论文标题
从宇宙噪声中找到ET信号
Finding the ET Signal from the Cosmic Noise
论文作者
论文摘要
本文强调了一种方法论方法，旨在通过假设传输技术可能具有两个特征来增强搜索外星智力（SETI），这可能具有两个特征：1）在微波炉或更高频率范围内，该频率来自所假定的ET Interanet interanetranety导航/通信（/nav/commiss）网络，X-ray基于X-ray基于X-ray navigation（XN）naviation（x-naviation）。 对该领域的潜在贡献包括在电磁频谱中找到传输技术和其他技术签名方面提高准确性，这是达到Schelling点的常见标准（相互实现了我们和ETS如何彼此找到彼此），以及诸如Drake方程之类的模型。
This paper highlights a methodological approach designed to enhance the search for extraterrestrial intelligence (SETI) by hypothesizing that a transmission technosignature would likely have two features: 1) be wideband in the microwave or higher frequency range that originates from a hub within a supposed ET interplanetary navigation/communication (nav/comm) network, and 2) contain x-ray pulsar-based navigation (XNAV) metadata. Potential contributions to the field include improved accuracy in finding transmission technosignatures and other technosignatures in the electromagnetic spectrum, a common standard in reaching a Schelling Point (a mutual realization of how we and ETs can find each other), and operationalizing models such as the Drake Equation.
