Reconstructing the Inflaton Potential

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dc.creatorKolb, Edward W
dc.creatorAbney, Mark
dc.creatorCopeland, Edmund J
dc.creatorLiddle, Andrew R
dc.creatorLidsey, James E
dc.date1994-07-07
dc.date.accessioned2026-07-07T02:19:16Z
dc.date.available2026-07-07T02:19:16Z
dc.descriptionA review is presented of recent work by the authors concerning the use of large scale structure and microwave background anisotropy data to determine the potential of the inflaton field. The importance of a detection of the stochastic gravitational wave background is emphasised, and some preliminary new results of tests of the method on simulated data sets with uncertainties are described. (Proceedings of ``Unified Symmetry in the Small and in the Large'', Coral Gables, 1994)
dc.description13 pages, uuencoded postscript file with figures included (LaTeX file available from ARL), FERMILAB-Conf 94/189A
dc.identifierhttps://arxiv.org/abs/astro-ph/9407021
dc.identifierhttp://arxiv.org/abs/astro-ph/9407021
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9801
dc.subjectAstrophysics
dc.titleReconstructing the Inflaton Potential
dc.typetext

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