Exact Solutions for Chiral Gravitational Waves from Spin-2 Mixing
gr-qc, astro-ph.CO, hep-ph, hep-th
Submitted: 2026-09-26
Updated: 2026-09-26
Comments: 13 pages, 3 figures
License: http://creativecommons.org/licenses/by/4.0/
The gist: A spectator spin-2 field can mix linearly with the metric tensor perturbations.
Terminology
Abstract
A spectator spin-2 field can mix linearly with the metric tensor perturbations. We study the coupled tensor system in an inflationary background, including a parity violating effect parametrised by θ. Without expanding in the linear mixing between the two fields, we solve the system exactly for arbitrary mass while treating the mixing strength nonperturbatively. The mode functions of both helicities are constructed by acting with an operator-valued Gauss hypergeometric function 2F 1 on Whittaker modes, and the late-time power spectrum of each graviton helicity is expressed in closed form in terms of the generalised hypergeometric function 3F 2. We find that one helicity is exponentially enhanced, showing that strong mixing with a spectator spin-2 field can generate a large and highly chiral primordial gravitational wave spectrum. The degree of circular polarisation is bounded by (πθ), independently of the spin-2 mass and the mixing strength. The same solution also gives the late-time power spectrum of the spectator field and its cross spectrum with the graviton. In the weak mixing limit, our exact result reproduces the perturbative Schwinger-Keldysh result. These solutions provide a nonperturbative framework for studying primordial gravitational waves sourced by additional tensor modes.
Sources
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
- Planck 2018 results. X. Constraints on inflation
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- Signatures of Supersymmetry from the Early Universe
- Effective field theory approach to quasi-single field inflation and effects of heavy fields
- Cosmological Collider Physics
- Non-Gaussianity as a Particle Detector
- Resummation of Massive Gravity
- Theoretical Aspects of Massive Gravity
- Massive Gravity
- Bimetric Gravity from Ghost-free Massive Gravity
- Interacting Spin-2 Fields
- Ghostfree quadratic curvature theories with massive spin-2 and spin-0 particles
- Cosmological Perturbation Theory in Metric-Affine Gravity
- Gauge-flation: Inflation From Non-Abelian Gauge Fields
- Non-Abelian Gauge Field Inflation
- Chromo-Natural Inflation: Natural inflation on a steep potential with classical non-Abelian gauge fields
- Gauge Fields and Inflation
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