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Slow roll in simple non-canonical inflation

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Slow roll in simple non-canonical inflation

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dc.contributor.author Barenboim Szuchman, Gabriela Alejandra
dc.contributor.author Kinney, William H.
dc.date.accessioned 2015-04-28T07:55:45Z
dc.date.available 2015-04-28T07:55:45Z
dc.date.issued 2007
dc.identifier.citation Barenboim Szuchman, Gabriela Alejandra Kinney, William H. 2007 Slow roll in simple non-canonical inflation Journal Of Cosmology And Astroparticle Physics 07 03 014
dc.identifier.uri http://hdl.handle.net/10550/43453
dc.description.abstract We consider inflation using a class of non-canonical Lagrangians for which the modification to the kinetic term depends on the field, but not its derivatives. We generalize the standard Hubble slow roll expansion to the non-canonical case and derive expressions for observables in terms of the generalized slow roll parameters. We apply the general results to the illustrative case of ``Slinky'' inflation, which has a simple, exactly solvable, non-canonical representation. However, when transformed into a canonical basis, Slinky inflation consists of a field oscillating on a multi-valued potential. We calculate the power spectrum of curvature perturbations for Slinky inflation directly in the non-canonical basis, and show that the spectrum is approximately a power law on large scales, with a ``blue'' power spectrum. On small scales, the power spectrum exhibits strong oscillatory behavior. This is an example of a model in which the widely used solution of Garriga and Mukhanov gives the wrong answer for the power spectrum.
dc.language.iso eng
dc.relation.ispartof Journal Of Cosmology And Astroparticle Physics, 2007, vol. 07, num. 03, p. 014
dc.subject Física
dc.subject Astrofísica
dc.title Slow roll in simple non-canonical inflation
dc.type journal article es_ES
dc.date.updated 2015-04-28T07:55:45Z
dc.identifier.doi 10.1088/1475-7516/2007/03/014
dc.identifier.idgrec 039409
dc.rights.accessRights open access es_ES

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