Coherence and Sakharov Oscillations in the Microwave Sky

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dc.creatorAlbrecht, Andreas
dc.date1996-12-02
dc.date.accessioned2026-07-07T02:22:25Z
dc.date.available2026-07-07T02:22:25Z
dc.descriptionI discuss the origin of the ``Sakharov oscillations'' (or ``secondary Doppler peaks'') in standard angular power spectra of the Cosmic Microwave Background anisotropies calculated for inflationary models. I contrast this with the production of CMB anisotropies in `active' models and argue that the presence or absence of Sakharov oscillations will reveal fundamental properties of the primordial perturbations.
dc.description13 pages including 4 figures. To appear in proceedings of the XXXIst Rencontre de Moriond, `Microwave Background Anisotropies'
dc.identifierhttps://arxiv.org/abs/astro-ph/9612015
dc.identifierhttp://arxiv.org/abs/astro-ph/9612015
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10869
dc.subjectAstrophysics
dc.titleCoherence and Sakharov Oscillations in the Microwave Sky
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