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dc.contributor.authorStevens, A.
dc.contributor.authorForgan, Duncan
dc.contributor.authorJames, J.O.
dc.date.accessioned2016-04-22T23:32:46Z
dc.date.available2016-04-22T23:32:46Z
dc.date.issued2015
dc.identifier.citationStevens , A , Forgan , D & James , J O 2015 , ' Observational signatures of self-destructive civilizations ' International Journal of Astrobiology , vol. FirstView . DOI: 10.1017/S1473550415000397en
dc.identifier.issn1473-5504
dc.identifier.otherPURE: 229669638
dc.identifier.otherPURE UUID: 98894914-ab9b-48dd-8aca-ed0842cc17f9
dc.identifier.otherScopus: 84945156665
dc.identifier.urihttp://hdl.handle.net/10023/8671
dc.descriptionD. F. gratefully acknowledges support from the ECOGAL ERC advanced grant, and the STFC grant ST/J001422/1.en
dc.description.abstractWe address the possibility that intelligent civilizations that destroy themselves could present signatures observable by humanity. Placing limits on the number of self-destroyed civilizations in the Milky Way has strong implications for the final three terms in Drake's Equation, and would allow us to identify which classes of solution to Fermi's Paradox fit with the evidence (or lack thereof). Using the Earth as an example, we consider a variety of scenarios in which humans could extinguish their own technological civilization. Each scenario presents some form of observable signature that could be probed by astronomical campaigns to detect and characterize extrasolar planetary systems. Some observables are unlikely to be detected at interstellar distances, but some scenarios are likely to produce significant changes in atmospheric composition that could be detected serendipitously with next-generation telescopes. In some cases, the timing of the observation would prove crucial to detection, as the decay of signatures is rapid compared with humanity's communication lifetime. In others, the signatures persist on far longer timescales.en
dc.language.isoeng
dc.relation.ispartofInternational Journal of Astrobiologyen
dc.rightsCopyright © Cambridge University Press 2015. This work is made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at https://dx.doi.org/10.1017/S1473550415000397en
dc.subjectDead civilizationsen
dc.subjectFermi's Paradoxen
dc.subjectObservational techniquesen
dc.subjectSETIen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectT-NDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleObservational signatures of self-destructive civilizationsen
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1017/S1473550415000397
dc.description.statusPeer revieweden
dc.date.embargoedUntil23-04-20


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