Evidence for a Preferred Handedness of Spiral Galaxies

dc.creatorLongo, Michael J.
dc.date2009-04-16
dc.date.accessioned2026-07-07T13:05:05Z
dc.date.available2026-07-07T13:05:05Z
dc.descriptionIn this article I extend an earlier study of spiral galaxies in the Sloan Digital Sky Survey (SDSS) to investigate whether the universe has an overall handedness. A preference for spiral galaxies in one sector of the sky to be left-handed or right-handed spirals would indicate a parity-violating asymmetry in the overall universe and a preferred axis. The previous study used 2616 spiral galaxies with redshifts <0.04 and identified handedness. The new study uses 15158 with redshifts <0.085 and obtains very similar results to the first with a signal exceeding 5 sigma, corresponding to a probability ~2.5x10-7 for occurring by chance. A similar asymmetry is seen in the Southern Galaxy spin catalog of Iye and Sugai. The axis of the dipole asymmetry lies at approx. (l, b) =(52 d, 68.5 d), roughly along that of our Galaxy and close to alignments observed in the WMAP cosmic microwave background distributions.
dc.descriptionIncreased data sample by factor of 7. Fit to dipole without prior assumptions or binning gives probability of 1.5x10-4
dc.identifierhttps://arxiv.org/abs/0904.2529
dc.identifierhttp://arxiv.org/abs/0904.2529
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/227382
dc.subjectCosmology and Nongalactic Astrophysics
dc.subjectAstrophysics of Galaxies
dc.titleEvidence for a Preferred Handedness of Spiral Galaxies
dc.typetext

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