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Searching for Fossil Fields in the Gravity Sector

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arxiv 1906.07204 v1 pith:5U7OVFT3 submitted 2019-06-17 astro-ph.CO gr-qchep-phhep-th

Searching for Fossil Fields in the Gravity Sector

classification astro-ph.CO gr-qchep-phhep-th
keywords tensorscalesanisotropiesextrafieldsaccessibleacrossanisotropy
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Evidence for the presence of extra fields during inflation may be found in the anisotropies of the scalar and tensor spectra across a vast range of scales. Indeed, beyond the single-field slow-roll paradigm, a long tensor mode can modulate the power spectrum inducing a sizable quadrupolar anisotropy. We investigate how this dynamics plays out for the tensor two-point correlator. The resulting quadrupole stores information on squeezed tensor non-Gaussianities, specifically those sourced by the extra field content and responsible for the breaking of so-called consistency relations. We underscore the potential of anisotropies as a probe of new physics: testable at CMB scales through the detection of B-modes, they are accessible at smaller scales via interferometers and pulsar timing arrays.

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Cited by 3 Pith papers

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    astro-ph.CO 2026-05 unverdicted novelty 6.0

    PTA statistical tests cannot distinguish Gaussian and non-Gaussian GWB amplitude distributions in a model-agnostic way after decorrelation.

  3. Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order

    astro-ph.CO 2025-05 unverdicted novelty 6.0

    Extends diagrammatic approach for scalar-induced gravitational waves to arbitrary-order local PNG, deriving semi-analytic spectra for energy density, anisotropies, bispectrum and trispectrum up to quartic terms.