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- Q1266091 subject Q7007334.
- Q1266091 subject Q7025480.
- Q1266091 subject Q8430682.
- Q1266091 subject Q8499139.
- Q1266091 abstract "Dark flow is an astrophysical term describing a possible non-random component of the peculiar velocity of galaxy clusters. The actual measured velocity is the sum of the velocity predicted by Hubble's Law plus a possible small and unexplained (or dark) velocity flowing in a common direction.According to standard cosmological models, the motion of galaxy clusters with respect to the cosmic microwave background should be randomly distributed in all directions. However, analyzing the three-year Wilkinson Microwave Anisotropy Probe (WMAP) data using the kinematic Sunyaev-Zel'dovich effect, astronomers Alexander Kashlinsky, F. Atrio-Barandela, D. Kocevski and H. Ebeling found evidence of a "surprisingly coherent" 600–1000 km/s flow of clusters toward a 20-degree patch of sky between the constellations of Centaurus and Vela.The researchers had suggested that the motion may be a remnant of the influence of no-longer-visible regions of the universe prior to inflation. Telescopes cannot see events earlier than about 380,000 years after the Big Bang, when the universe became transparent (the cosmic microwave background); this corresponds to the particle horizon at a distance of about 46 billion (4.6×1010) light years. Since the matter causing the net motion in this proposal is outside this range, it would in a certain sense be outside our visible universe; however, it would still be in our past light cone.The results appeared in the October 20, 2008, issue of Astrophysical Journal Letters.In 2013, data from the Planck spacecraft showed no evidence of "dark flow" on that sort of scale, discounting the claims of evidence for either gravitational effects reaching beyond the visible universe or existence of a multiverse. However in 2015 Kashlinsky et al claim to have found support for its existence using both Planck and WMAP data.".
- Q1266091 thumbnail 2MASS_LSS_chart-NEW_Nasa.jpg?width=300.
- Q1266091 wikiPageExternalLink 1010.4276v1.
- Q1266091 wikiPageExternalLink 100322-dark-flow-matter-outside-universe-multiverse.
- Q1266091 wikiPageExternalLink Galaxies_on_the_move.
- Q1266091 wikiPageExternalLink dn14098-hints-of-structure-beyond-the-visible-universe.html.
- Q1266091 wikiPageExternalLink PRD14.pdf.
- Q1266091 wikiPageExternalLink www.kashlinsky.info.
- Q1266091 wikiPageExternalLink mg20126921.900-dark-flow-proof-of-another-universe.html?full=true&print=true.
- Q1266091 wikiPageExternalLink 080923-dark-flows.html.
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- Q1266091 type Thing.
- Q1266091 comment "Dark flow is an astrophysical term describing a possible non-random component of the peculiar velocity of galaxy clusters. The actual measured velocity is the sum of the velocity predicted by Hubble's Law plus a possible small and unexplained (or dark) velocity flowing in a common direction.According to standard cosmological models, the motion of galaxy clusters with respect to the cosmic microwave background should be randomly distributed in all directions.".
- Q1266091 label "Dark flow".
- Q1266091 differentFrom Q18343.
- Q1266091 differentFrom Q5223514.
- Q1266091 differentFrom Q79925.
- Q1266091 depiction 2MASS_LSS_chart-NEW_Nasa.jpg.