Dark-pion dark matter beyond leading order: unitarized chiral dynamics
Yuki Watanabe

TL;DR
This paper investigates how unitarization techniques modify dark pion scattering amplitudes beyond leading order, revealing resonance effects that significantly impact dark matter phenomenology in SIMP and WIMP models.
Contribution
It applies the chiral unitary method to dark pions, showing the emergence of resonance poles and their effects on dark matter interactions beyond leading order.
Findings
Resonance poles appear in unitarized amplitudes, absent at leading order.
Unitarization significantly alters dark pion self-scattering and annihilation rates.
Parameter space for dark matter models is notably affected by these nonperturbative effects.
Abstract
Dark pions are promising dark matter candidates, yet most analyses rely on leading-order (LO) chiral perturbation theory (ChPT). Motivated by the fact that, even for QCD pi-pi scattering, LO ChPT near threshold underestimates the isoscalar s-wave amplitude by an O(1) factor relative to high-precision dispersive results, we quantify how unitarization modifies the standard LO ChPT picture using the chiral unitary method, a nonperturbative resummation that implements the correct analytic structure with minimal input, and assess its impact on the phenomenology of dark-pion dark matter, taking SIMP and WIMP scenarios as canonical examples. We fix the subtraction constant to its natural estimate, interpreted as an effective cutoff at the chiral scale, so that the unitarized amplitudes depend only on the dark-pion mass and decay constant. We show that, depending on the coupling, the unitarized…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Quantum Chromodynamics and Particle Interactions · Particle physics theoretical and experimental studies
