他的实在论还有两个主要特征:一、概念模式必须是空—时描述(spacetime representation)的;二、这种空—时描述必须是因果性的,严格地说,必须是以非概率定律的形式表现的。对于这两个特征,爱因斯坦还是有所偏重的。
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相应操作对应的代码和启动服务器时描述的代码几乎完全相同,所以这里没有列出。
The code for the corresponding action will be much the same as that described for starting the server, so it won't be listed here.
我已经在上面讨论cname字段时描述过了生成principalname数据结构的策略。
I have already described the strategy for authoring a PrincipalName data structure while discussing the cname field above.
海伦描述了她身处太空时失重状态下的生活。
Helen described life in a weightless environment during her period in space.
And today we'll finish that discussion, and, of course, point out actually the failure of classical mechanics to appropriately describe what's going on in an atom.
结束这部分的讨论,当然的,要指出经典力学,在描述原子内部,情况时是失败的。
Usually what I want to talk about is what's the smallest size class in which this function grows? With all of that, what that says b is that this we would write is order b.
通常我们想要的是,方法增长时最贴切的描述,也就是说,在这个问题上,算法关于。
The way he described is when you try to get down a quantum dimensions and you are standing there with your camera, just remember the sun is at your back and your shadow is always in the picture.
这种方法被他描述为,当你试着处理一个量子尺寸时,并且你试着拿着你的相机在那,记住太阳在你的背后,而你的影子总是在照片上。
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