Limits on the Gravity Wave Background From Microlensed Quasars

dc.creatorGould, Andrew
dc.date1995-07-18
dc.date1995-08-01
dc.date.accessioned2026-07-07T08:58:18Z
dc.date.available2026-07-07T08:58:18Z
dc.descriptionThe paper previously submitted under this title is incorrect in that it drastically overestimates the cumulative deflection due to a gravitational wave (GW) background. Avi Loeb gives a simple argument that there can be no $(Dω)^{1/2}$ enhancement: since the problem is linear in $h$, one can decompose the GWs into plane waves and for each of these there is no enhancement.
dc.descriptionThis paper was incorrect in that it drastically overestimated the cumulative deflection due to a gravitational wave background. Withdrawn
dc.identifierhttps://arxiv.org/abs/astro-ph/9507069
dc.identifierhttp://arxiv.org/abs/astro-ph/9507069
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/147276
dc.subjectAstrophysics
dc.titleLimits on the Gravity Wave Background From Microlensed Quasars
dc.typetext

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