Supersymmetric DBI inflation
arXiv:1205.1353 · doi:10.1016/j.physletb.2012.10.006
Abstract
We discuss a supersymmetric version of DBI (Dirac-Born-Infeld) inflation, which is a typical inflation model in string cosmology. The supersymmetric DBI action together with a superpotential always leads to correction terms associated with the potential into the kinetic term, which drastically change the dynamics of DBI inflation. We find two significant features of supersymmetric DBI inflation. The first one is that ultra-relativistic motion is prohibited to cause inflation, which leads to order of unity sound velocity squared and hence small non-Gaussianities of primordial curvature perturbations. The second one is that the relation between the tensor-to-scalar ratio and the field variation is modified. Then, significant tensor-to-scalar ratio is possible even for sub-Planck variation of the field. These new features are in sharp contrast with those of the standard non-supersymmetric DBI inflation and hence have a lot of interest implications on upcoming observations of cosmic microwave background (CMB) anisotropies by the Planck satellite as well as direct detection experiments of gravitational waves like DECIGO and BBO.
5 pages, final version accepted for publication in PLB
References in corpus (12)
- Observational Signatures and Non-Gaussianities of General Single Field Inflation
- G-inflation: inflation driven by the Galileon field
- CMBPol Mission Concept Study: Probing Inflation with CMB Polarization
- Galileon inflation
- Primordial perturbations and non-Gaussianities in DBI and general multi-field inflation
- A Microscopic Limit on Gravitational Waves from D-brane Inflation
- Primordial fluctuations and non-Gaussianities in multi-field DBI inflation
- Comparing Infrared Dirac-Born-Infeld Brane Inflation to Observations
- Gravitational Wave Constraints on DBI Inflation
- Flux interactions on D-branes and instantons
- IR Inflation from Multiple Branes
- Deformation of Super Yang-Mills Theories in R-R 3-form Background
Cited by in corpus (29)
- On the Starobinsky Model of Inflation from Supergravity
- Higher-Derivative Chiral Superfield Actions Coupled to N=1 Supergravity
- DBI Galileon inflation in background SUGRA
- BPS States in Supersymmetric Chiral Models with Higher Derivative Terms
- The goldstone and goldstino of supersymmetric inflation
- A supersymmetric Skyrme model
- The Imaginary Starobinsky Model and Higher Curvature Corrections
- Classifying BPS States in Supersymmetric Gauge Theories Coupled to Higher Derivative Chiral Models
- Higher Derivative Corrections to Manifestly Supersymmetric Nonlinear Realizations
- Topological solitons in the supersymmetric Skyrme model
- Ghostbusters in higher derivative supersymmetric theories: who is afraid of propagating auxiliary fields?
- DBI Inflation in N=1 Supergravity
- Higher derivative three-form gauge theories and their supersymmetric extension
- Supersymmetry Breaking in Spatially Modulated Vacua
- Topological couplings in higher derivative extensions of supersymmetric three-form gauge theories
- Ghost-free vector superfield actions in supersymmetric higher-derivative theories
- Stable small spatial hairs in a power-law k-inflation model
- CMB imprints of non-canonical anisotropic inflation
- Supersymmetry breaking and ghost Goldstino in modulated vacua
- Ghostbusters in supergravity
- KK-number non-conserving decays: Signal of n = 2 excitations of Extra-Dimensional Models at the LHC
- More on DBI action in 4D supergravity
- High Energy Physics and Cosmology at the Unification Frontier: Opportunities and Challenges in the coming years
- Higher Derivative Supersymmetric Nonlinear Sigma Models on Hermitian Symmetric Spaces, and BPS States Therein
- Supersymmetric Dirac-Born-Infeld Axionic Inflation and Non-Gaussianity
- Enhancement of the Axion Decay Constant in Inflation and the Weak Gravity Conjecture
- Horndeski model in nonlinearly realized supergravity
- On the validity of cosmic no-hair conjecture in an anisotropic inflationary model
- Vacua by Derivative Corrections in Supergravity with Matter Multiplets