The Universe as a Diffusive Medium -- Constraining or Detecting the Gravitational Wave Background

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dc.creatorMarleau, Francine
dc.creatorStarkman, Glenn
dc.date1996-05-14
dc.date.accessioned2026-07-07T02:21:16Z
dc.date.available2026-07-07T02:21:16Z
dc.descriptionWe calculate the ``seeing'' effect on distant sources due to a gravitational wave background. We derive the limit in strain and energy density of the gravitational wave based on the limit of detectability of this effect with the present day telescope resolution. We also compare our detection limit to those obtained from existing methods.
dc.description7 pages LaTeX (uses REVTeX), 1 figure as separate PostScript file, submitted to Phys. Rev. D -- Brief Reports
dc.identifierhttps://arxiv.org/abs/astro-ph/9605066
dc.identifierhttp://arxiv.org/abs/astro-ph/9605066
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10485
dc.subjectAstrophysics
dc.titleThe Universe as a Diffusive Medium -- Constraining or Detecting the Gravitational Wave Background
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