The Scalar Chemical Potential in Cosmological Collider Physics
Arushi Bodas, Soubhik Kumar, Raman Sundrum

TL;DR
This paper proposes a novel mechanism using a derivative coupling with a chemical potential to produce heavy scalar particles during inflation without exponential suppression, enabling potential detection through non-Gaussian bispectrum signals.
Contribution
It introduces a new chemical potential coupling that enhances heavy particle production during inflation, avoiding Boltzmann suppression and allowing for analytical bispectrum calculations.
Findings
Non-suppressed particle production for masses up to 10^{15} GeV.
Detectable bispectrum signals with f_NL ~ 0.01-10.
Analytical tree-level calculation of the bispectrum.
Abstract
Non-analyticity in co-moving momenta within the non-Gaussian bispectrum is a distinctive sign of on-shell particle production during inflation, presenting a unique opportunity for the "direct detection" of particles with masses as large as the inflationary Hubble scale (). However, the strength of such non-analyticity ordinarily drops exponentially by a Boltzmann-like factor as masses exceed . In this paper, we study an exception provided by a dimension-5 derivative coupling of the inflaton to heavy-particle currents, applying it specifically to the case of two real scalars. The operator has a "chemical potential" form, which harnesses the large kinetic energy scale of the inflaton, , to act as an efficient source of scalar particle production. Derivative couplings of inflaton ensure radiative stability of the slow-roll potential, which in turn…
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