Solar Capture Tests of Inelastic Dark Matter after the LZ High-Recoil Event

Abstract

The LUX-ZEPLIN (LZ) Collaboration has reported a $248$ keV nuclear-recoil candidate for which endothermic dark matter (DM) gives some of the largest local significances. We study Solar-capture constraints on three interpretations: a thermal Higgsino, a thermal pseudo-Dirac fermion with off-diagonal vector interactions, and neutron-philic endothermic spin-dependent scattering through ${\mathcal{O}}_4$. The canonical full-density thermal Higgsino is excluded: its LZ-preferred splitting near $0.38\mathrm{MeV}$ lies well below the splitting required to suppress Solar capture sufficiently to satisfy the IceCube upper limits on DM annihilation in the Sun, $\delta \gtrsim 0.51$-$0.56\mathrm{MeV}$. For the pseudo-Dirac benchmark parameters that fit the LZ event, we find $C_{\odot }=1.53\times 10^{20}{\mathrm{s}}^{-1}$, while two-state kinetics limits the fixed-orbit annihilation rate to ${\Gamma }_A\lesssim 4.4\times 10^{14}{\mathrm{s}}^{-1}$, about $1.7\times 10^5$ below the IceCube upper limit for the $b\bar{b}$ channel. A semi-analytic treatment indicates that re-excitation cycles further cool the captured population, although a full phase-space calculation is required for its final distribution. For neutron-philic ${\mathcal{O}}_4$ scattering at $m_{\chi }=1$ TeV and $\delta =300$ keV, finite-temperature capture gives $C_{\odot }=3.98\times 10^{17}{\mathrm{s}}^{-1}$, with nuclear-structure uncertainties giving an envelope $(1.77$-$9.72)\times 10^{17}{\mathrm{s}}^{-1}$. Under the equilibrium assumption, the upper edge remains about a factor $154$ below the IceCube upper limit for the $b\bar{b}$ channel. We use $b\bar{b}$ only as a soft-hadronic proxy because an exact constraint requires the model-specific annihilation spectrum. Solar capture therefore excludes the thermal-Higgsino interpretation but not endothermic explanations generically.

arXiv comment43 pages, 14 figures and 3 tables. Comments are welcome