Multi-field DBI inflation: introducing bulk forms and revisiting the gravitational wave constraints
We study multi-field Dirac-Born-Infeld (DBI) inflation models, taking into account the NS-NS and R-R bulk fields present in generic flux compactifications. We compute the second-order action, which governs the behaviour of linear cosmological perturbations, as well as the third-order action, which c...
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Published in | Journal of cosmology and astroparticle physics Vol. 2009; no. 4; p. 021 |
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Abstract | We study multi-field Dirac-Born-Infeld (DBI) inflation models, taking into account the NS-NS and R-R bulk fields present in generic flux compactifications. We compute the second-order action, which governs the behaviour of linear cosmological perturbations, as well as the third-order action, which can be used to calculate non-Gaussianities in these models. Remarkably, for scalar-type perturbations, we show that the contributions due to the various form fields exactly cancel in both the second- and third-order actions. Primordial perturbations and their non-Gaussianities are therefore unaffected by the presence of form fields and our previous results are unmodified. We also study vector-type perturbations associated with the U(1) gauge field confined on the D3-brane, and discuss whether their quantum fluctuations can be amplified. Finally, we revisit the gravitational wave constraints on DBI inflation and show that an ultra-violet DBI multi-field scenario is still compatible with data, in contrast with the single field case, provided there is a transfer from entropy into adiabatic perturbations. |
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AbstractList | We study multi-field Dirac-Born-Infeld (DBI) inflation models, taking into account the NS-NS and R-R bulk fields present in generic flux compactifications. We compute the second-order action, which governs the behaviour of linear cosmological perturbations, as well as the third-order action, which can be used to calculate non-Gaussianities in these models. Remarkably, for scalar-type perturbations, we show that the contributions due to the various form fields exactly cancel in both the second- and third-order actions. Primordial perturbations and their non-Gaussianities are therefore unaffected by the presence of form fields and our previous results are unmodified. We also study vector-type perturbations associated with the U(1) gauge field confined on the D3-brane, and discuss whether their quantum fluctuations can be amplified. Finally, we revisit the gravitational wave constraints on DBI inflation and show that an ultra-violet DBI multi-field scenario is still compatible with data, in contrast with the single field case, provided there is a transfer from entropy into adiabatic perturbations. |
Author | Langlois, David Steer, Danièle A Renaux-Petel, Sébastien |
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Snippet | We study multi-field Dirac-Born-Infeld (DBI) inflation models, taking into account the NS-NS and R-R bulk fields present in generic flux compactifications. We... |
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SubjectTerms | Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY BORN-INFELD THEORY COMPACTIFICATION Cosmology and Extra-Galactic Astrophysics D-BRANES DIRAC COSMOLOGY DISTURBANCES ENTROPY FLUCTUATIONS GAUGE INVARIANCE General Relativity and Quantum Cosmology GRAVITATIONAL WAVES High Energy Physics - Theory INFLATIONARY UNIVERSE LIMITING VALUES NONLUMINOUS MATTER Physics PHYSICS OF ELEMENTARY PARTICLES AND FIELDS SCALARS Sciences of the Universe U-1 GROUPS |
Title | Multi-field DBI inflation: introducing bulk forms and revisiting the gravitational wave constraints |
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