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dc.contributor.authorPenner, A. Raymond
dc.date.accessioned2018-04-05T16:12:04Z
dc.date.available2018-04-05T16:12:04Z
dc.date.issued2017-04
dc.identifier.citationPenner, A.R. (2017). Gravitational anti-screening and binary galaxies. Astrophysics and Space Science, 362(4), 1-10. DOI: 10.1007/s10509-017-3054-7en
dc.identifier.issn0004-640X
dc.identifier.otherDOI: 10.1007/s10509-017-3054-7en
dc.identifier.otherDOI: 10.25316/IR-635
dc.identifier.urihttp://hdl.handle.net/10613/5698
dc.identifier.urihttp://dx.doi.org/10.25316/IR-635
dc.descriptionPre-printen
dc.description.abstractPreviously, in Penner (2016a, 2016b), a theory of gravitational anti-screening was shown to lead naturally to the Baryonic Tully-Fisher Relationship. In addition, it was shown to agree with the observed rotational curve of the Galaxy, the observed features in the rotational curves of other spiral galaxies, with observations of the Coma cluster, and with a geometrically flat universe. In this paper the theory will now be applied to binary galaxies. It is shown that there is a relationship between the line-of-sight velocity difference of the pair and the individual rotational velocities of the galaxies. The resulting probability function for β, defined as the ratio of the line-of-sight velocity difference to the rotational velocity of the larger galaxy of the pair, is in excellent agreement with the observations taken by multiple researchers for the case of the binaries being on radial orbits.en
dc.format.extent23 pg.en
dc.format.mediumtexten
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherSpringeren
dc.subject.lcshDark matter (Astronomy)en
dc.subject.lcshGalaxiesen
dc.subject.lcshGravitationen
dc.subject.lcshCosmologyen
dc.title[Pre-print] Gravitational anti-screening and binary galaxiesen
dc.typeArticleen
dc.description.versionPre-printen
dc.description.noteThis is a pre-copyedited, author produced version of an article published as: Penner, A.R. (2017). Gravitational anti-screening and binary galaxies. Astrophysics and Space Science, 362(4), 1-10. DOI: 10.1007/s10509-017-3054-7 The final publication is available at Springer via http://dx.doi.org/10.1007/s10509-017-3054-7.en
dc.description.fulltexthttps://viurrspace.ca/bitstream/handle/10613/5698/Penner.80.pdf?sequence=3en
dc.identifier.doi10.1007/s10509-017-3054-7
dc.identifier.doi10.25316/IR-635


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