Fingerprints of the Dark Universe in Geoscience

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dc.contributor.authorZioutas, K.
dc.contributor.authorAnastassopoulos, V.
dc.contributor.authorArgiriou, A.
dc.contributor.authorCantatore, G.
dc.contributor.authorCetin, S.
dc.contributor.authorGardikiotis, A.
dc.contributor.authorGuo J.
dc.date.accessioned2024-05-19T14:33:47Z
dc.date.available2024-05-19T14:33:47Z
dc.date.issued2024
dc.departmentİstinye Üniversitesien_US
dc.description1st International conference on Mediterranean Geosciences Union, MedGU 2021 -- 25 November 2021 through 28 November 2021 -- -- 304559en_US
dc.description.abstractDark matter (DM) dominates our universe, while its nature remains unknown. To unravel its composition is of fundamental importance for all physics. The solid Earth, with its atmosphere, could be the new target and detector of “invisible matter”. Any not well-understood dynamical behavior is of potential interest, e.g., the anomalous annual temperature excursions in the stratosphere and the global electron content of the Ionosphere (with its anomalous behavior around December-January known since 1937) also show planetary relationship, which is the ultimate signature for streaming DM involvement. Because this to happen is not expected within known physics, since a remote planetary tidal force is extremely feeble to cause any noticeable impact. Following this reasoning, here we present novel results combining the dynamical behavior of spatiotemporally occurring atmospheric activity with inner Earth activity like earthquakes. This finding should encourage geoscience to make the Earth the as-yet overlooked observatory for (streaming) DM, even parasitically, because Earth’s dynamic atmosphere and seismic activity are monitored continuously for other reasons. Of note, such an endeavor would be a natural extension of using the Earth to detect conventional cosmic rays. Exotic cosmic particles like anti quark nuggets, magnetic monopoles, and hidden-sector photons are among the most promising candidates. Other as-yet unpredicted DM constituents could make the surprise. © The Author(s), under exclusive license to Springer Nature Switzerland AG 2024.en_US
dc.identifier.doi10.1007/978-3-031-43218-7_96
dc.identifier.endpage419en_US
dc.identifier.isbn9783031432170
dc.identifier.issn2522-8714
dc.identifier.scopus2-s2.0-85189329991en_US
dc.identifier.scopusqualityQ3en_US
dc.identifier.startpage415en_US
dc.identifier.urihttps://doi.org/10.1007/978-3-031-43218-7_96
dc.identifier.urihttps://hdl.handle.net/20.500.12713/4333
dc.indekslendigikaynakScopusen_US
dc.language.isoenen_US
dc.publisherSpringer Natureen_US
dc.relation.ispartofAdvances in Science, Technology and Innovationen_US
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.snmz20240519_kaen_US
dc.subjectDark Matteren_US
dc.subjectEarthquakesen_US
dc.subjectGravitational Lensingen_US
dc.subjectIonosphereen_US
dc.subjectPlanetsen_US
dc.subjectStreamsen_US
dc.titleFingerprints of the Dark Universe in Geoscienceen_US
dc.typeConference Objecten_US

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