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Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12128/7301
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dc.contributor.authorBiesiada, Marek-
dc.date.accessioned2018-11-30T12:27:39Z-
dc.date.available2018-11-30T12:27:39Z-
dc.date.issued2003-
dc.identifier.citationActa Physica Polonica B, Vol. 34, no. 11 (2003), s. 5423-5432pl_PL
dc.identifier.issn0587-4254-
dc.identifier.urihttp://hdl.handle.net/20.500.12128/7301-
dc.description.abstractFuture generation of interferometric gravitational wave detectors is hoped to provide accurate measurements of the final stages of binary in-spirals. The sources probed by such experiments are of extragalactic origin and the observed chirp mass distribution carries information about their redshifts. Moreover the luminosity distance is directly observable is such experiments. This creates the possibility to establish a new kind of cosmo- logical tests, supplementary to more standard ones. The paper discusses the utility of gravity wave experiments for testing the dark energy in the Universe, which is one of the most important issues in modern cosmology.pl_PL
dc.language.isoenpl_PL
dc.rightsUznanie autorstwa 3.0 Polska*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/pl/*
dc.subjectfale grawitacyjnepl_PL
dc.subjectgenerowanie falpl_PL
dc.subjectgwiazdypl_PL
dc.subjectkosmologiapl_PL
dc.titlePerspective for testing dark energy scenarios with advanced LIGO type gravity wave experimentspl_PL
dc.typeinfo:eu-repo/semantics/articlepl_PL
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