Large Scale Periodicity in Redshift Distribution

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dc.creatorBajan, K.
dc.creatorBiernacka, M.
dc.creatorFlin, P.
dc.creatorGodlowski, W.
dc.creatorPervushin, V.
dc.creatorZorin, A.
dc.date2004-08-30
dc.date.accessioned2026-07-07T02:14:25Z
dc.date.available2026-07-07T02:14:25Z
dc.descriptionWe review the previous studies of galaxies and quasar redshifts discretisation. We present also the investigations of the large scale periodicity, detected by pencil--beam observations, which revealed 128 (1/h) Mpc period, afterwards confirmed with supercluster studies. We present the theoretical possibility of obtaining such a periodicity using a toy-model. We solved the Kepler problem, i.e. the equation of motion of a particle with null energy moving in the uniform, expanding Universe, decribed by FLRW metrics. It is possible to obtain theoretically the separation between large scale structures similar to the observed one.
dc.descriptionTalk presented at 2-nd Gravitational Conference ``Gravitation, and relativistic astrophysics'', 23--27 June 2003 Kharkov, Ukraine (4 pages, 1 figure)
dc.identifierhttps://arxiv.org/abs/astro-ph/0408551
dc.identifierhttp://arxiv.org/abs/astro-ph/0408551
dc.identifierSpacetime & Substance, Vol. 4 (2003) pp. 225-228
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8106
dc.subjectAstrophysics
dc.titleLarge Scale Periodicity in Redshift Distribution
dc.typetext

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