Novel Planetary Signatures from the Dark Universe

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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.authorHaralambous, H.
dc.date.accessioned2024-05-19T14:50:26Z
dc.date.available2024-05-19T14:50:26Z
dc.date.issued2023
dc.departmentİstinye Üniversitesien_US
dc.description.abstractDunkle Materie (DM) came from unexpected cosmological observations. Nowadays within our solar system, diverse observations also defy conventional explanations, like the main physical process(es) underlying the heating of the different solar atmospheric layers. Streaming DM offers a viable common scenario following gravitational focusing by the solar system bodies. This fits as the underlying process behind the solar cycle, which was the first signature suggesting a planetary dependency. The challenge, since 1859, is to find a remote planetary impact, beyond the extremely feeble planetary tidal force. We stress the possible involvement of an external impact by some overlooked streaming invisible matter, which reconciles all investigated mysterious observations mimicking a not extant remote planetary force. Unexpected planetary relationships exist for both the dynamic Sun and Earth, reflecting multiple signatures for streaming DM. The local reasoning a la Zwicky is also suggestive for searches including puzzling biomedical phenomena. Favourite DM candidates are anti-quark-nuggets, magnetic monopoles, dark photons, or the composite pearls. Then, anomalies within the solar system are the manifestation of the dark Universe. The tentative streaming DM scenario enhances spatiotemporally the DM fluxen_US
dc.description.sponsorshipRepublic of Korea [IBS-R017-D1]en_US
dc.description.sponsorshipWe are thankful to Dima Budker for his encouraging words and remarks, who also has pointed out to use somemore recent publications. Y.K.S acknowledges support by IBS-R017-D1 of the Republic of Korea.en_US
dc.identifier.doi10.1007/s10511-024-09809-2
dc.identifier.endpage558en_US
dc.identifier.issn0571-7256
dc.identifier.issn1573-8191
dc.identifier.issue4en_US
dc.identifier.scopus2-s2.0-85182413256en_US
dc.identifier.scopusqualityQ4en_US
dc.identifier.startpage550en_US
dc.identifier.urihttps://doi.org10.1007/s10511-024-09809-2
dc.identifier.urihttps://hdl.handle.net/20.500.12713/5709
dc.identifier.volume66en_US
dc.identifier.wosWOS:001145333800007en_US
dc.identifier.wosqualityN/Aen_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
dc.language.isoenen_US
dc.publisherSpringer/Plenum Publishersen_US
dc.relation.ispartofAstrophysicsen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.snmz20240519_kaen_US
dc.subjectMatteren_US
dc.subjectSunen_US
dc.titleNovel Planetary Signatures from the Dark Universeen_US
dc.typeArticleen_US

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