An Anomaly in the Angular Distribution of Quasar Magnitudes: Evidence for a Bubble Universe with a Mass ~10^21 M\odot
Michael J. Longo

TL;DR
This paper presents evidence for a massive bubble universe affecting quasar brightness distribution, suggesting a new cosmological structure that explains multiple large-scale anomalies across different observations.
Contribution
It introduces the hypothesis of a massive bubble universe as an explanation for various large-scale cosmic anomalies, supported by quasar and galaxy data.
Findings
Detection of a 'bulls eye' pattern in quasar magnitudes
Consistency of the anomaly across UV to infrared wavelengths
Correlation with other cosmic anomalies in the same sky region
Abstract
Quasars provide our farthest-reaching view of the Universe. The Sloan Survey now contains over 100,000 quasar candidates. A careful look at the angular distribution of quasar magnitudes shows a surprising intensity enhancement with a "bulls eye" pattern toward (alpha,delta) ~ (195{\deg}, 0{\deg}) for all wavelengths from UV through infrared. The angular pattern and size of the enhancement is very similar for all wavelengths, which is inconsistent with a Doppler shift due to a large peculiar velocity toward that direction. The shift is also too large to explain as a systematic error in the quasar magnitudes. The general features of the anomaly can be explained by the gravitational lensing of a massive bubble with Mlens ~ 10^21 M\odot, a lens radius ~350 Mpc, and with the lens subtending an angle of \pm15{\deg} on the sky. It is remarkable that the presence of such a massive bubble…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Cosmology and Gravitation Theories
