Universe, Volume 8, Issue 1
2022 January - 56 articles
Cover Story: The probability that an observed gravitational wave has been (de-)amplified due to gravitational lensing by a given amount is a detector-dependent quantity. It is a function of lens distribution, distribution of sources, and detector sensitivity. We introduce a semi-analytic approach to determine the probability distribution of the magnification of a given source population observed with a given detector. We computed the expected magnification as both a function of redshift and of the observed source luminosity distance, which is the only quantity one can access in the absence of an electromagnetic counterpart. We show that we cannot reasonably ’tweak’ galaxy population models or stellar evolution models so that we could conclude that most of the observed LIGO/Virgo detections are strongly lensed. View this paper - Issues are regarded as officially published after their release is announced to the table of contents alert mailing list .
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