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If Loud Aliens Explain Human Earliness, Quiet Aliens Are Also Rare

Hanson, Robin; Martin, Daniel; McCarter, Calvin; Paulson, Jonathan

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Authors

Robin Hanson

Daniel Martin

Calvin McCarter

Jonathan Paulson



Abstract

If life on Earth had to achieve n “hard steps“ to reach humanityʼs level, then the chance of this event rose as time to the nth power. Integrating this over habitable star formation and planet lifetime distributions predicts >99% of advanced life appears after today, unless n < 3 and max planet duration <50 Gyr. That is, we seem early. We offer this explanation: a deadline is set by loud aliens who are born according to a hard steps power law, expand at a common rate, change their volume appearances, and prevent advanced life like us from appearing in their volumes. Quiet aliens, in contrast, are much harder to see. We fit this three-parameter model of loud aliens to data: (1) birth power from the number of hard steps seen in Earth’s history, (2) birth constant by assuming a inform distribution over our rank among loud alien birth dates, and (3) expansion speed from our not seeing alien volumes in our sky. We estimate that loud alien civilizations now control 40%–50% of universe volume, each will later control ∼ 105 –3 × 107 galaxies, and we could meet them in ∼200 Myr–2 Gyr. If loud aliens arise from quiet ones, a depressingly low transition chance (<∼10−4 ) is required to expect that even one other quiet alien civilization has ever been active in our galaxy. Which seems to be bad news for the Search for Extraterrestrial Intelligence. But perhaps alien volume appearances are subtle, and their expansion speed lower, in which case we predict many long circular arcs to find in our sky.

Citation

Hanson, R., Martin, D., McCarter, C., & Paulson, J. (2021). If Loud Aliens Explain Human Earliness, Quiet Aliens Are Also Rare. Astrophysical Journal, 922(2), Article 182. https://doi.org/10.3847/1538-4357/ac2369

Journal Article Type Article
Acceptance Date Aug 31, 2021
Online Publication Date Nov 30, 2021
Publication Date Dec 1, 2021
Deposit Date Jan 18, 2022
Publicly Available Date Jan 18, 2022
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 922
Issue 2
Article Number 182
DOI https://doi.org/10.3847/1538-4357/ac2369

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