Interferometer constraints on the inflationary field content

DOI10.1088/1475-7516/2020/03/031zbMath1490.83077arXiv1910.12921OpenAlexW2982371576MaRDI QIDQ5068422

David Wands, Emanuela Dimastrogiovanni, Laura Iacconi, Hooshyar Assadullahi, Matteo Fasiello

Publication date: 6 April 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1910.12921

zbMATH Keywords

inflationcosmological perturbation theoryprimordial gravitational waves (theory)

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Spectrum, resolvent (47A10) Geometrodynamics and the holographic principle (83E05) Perturbations in context of PDEs (35B20) Gravitational waves (83C35) Radiative transfer in astronomy and astrophysics (85A25)

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 ⋮ Testing the early universe with anisotropies of the gravitational wave background ⋮ Inflation with antisymmetric tensor field: new candidates ⋮ Cross-correlations as a diagnostic tool for primordial gravitational waves ⋮ Gravitational waves from inflation with antisymmetric tensor field ⋮ Small-scale tests of inflation ⋮ Probing parity-odd bispectra with anisotropies of GW V modes

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