Natural Ultralight Dark Matter: The Quadratic Twin
Cédric Delaunay, Michael Geller, Zamir Heller-Algazi, Gilad Perez, Konstantin Springmann
TL;DR
This work tackles the naturalness problem of ultralight dark matter (ULDM) with substantial quadratic couplings to the Standard Model by introducing a twin-Higgs-inspired mechanism. The ULDM is realized as a pseudo-Nambu-Goldstone boson whose mass corrections are protected by a mirror-$\mathbb{Z}_2$ symmetry between the SM and a twin SM, causing linear sensitivity to cancel and leaving leading mass shifts quadratic in the couplings. Explicit $U(1)$ and $U(2)$ constructions demonstrate how the mass corrections are highly suppressed, opening roughly $25$ orders of magnitude in the coupling-mass parameter space for $m_\phi$ in the range $\sim(10^{-20}-10^{-15})$ eV, within reach of clocks, interferometers, and future nuclear-clock probes. The framework predicts density-dependent effects with potential screening and gradient enhancements on Earth, providing concrete phenomenology for current and upcoming tabletop experiments, and it points to a rich cosmological history in the twin sector that warrants further study. Overall, the paper presents a natural, testable path to ULDM that is compatible with experimental sensitivities and offers new directions for early-Universe dynamics.
Abstract
Scalar ultralight dark matter (ULDM) is uniquely accessible to tabletop experiments such as clocks and interferometers, and its search has been the focus of a vast experimental effort. However, the scalar ULDM mass is not protected from radiative corrections, and the entirety of the parameter space within reach of experiments suffers from a severe naturalness problem. In this paper, we propose a new twin mechanism that protects the mass of the scalar ULDM. Our scalar ULDM is a pseudo-Nambu-Goldstone boson with quadratic couplings to the Standard Model (SM) and to a twin copy of the SM, with a mirror $\mathbb{Z}_2$ symmetry exchanging each SM particle with its twin. Due to the mirror symmetry, the leading-order mass correction is quadratic in the (tiny) coupling while the linear order is canceled. This opens up vast regions of parameter space for natural quadratically coupled ultralight dark matter, within the sensitivity of existing and future experiments.
