2015
DOI: 10.1088/1475-7516/2015/11/020
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Tachyon inflation in the large-Nformalism

Abstract: We study tachyon inflation within the large-N formalism, which takes a prescription for the small Hubble flow slow-roll parameter ϵ1 as a function of the large number of e-folds N. This leads to a classification of models through their behaviour at large N. In addition to the perturbative N class, we introduce the polynomial and exponential classes for the ϵ1 parameter. With this formalism we reconstruct a large number of potentials used previously in the literature for tachyon inflation. We also obtain new fa… Show more

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Cited by 21 publications
(39 citation statements)
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“…Barbosa-Cendejas et al [61] have expressed this formalism in terms of the parameter ε 1 = ε H . From Equation (3.53) we have…”
Section: Inflection-point Inflationmentioning
confidence: 99%
See 2 more Smart Citations
“…Barbosa-Cendejas et al [61] have expressed this formalism in terms of the parameter ε 1 = ε H . From Equation (3.53) we have…”
Section: Inflection-point Inflationmentioning
confidence: 99%
“…So called tachyon inflation is a string theory inspired model of inflation where the action has a certain form [28,61,198,199]. Although it has been shown by Kofman and Linde [200] that there are certain problems with tachyon inflation, it is considered here because it also has some nice properties.…”
Section: Tachyon Inflationmentioning
confidence: 99%
See 1 more Smart Citation
“…[57][58][59][60][61][62][63][64][65][66][67][68][69][70][71][72][73]. The cosmological implications of the tachyon were studied in [74][75][76][77][78][79][80][81][82][83][84][85][86]. For more details see also Refs.…”
Section: Introductionmentioning
confidence: 99%
“…Inflationary paradigm [75][76][77][78][79][80][81][82][83][84][85][86]92], 2. Primordial non-Gaussianity and CMB aspects [96][97][98][99][100][101][102][103][104], 3.…”
Section: Introductionmentioning
confidence: 99%