Tree-level scalar correlators with massive scalar exchange in quasi-single-field inflation

This domain is quasi-single-field inflation and its descendants: primordial scalar correlators are modified by an extra scalar with mass of order the Hubble scale, typically through mixing with the inflaton or curvature mode. The field was anchored by arXiv:0911.3380, which defined the core physics of Hubble-mass isocurvature modes generating intermediate-shape non-Gaussianity and potentially large trispectra. For doing calculations, the most useful starting point is arXiv:1703.10166, which turns the in-in formalism into practical Schwinger-Keldysh rules and shows how mixed propagators simplify tree-level exchange calculations. Later work broadens the toolkit: bootstrap and Mellin-space methods give analytic constraints and closed forms for exchange correlators; differential-equation and flow methods systematize general trees and numerics; recent papers extend to multiple exchanges, dynamical masses, boost breaking, and data-facing templates. For this briefing, the foundation paper is the historical/domain anchor, while the best reference paper is the primary paper to read before proposing new calculations or ideas.

Task Focus for Idea Generation

Key Papers

Methodology

Known Solved Cases

Use these solved cases as examples of strong research form, not as new ideas. Do not propose a solved case itself as the core deliverable unless the proposal adds a genuinely new scientific component with substantial impact.

Open Axes for New Work

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