Abstract

The current paradigm for dark matter direct detection is to assume that the dark sector is solely composed of a single particle species. In this short paper, we make the observation that dark matter comprising both a light and a heavy component that modulate out of phase leads to interesting phenomenology in annual modulation experiments. For an illustrative example, we use the recently released DAMA/LIBRA phase-2 results with a lower energy threshold. Immediately after, it was argued that a one-component spin-independent dark matter explanation of the observed annual modulation is strongly disfavored or excluded unless isospin-violating couplings are invoked. We show that a simple two-component extension can reproduce the observed spectrum without the need to invoke fine-tuned couplings. Using the publicly available DAMA/LIBRA data, we perform a fit of the DAMA/LIBRA energy spectrum of the annual modulation amplitude to a scenario with two dark matter components. We also take into account how gravitational focusing affects the phases of the light and a heavy components differently, which leads to nontrivial effects in the total time-dependent rate. Our results show that there exists a unique solution in agreement with the data in the simplest case of isospin-conserving couplings with equal cross sections. The distinctive features found in this work are crucial for a dark matter interpretation of any observed annual modulation.

Highlights

  • Dark matter (DM) is one of nature’s greatest enigmas

  • Since gravitational focusing (GF) does not affect the sinusoidality of the DAMA signal for DM masses below ∼30 GeV, we find that the light solution is excluded at 5.4σ, which is roughly the same significance as observed in previous studies

  • We have studied how a simple 2DM can lead to interesting signals in annual modulation experiments

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Summary

INTRODUCTION

Dark matter (DM) is one of nature’s greatest enigmas. Until now, evidence for its existence has stemmed from its gravitational interactions. Heavy DM mass solutions mentioned above for vanilla isospin-conserving spin-independent (SI) interactions, even before considering its compatibility with other null-result experiments This is because below 2 keVee the direct detection rates for the two standard DM solutions behave very differently with decreasing recoil energy: the light DM gives rise to scatterings off iodine, increasing its rate significantly, while for the heavy DM (that scatters predominately off iodine), the modulation amplitude decreases, eventually giving rise to a phase flip. This was already pointed out in Ref.

DARK MATTER DIRECT DETECTION SIGNAL
Gravitational focusing and the nonsinusoidal signal
DAMA ENERGY SPECTRUM OF THE MODULATION AMPLITUDE
One-component dark matter fit
Two-component dark matter fit
CONCLUSIONS
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