
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.
7 pages, 2 figure
High Energy Physics - Theory, ST/S000550/1, Cosmology and Nongalactic Astrophysics (astro-ph.CO), RCUK, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Physics and Astronomy(all), General Relativity and Quantum Cosmology, ST/P00055X/1, High Energy Physics - Phenomenology, High Energy Physics - Phenomenology (hep-ph), High Energy Physics - Theory (hep-th), /dk/atira/pure/subjectarea/asjc/3100, STFC, Astrophysics - Cosmology and Nongalactic Astrophysics
High Energy Physics - Theory, ST/S000550/1, Cosmology and Nongalactic Astrophysics (astro-ph.CO), RCUK, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Physics and Astronomy(all), General Relativity and Quantum Cosmology, ST/P00055X/1, High Energy Physics - Phenomenology, High Energy Physics - Phenomenology (hep-ph), High Energy Physics - Theory (hep-th), /dk/atira/pure/subjectarea/asjc/3100, STFC, Astrophysics - Cosmology and Nongalactic Astrophysics
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