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dc.contributor.author | Barenboim, Gabriela | en_US |
dc.contributor.author | Kinney, William H. | en_US |
dc.date.accessioned | 2008-12-10T12:14:06Z | - |
dc.date.available | 2008-12-10T12:14:06Z | - |
dc.date.issued | 2007-03-15 | en_US |
dc.identifier.citation | Journal of Cosmology and Astroparticle Physics 3: 014 (2007) | en_US |
dc.identifier.citation | JCAP03(2007)014 | - |
dc.identifier.issn | 1475-7516 | en_US |
dc.identifier.uri | http://hdl.handle.net/10261/9079 | - |
dc.description | 17 pages, 4 figures.-- ISI Article Identifier: 000245945000008.-- ArXiv pre-print available at: http://arxiv.org/abs/astro-ph/0701343 | en_US |
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 behaviour. 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. | en_US |
dc.description.sponsorship | WHK is supported in part by the National Science Foundation under grant NSF-PHY-0456777. GB is grateful for the support from the Spanish MEC under Contract PR2006-0195 and FPA 2005/1678. | - |
dc.format.extent | 2373 bytes | - |
dc.format.mimetype | text/plain | - |
dc.language.iso | eng | en_US |
dc.publisher | International School for Advanced Studies | en_US |
dc.publisher | Institute of Physics Publishing | - |
dc.rights | openAccess | en_US |
dc.subject | K-inflation | en_US |
dc.subject | Physics of the early universe | en_US |
dc.subject | Cosmological perturbation theory | en_US |
dc.subject | Flatness | en_US |
dc.subject | Horizon | en_US |
dc.title | Slow roll in simple non-canonical inflation | en_US |
dc.type | artículo | en_US |
dc.identifier.doi | 10.1088/1475-7516/2007/03/014 | - |
dc.description.peerreviewed | Peer reviewed | en_US |
dc.relation.publisherversion | http://dx.doi.org/10.1088/1475-7516/2007/03/014 | en_US |
dc.type.coar | http://purl.org/coar/resource_type/c_6501 | es_ES |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.cerifentitytype | Publications | - |
item.openairetype | artículo | - |
item.languageiso639-1 | en | - |
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0701343v2.pdf | 210,68 kB | Adobe PDF | Visualizar/Abrir |
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