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Case for two-dimensional time

机译:二维时间的案例

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摘要

This paper brings in additional arguments in favor of two-dimensional time in the context of the diachronic approach to physical reality. The arguments are based on symmetry and convention considerations. Consider a distant event, for example, a meteorite impact on Mars now observedby us through a telescope in Greenwich, for example, or thanks to television signals sent by a Martian robot. Seen from Earth the Martian robot's clock displays what can be called synchronic local Einstein time, that clock having been synchronized by electromagnetic means according to Einstein'smethod. In the diachronic approach, this distant event is characterized by the offset between local Einstein time and the central terrestrial observer's own clock display in Greenwich. The latter display is taken to be the event's diachronic time and to constitute the fourth dimension of space-timein diachronic special relativity. The other temporal coordinate is the offset of local Einstein time with respect to central time, i.e., Greenwich time in the chosen example. In the diachronic approach, this offset serves as the radial coordinate in a spherical coordinate system centered onthe terrestrial observer. This time offset radial coordinate is currently used in astronomy, its values being typically expressed in light-years and interpreted as spatial distance. In the diachronic approach, the radial time offset is interpreted as a temporal distance. The two conceptualdistances are separated by 45° on a Minkowski space-time diagram. The two angles defining the telescope's orientation are the other two dimensions. At the now-here point (in Greenwich in the example), the two-dimensional time coordinate system allows one to speak of symmetry inthe up-dated historical content available to the central observer and to a second observer flying by. On their respective past light cones, the same events are displayed, and their diachronic time ordering is preserved, unlike in the conventional approach to special relativity. The preservationof photon detection time ordering is relevant to the explanation of some experiments with quantum entangled states. Implicit in the diachronic choice of coordinates is that a photon detection event is interpreted as an instantaneous transfer of energy and momentum from emitter to receiver.An important consequence of the diachronic approach is that the universe daily observed by astronomers is now regarded as part of our present physical reality from our terrestrial point of view. Moving the central observer into an orbit around a star like Sirius does not change the diachronicnature of the universe, so that this can also be taken by convention as another symmetry feature of the universe.
机译:本文带来了额外的论据,有利于在历时的物理现实方法的上下文中的二维时间。论点是基于对称性和公约的考虑因素。例如,考虑一个遥远的事件,例如,现在通过格林威治的望远镜观察Mars的陨石对火星的影响,或者由于火星机器人发送的电视信号。从地球看,火星机器人的时钟显示了可以称为同步本地爱因斯坦的时间,该时钟根据艾因斯坦的iInstein'smethod通过电磁方式同步。在历时的方法中,这种远处的事件的特点是当地爱因斯坦时间与中央地面观察者在格林威治的时钟显示之间的偏移。后一种显示器被认为是事件的历时的时间,并构成太空时滞历入高度相对性的第四维度。另一个时间坐标是当地爱因斯坦时间相对于中央时间,即在所选示例中的格林威治时间。在沿高频方法中,该偏移用作以地面观测器为中心的球面坐标系中的径向坐标。该时间偏移径向坐标目前用于天文学,其值通常在光年中表示并被解释为空间距离。在沿高频方法中,径向时间偏移被解释为时间距离。两种概念节目在Minkowski空间时间图上分开45°。定义望远镜定位的两个角度是其他两个维度。在现在的点(在榜样中的格林威治),二维时间坐标系允许一个人谈论对称的历史内容可供中央观察者和第二种观察者飞行。在各自过去的光锥上,显示相同的事件,并且它们的历时时间顺序被保留,与特殊相对性的传统方法不同。光子检测时间排序的保存与量子缠结状态的一些实验的解释是相关的。隐含在坐标的坐标中的选择是,光子检测事件被解释为从发射器到接收器的能量和动量的瞬时转移。历史反应方法的重要结果是天文学家观察到的宇宙现在被视为我们的一部分从我们的地面的角度出现体质现实。将中央观察者移动到像Sirius这样的星系周围的轨道上并没有改变宇宙的历时潮流,因此这也可以被惯例作为宇宙的另一个对称特征。

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