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Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12128/6939
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dc.contributor.authorBiesiada, Marek-
dc.date.accessioned2018-11-05T12:42:12Z-
dc.date.available2018-11-05T12:42:12Z-
dc.date.issued1999-
dc.identifier.citationActa Physica Polonica. B, 1999, no. 11, s. 3211-3228pl_PL
dc.identifier.issn0587-4254-
dc.identifier.urihttp://hdl.handle.net/20.500.12128/6939-
dc.description.abstractLaser interferometrie experiments planned for 2002 will open up a new window onto the Universe. The first part of the paper gives a brief intuitive introduction to gravity waves, detection techniques and enumeration of main astrophysical sources and frequency bands to which they contribute. Then two more specific issues are discussed concerning cosmological perspectives of gravity waves detection. First one is the problem of gravitational lensing of the signal from inspiralling NS-NS binaries. The magnitude of the so called magnification bias is estimated and found non-negligible for some quite realistic lens models, but strongly modeldependent. The second problem is connected with estimates of galactic and extragalactic parts of the stochastic background. The main conclusion from these two examples is that in so far as the cosmological payoff of gravitational wave detection would be high, we should substantially deepen our understanding of basic astrophysical properties of galaxies and their clusters (in terms of mass distribution) in order to draw clear cosmological conclusions[…]pl_PL
dc.language.isoenpl_PL
dc.rightsUznanie autorstwa 3.0 Polska*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/pl/*
dc.subjectgravitational wavespl_PL
dc.subjectastrofizykapl_PL
dc.titleGravitational waves-new perspectivespl_PL
dc.typeinfo:eu-repo/semantics/articlepl_PL
dc.relation.journalActa Physica Polonica. Bpl_PL
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