Small-scale tests of inflation
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Publication:5027067
DOI10.1088/1475-7516/2020/12/005zbMath1484.83131arXiv2008.00452OpenAlexW3111331080MaRDI QIDQ5027067
Hooshyar Assadullahi, Matteo Fasiello, Laura Iacconi, David Wands
Publication date: 3 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2008.00452
Relativistic cosmology (83F05) Anisotropy in solid mechanics (74E10) Gravitational waves (83C35) Effective quantum field theories (81T12)
Related Items (9)
Enhancing gravitational wave anisotropies with peaked scalar sources ⋮ Primordial stochastic gravitational wave background anisotropies: in-in formalization and applications ⋮ Spinning guest fields during inflation: leftover signatures ⋮ Primordial tensor bispectra in μ-CMB cross-correlations ⋮ Testing the early universe with anisotropies of the gravitational wave background ⋮ Primordial gravitational waves from excited states ⋮ Tensor non-Gaussianity in chiral scalar-tensor theories of gravity ⋮ Cross-correlations as a diagnostic tool for primordial gravitational waves ⋮ Probing parity-odd bispectra with anisotropies of GW V modes
Uses Software
Cites Work
- Bimetric gravity from ghost-free massive gravity
- Anisotropies of gravitational wave backgrounds: a line of sight approach
- Possible signatures of the inflationary particle content: spin-2 fields
- Anisotropic tensor power spectrum at interferometer scales induced by tensor squeezed non-Gaussianity
- Probing the inflationary particle content: extra spin-2 field
- Light Particles with Spin in Inflation
- Let Effective Field Theory of inflation flow: stochastic generation of models with red/blue tensor tilt
- Primordial tensor non-gaussianity from massive gravity
- Interferometer constraints on the inflationary field content
- Inflation and String Theory
- Squeezed tensor non-Gaussianity in non-attractor inflation
- Tensor non-gaussianities from non-minimal coupling to the inflaton
- Searching for bispectrum of stochastic gravitational waves with pulsar timing arrays
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