Second-order corrections to noncommutative spacetime inflation
arXiv:hep-th/0402198 · doi:10.1103/PhysRevD.70.043521
Abstract
We investigate how the uncertainty of noncommutative spacetime affects on inflation. For this purpose, the noncommutative parameter is taken to be a zeroth order slow-roll parameter. We calculate the noncommutative power spectrum up to second order using the slow-roll expansion. We find corrections arisen from a change of the pivot scale and the presence of a variable noncommutative parameter, when comparing with the commutative power spectrum. The power-law inflation is chosen to obtain explicit forms for the power spectrum, spectral index, and running spectral index. In cases of the power spectrum and spectral index, the noncommutative effect of higher-order corrections compensates for a loss of higher-order corrections in the commutative case. However, for the running spectral index, all higher-order corrections to the commutative case always provide negative spectral indexes, which could explain the recent WMAP data.
15 pages, no figure, version published in PRD
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- Observational constraints on patch inflation in noncommutative spacetime
- Inflationary universe in loop quantum cosmology
- Noncommutative Conformally Coupled Scalar Field Cosmology and its Commutative Counterpart
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- A Note on Noncommutative Brane Inflation
- Noncommutative KKLMMT Model
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- Flow equations in generalized braneworld scenarios
- Slow-roll reconstruction for running spectral index
- Cosmological constraints from Gauss-Bonnet braneworld with large-field potentials