Cosmic Microwave Background Anisotropies and the Geometry of the Universe

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dc.creatorKamionkowski, Marc
dc.date1994-07-20
dc.date.accessioned2026-07-07T02:19:17Z
dc.date.available2026-07-07T02:19:17Z
dc.descriptionIn this talk, I review some recent work on cosmic microwave background (CMB) anisotropies in an open universe. I emphasize that the observed CMB anisotropies are still consistent with a low value of $Ω$, and I address the question of whether future CMB measurements will be able to provide information on the geometry of the Universe.
dc.description(8 page uuencoded PostScript file), IASSNS-HEP-94/56. To appear in the proceedings of the Case Western Reserve University CMB Workshop
dc.identifierhttps://arxiv.org/abs/astro-ph/9407062
dc.identifierhttp://arxiv.org/abs/astro-ph/9407062
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9809
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleCosmic Microwave Background Anisotropies and the Geometry of the Universe
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