Drift Rates of Narrowband Signals in Long-term SETI Observations for Exoplanets
Jian-Kang Li, Haichen Zhao, Zhenzhao Tao, Tong-Jie Zhang, Sun Xiaohui

TL;DR
This paper analyzes how the relative motions of Earth and exoplanets cause drifting in narrowband signals, proposing that long-term observations can reveal characteristic pseudosinusoidal patterns useful for SETI detection.
Contribution
It introduces a celestial mechanics-based model for predicting drift rates of extraterrestrial signals and suggests using long-term observations to identify characteristic drifting patterns.
Findings
Expected pseudosinusoidal drift patterns in long-term observations
Higher exoplanet eccentricities cause asymmetric drifts
Intermittent pseudosinusoidal curves serve as a new detection criterion
Abstract
The Doppler shift of a radio signal is caused by the relative motion between the transmitter and receiver. The change in frequency of the signal over time is called drift rate. In the studies of radio SETI (Search for Extraterrestrial Intelligence), extraterrestrial narrowband signals are expected to appear "chirped" since both the exoplanet and the Earth are moving. Such planet rotation and orbital revolution around the central star can cause a non-zero drift rate. Other relative motions between the transmitter and receiver, such as the gravitational redshift and galactic potential, are negligible. In this paper, we mainly consider the common cases that the drift rate is contributed by the rotations and orbits of the Earth and exoplanet in celestial mechanics perspective, and briefly discuss other cases different from the Earth-exoplanet one. We can obtain the expected pseudosinusoidal…
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Taxonomy
TopicsSpace Science and Extraterrestrial Life · Radio Astronomy Observations and Technology · Gamma-ray bursts and supernovae
