has quantitative impacts on the evolution of the AHDE model, while adopting different c has qualitative impacts; (2) compared with S(1), S(41) can give larger differences among the cosmic evolutions of the AHDE model associated with different ΩA0 or different c; (3) compared with the case of using a single diagnostic, adopting a CND pair has much stronger ability to diagnose the AHDE model. 展开更多
关键词 dark energy COSMOLOGY cosmological constant
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