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arXiv:2602.19958·v3·High Energy Physics — Phenomenology

Leptophilic scalar dark matter in U(1): Evading direct detection and prospective neutron star heating

Chengfeng Cai🇨🇳 · Hong-Hao Zhang🇨🇳

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Abstract

Leptophilic dark matter (DM) is a well-motivated thermal weakly interacting massive particle framework that can evade stringent nuclear-recoil searches while remaining testable via DM-induced heating of neutron stars (NSs). In this work, we study leptophilic scalar DM in a gauge extension of the Standard Model, which provides a common leptophilic portal for all scenarios considered. To reproduce the observed relic abundance while suppressing direct-detection signals, we investigate three benchmark realizations: (i) a secluded DM scenario in which the relic density is set by annihilation into gauge bosons and two pseudo-Nambu-Goldstone boson (pNGB) DM models based on (ii) an symmetry and (iii) an symmetry. In the pNGB model, the DM mass arises at tree level from a soft breaking term, while the elastic scattering amplitude is suppressed by a symmetry-protected cancellation. In the pNGB model, the DM mass is generated radiatively at one loop via the gauge interaction, and we show that this gauging preserves the same cancellation mechanism, maintaining compatibility with direct-detection null results. We perform a systematic parameter scan imposing relic density, direct and indirect detection, and neutrino trident constraints and identify viable sub-TeV to TeV DM candidates. Under the optimistic maximal-heating assumption that the capture rate reaches the geometric limit and that the captured DM population efficiently thermalizes and attains capture-annihilation equilibrium inside NSs, we find that the remaining parameter space can be tested by near-infrared observations of old NSs, providing sensitivity complementary to terrestrial searches in regions that are currently weakly constrained.

Comments: 38 pages, 7 figures. Added appendix A. Updated formulas and figures

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