Anisotropic tensor power spectrum at interferometer scales induced by tensor squeezed non-Gaussianity

DOI10.1088/1475-7516/2018/02/011OpenAlexW3102031542MaRDI QIDQ5022071

Angelo Ricciardone, Gianmassimo Tasinato

Publication date: 18 January 2022

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

Full work available at URL: https://arxiv.org/abs/1711.02635

zbMATH Keywords

inflationprimordial gravitational waves (theory)

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (16)

Inflation with multiple vector fields and non-Gaussianities ⋮ Primordial stochastic gravitational wave background anisotropies: in-in formalization and applications ⋮ Primordial tensor bispectra in μ-CMB cross-correlations ⋮ Probing a stationary non-Gaussian background of stochastic gravitational waves with pulsar timing arrays ⋮ Primordial tensor non-gaussianity from massive gravity ⋮ Gravitational wave anisotropies from primordial black holes ⋮ Doppler boosting the stochastic gravitational wave background ⋮ Squeezed tensor non-Gaussianity in non-attractor inflation ⋮ Tensor non-gaussianities from non-minimal coupling to the inflaton ⋮ Statistically anisotropic tensor modes from inflation ⋮ Probing the inflationary particle content: extra spin-2 field ⋮ Probing non-Gaussian stochastic gravitational wave backgrounds with LISA ⋮ A new mechanism to enhance primordial tensor fluctuations in single field inflation ⋮ Cross-correlations as a diagnostic tool for primordial gravitational waves ⋮ Small-scale tests of inflation ⋮ Probing parity-odd bispectra with anisotropies of GW V modes

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• Parity Violation of Gravitons in the CMB Bispectrum
• Possible signatures of the inflationary particle content: spin-2 fields
• Effective field theory of statistical anisotropies for primordial bispectrum and gravitational waves
• CMB scale dependent non-Gaussianity from massive gravity during inflation
• The Primordial Density Perturbation

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