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THE ? SEARCH FOR EXTRATERRESTRIAL CIVILIZATIONS WITH LARGE ENERGY SUPPLIES. IV. THE SIGNATURES AND INFORMATION CONTENT OF TRANSITING MEGASTRUCTURES

机译:该?搜索具有大量能源的地外文明。 IV。过渡宏结构的标志和信息内容

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Arnold, Forgan, and Korpela et al. noted that planet-sized artificial structures could be discovered with Kepler as they transit their host star. We present a general discussion of transiting megastructures, and enumerate 10 potential ways their anomalous silhouettes, orbits, and transmission properties would distinguish them from exoplanets. We also enumerate the natural sources of such signatures. Several anomalous objects, such as KIC 12557548 and CoRoT-29, have variability in depth consistent with Arnold's prediction and/or an asymmetric shape consistent with Forgan's model. Since well-motivated physical models have so far provided natural explanations for these signals, the ETI hypothesis is not warranted for these objects, but they still serve as useful examples of how non-standard transit signatures might be identified and interpreted in a SETI context. Boyajian et al. recently announced KIC 8462852, an object with a bizarre light curve consistent with a "swarm" of megastructures. We suggest that this is an outstanding SETI target. We develop the normalized information content statistic M to quantify the information content in a signal embedded in a discrete series of bounded measurements, such as variable transit depths, and show that it can be used to distinguish among constant sources, interstellar beacons, and naturally stochastic or artificial, information-rich signals. We apply this formalism to KIC 12557548 and a specific form of beacon suggested by Arnold to illustrate its utility.
机译:Arnold,Forgan和Korpela等。他指出,开普勒可能会在其传播其恒星的过程中发现行星大小的人造结构。我们提出了一个关于正在运行的巨型结构的一般性讨论,并列举了它们的异常轮廓,轨道和传输特性将它们与系外行星区分开的10种潜在方式。我们还列举了此类签名的自然来源。几个异常物体,例如KIC 12557548和CoRoT-29,在深度上的变化与Arnold的预测一致,和/或与Forgan模型的不对称形状一致。由于到目前为止动机良好的物理模型已经为这​​些信号提供了自然的解释,因此对于这些对象而言,ETI假设不成立,但它们仍可作为在SETI上下文中如何识别和解释非标准运输签名的有用示例。博雅坚等。最近发布的KIC 8462852,其物体具有奇异的光线曲线,与庞大的“巨型”结构一致。我们建议这是一个出色的SETI目标。我们开发了归一化的信息含量统计量M来量化嵌入离散量有界测量(例如可变的传播深度)的离散系列中的信号中的信息含量,并表明它可用于区分恒定源,星际信标和自然随机源或人工的,信息丰富的信号。我们将此形式主义应用于KIC 12557548和Arnold建议的一种特定形式的信标,以说明其效用。

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