论文标题
搜索靶向Alpha Centauri的太阳引力镜头的无线电签名
A Search for Radio Technosignatures at the Solar Gravitational Lens Targeting Alpha Centauri
论文作者
论文摘要
恒星以其引力重点为星际通信提供了巨大的收益,也许是星际网络的一部分。如果太阳是这种网络的一部分,则应在附近恒星的重力焦点处有探针。如果连接到该网络的太阳系中有探针,我们可以通过拦截这些焦点中继传输的传输来检测它们。在这里,我们使用绿色银行望远镜(GBT)(GBT)和突破性的收听(BL)后端展示了超越太阳最内向的重力焦点的星际通信中继的搜索。作为第一个目标,我们在Alpha Centauri AB系统的焦点上搜索了一个继电器,同时由于围绕太阳的地球轨道校正了视差。我们从L和S频段中的这样的源搜索了针对内部太阳系的无线电信号。我们使用BL开发的Turboseti软件的分析未检测到任何指示非人造人工来源的信号。进一步的分析排除了附近目标HD 13908的虚假负面因素和信号。假设L频段的保守增益为10^3,大约4倍,在S频段中,在550 au或23 w au的7 W上方可以检测到〜1米的定向发射器,或者在550 au或L频段的1000 au中,在1000 au中以上23 w,而在550 au或7 w af 1000 au au au au au au au au a in 1000 au au au a in 1000 au au au au a in 1000 au。最后,我们讨论了该方法在其他频率和目标中的应用。
Stars provide an enormous gain for interstellar communications at their gravitational focus, perhaps as part of an interstellar network. If the Sun is part of such a network, there should be probes at the gravitational foci of nearby stars. If there are probes within the solar system connected to such a network, we might detect them by intercepting transmissions from relays at these foci. Here, we demonstrate a search across a wide bandwidth for interstellar communication relays beyond the Sun's innermost gravitational focus at 550 AU using the Green Bank Telescope (GBT) and Breakthrough Listen (BL) backend. As a first target, we searched for a relay at the focus of the Alpha Centauri AB system while correcting for the parallax due to Earth's orbit around the Sun. We searched for radio signals directed at the inner solar system from such a source in the L and S bands. Our analysis, utilizing the turboSETI software developed by BL, did not detect any signal indicative of a non-human-made artificial origin. Further analysis excluded false negatives and signals from the nearby target HD 13908. Assuming a conservative gain of 10^3 in L-band and roughly 4 times that in S-band, a ~1 meter directed transmitter would be detectable by our search above 7 W at 550 AU or 23 W at 1000 AU in L-band, and above 2 W at 550 AU or 7 W at 1000 AU in S-band. Finally, we discuss the application of this method to other frequencies and targets.