Non-trivial running of the primordial tensor spectrum
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- Type
- preprint
- Published
- 2014-03-20
- Cited by
- 5
- References
- 18
- Access
- Open access
- OpenAlex
- https://openalex.org/W258449867
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:117933402
Keywords
Spectral density, Physics, Spectral index, Tensor (intrinsic definition), Polarization (electrochemistry)
References
- Punctuated inflation and the low CMB multipoles
- Features of heavy physics in the CMB power spectrum
- Correlating features in the primordial spectra
- Closed String Thermodynamics and a Blue Tensor Spectrum
- Mass hierarchies and non-decoupling in multi-scalar field dynamics
- Localized correlated features in the CMB power spectrum and primordial bispectrum from a transient reduction in the speed of sound
- The Standard Model Higgs boson as the inflaton
- Planck 2013 results. XVI. Cosmological parameters
- Equilateral non-Gaussianity from multifield dynamics
- Correlating correlation functions of primordial perturbations
- Effective theories of single field inflation when heavy fields matter
- Non-Gaussianity consistency relations, initial states and back-reaction
- Detection of B-mode polarization at degree angular scales by BICEP2.
- Lessons from the running of the tensor-to-scalar ratio
- Tensor-to-scalar ratio in punctuated inflation
- Planck 2015. XX. Constraints on inflation
- Inflationary Cosmology after Planck 2013
- ournal of C osmology and A stroparticle hysics Suppressing the impact of a high tensor-to-scalar ratio on the temperature anisotropies
- Effective theories of single field inflation when heavy fields matter
Cited by
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