Sketching the inflaton potential

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dc.creatorTerrero-Escalante, C. A.
dc.date2002-04-03
dc.date.accessioned2026-07-07T02:03:20Z
dc.date.available2026-07-07T02:03:20Z
dc.descriptionBased on solutions of the Stewart-Lyth inverse problem it is argued that in the CMB data analysis the parametrization of the primordial spectra from inflation must include the `running' of both, scalar and tensorial, spectral indices if information beyond the exponential potential model is wanted to be detected.
dc.descriptionTo appear in the Proceedings of the ``1st Mexican Meeting on Mathematical and Experimental Physics", El Colegio Nacional, Mexico City, September, 2001. 8 pages, uses kapproc.cls
dc.identifierhttps://arxiv.org/abs/astro-ph/0204064
dc.identifierhttp://arxiv.org/abs/astro-ph/0204064
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4354
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSketching the inflaton potential
dc.typetext

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