Constraints on Ultralight Scalar Dark Matter with Quadratic Couplings
Thomas Bouley, Philip S{\o}rensen, Tien-Tien Yu

TL;DR
This paper investigates how quadratically-coupled ultralight scalar dark matter influences Big Bang Nucleosynthesis predictions, providing new constraints on its properties by incorporating thermal mass effects and full kinetic equations.
Contribution
It introduces improved modeling of ultralight dark matter's impact on primordial element abundances, extending previous work to more general couplings and detailed cosmological evolution.
Findings
Big Bang Nucleosynthesis constrains ultralight dark matter with quadratic couplings over a wide mass range.
Thermal mass effects significantly alter dark matter evolution and BBN predictions.
Full kinetic treatment refines the predicted Helium-4 abundance.
Abstract
Ultralight dark matter is a compelling dark matter candidate. In this work, we examine the impact of quadratically-coupled ultralight dark matter on the predictions of Big Bang Nucleosynthesis. The presence of ultralight dark matter can modify the effective values of fundamental constants during Big Bang Nucleosynthesis, modifying the predicted abundances of the primordial elements such as Helium-4. We improve upon the existing literature in two ways: firstly, we take into account the thermal mass acquired by the ultralight dark matter due to its quadratic interactions with the Standard Model bath, which affects the cosmological evolution of the dark matter. Secondly, we treat the weak freeze-out using the full kinetic equations instead of using an instantaneous approximation. Both improvements were shown to impact the Helium-4 prediction in the context of universally-coupled dark…
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